<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">JMF</journal-id><journal-title-group><journal-title>Journal of Mathematical Finance</journal-title></journal-title-group><issn pub-type="epub">2162-2434</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jmf.2014.43017</article-id><article-id pub-id-type="publisher-id">JMF-46378</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>BUSINESS &amp; ECONOMICS</subject><subject>PHYSICS &amp; MATHEMATICS</subject></subj-group></article-categories><title-group><article-title>Multi-Name Extension to the Credit Grades and an Efficient Monte Carlo Method</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Hideyuki</surname><given-names>Takada</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Department of Information Science, Toho University, Chiba, Japan</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>hideyuki.takada@is.sci.toho-u.ac.jp</email></corresp></author-notes><pub-date pub-type="epub"><day>22</day><month>04</month><year>2014</year></pub-date><volume>04</volume><issue>03</issue><fpage>188</fpage><lpage>206</lpage><history><date date-type="received"><day>4</day>	<month>March</month>	<year>2014</year></date><date date-type="rev-recd"><day>11</day>	<month>April</month>	<year>2014</year>	</date><date date-type="accepted"><day>3</day>	<month>May</month>	<year>2014</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
	In this paper, we present a multi-name incomplete information structural model which possess the contagion mechanism and its efficient Monte Carlo algorithm based on Interacting Particle System. Along with the Credit Grades, which is industrially used single-name credit model, we suppose that investors can observe firm values and defaults but are not informed of the threshold level at which a firm is deemed to default. Additionally, in order to model the possibility of crisis normalization, we introduce the concept of memory period after default. During the memory period after a default, public investors remember when the previous default occurred and directly reflect that information for updating their belief. When the memory period after a default finish, investors forget about that default and shift their interest to recent defaults if exist. One of the variance reduction techniques, relying upon Interacting Particle System, is combined with the standard Monte Carlo method to address the rare but critical events represented by the tail of loss distribution of portfolio. 
</p></abstract><kwd-group><kwd>Credit Risk</kwd><kwd> Default Contagion</kwd><kwd> Monte Carlo Method</kwd><kwd> Interacting Particle System</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Interaction of default events play a central role for systemic risk measurement as well as the credit risk manage- ment and portfolio credit derivative valuation. Recent financial crisis has revealed a necessity of quantitative methodology to analyze default contagion effects which are observed in several financial markets. Default contagion is a phenomenon where a default by one firm has direct impact on the health of other surviving firms. Since the contagion effects heavily influence the correlations of defaults, capturing them in quantitative models is crucial. Existing dynamic credit risk models which deal with default contagion include, among others, Davis and Lo [<xref ref-type="bibr" rid="scirp.46378-ref1">1</xref>] , Fan Yu [<xref ref-type="bibr" rid="scirp.46378-ref2">2</xref>] , Frey and Backhaus [<xref ref-type="bibr" rid="scirp.46378-ref3">3</xref>] , Frey and Runggaldier [<xref ref-type="bibr" rid="scirp.46378-ref4">4</xref>] , Giesecke [<xref ref-type="bibr" rid="scirp.46378-ref5">5</xref>] , Giesecke and Goldberg [<xref ref-type="bibr" rid="scirp.46378-ref6">6</xref>] , Giesecke et al. [<xref ref-type="bibr" rid="scirp.46378-ref7">7</xref>] , Sch&#246;nbucher [<xref ref-type="bibr" rid="scirp.46378-ref8">8</xref>] , Takada and Sumita [<xref ref-type="bibr" rid="scirp.46378-ref9">9</xref>] and comprehensive surveys can be found in Chapter 9 of McNeil, Frey and Embrechts [<xref ref-type="bibr" rid="scirp.46378-ref10">10</xref>] . Generally, credit risk modeling methodologies are categorized to either reduced form approach or structural approach. In the reduced form approach, by introducing interacting intensities, default contagion can be captured by the jump up of the default intensity immediately after the default as in Davis and Lo [<xref ref-type="bibr" rid="scirp.46378-ref1">1</xref>] , Fan Yu [<xref ref-type="bibr" rid="scirp.46378-ref2">2</xref>] , Frey and Backhaus [<xref ref-type="bibr" rid="scirp.46378-ref3">3</xref>] , Giesecke et al. [<xref ref-type="bibr" rid="scirp.46378-ref7">7</xref>] and Takada and Sumita [<xref ref-type="bibr" rid="scirp.46378-ref9">9</xref>] . However, it is not easy to incorporate the mechanism where the crisis mode would resolve after some period. Information based default contagion described in Chapter 9 of McNeil, Frey and Embrechts [<xref ref-type="bibr" rid="scirp.46378-ref10">10</xref>] and Frey and Runggaldier [<xref ref-type="bibr" rid="scirp.46378-ref4">4</xref>] might be promising methods that allow to represent normalization of crisis via belief updating, however, explicit formulation of normalization and its effects to future defaults are not thoroughly studied. On the other hand, Giesecke [<xref ref-type="bibr" rid="scirp.46378-ref5">5</xref>] and Giesecke and Goldberg [<xref ref-type="bibr" rid="scirp.46378-ref6">6</xref>] have studied multi-name structural model under incomplete information and proposed a simulation method for sequential defaults without covering the explicit formulation of normalization. Unfortunately, since the closed formula for joint distribution of the first-passage time of correlated multivariate Brownian motion is unknown, the proposed algorithms therein are not directly applicable to correlated firm value cases.</p><p>In this paper, we present a multi-name incomplete information structural model which possess a default contagion mechanism in the sense that the sudden change of default probabilities arise from the investors’ revising their perspectives towards unobserved factors which characterize the joint density of default thresholds. Here, in our model, default thresholds are assumed to be unobservable from public investors and a firm is deemed to default when firm value touch this level of threshold for the first time. This formulation is a slight generalization of Giesecke and Goldberg [<xref ref-type="bibr" rid="scirp.46378-ref6">6</xref>] . Also, to analyze the contagion effects under general settings, we consider the dependence structure of firm value dynamics as well as the joint distribution of default thresholds. Additionally, in order to model the possibility of crisis normalization, we introduce the concept of memory period after default. A preliminary version of this study is reported at RIMS Workshop on Financial Modeling and Analysis (FMA2013) by Takada [<xref ref-type="bibr" rid="scirp.46378-ref11">11</xref>] which introduced the concept of memory period first. As Takada [<xref ref-type="bibr" rid="scirp.46378-ref11">11</xref>] pointed out, the model is designed so as to confine investors’ attention to the recent defaults. During the memory period after a default, public investors remember when the previous default occurred and directly reflect that information for updating their belief. When the memory period after a default terminate, investors attach little importance to that default and shift their interest to recent defaults if exist. When all the existing memory periods terminate, we can consider the situation as a complete return to the normal economic condition. In order to evaluate the credit risk under the presence of the default contagion and possibilities of normalization, Monte Carlo simulation is the most reasonable method because of their non Markovian environment. However, the previous study, relying on standard Monte Carlo method, performed slow convergence. We examine that the Interacting Particle System (IPS) is a powerful tool to overcome the slow convergence. Intuitively, Interacting Particle System works in a following mechanism. On a discrete time grid, IPS evolves a collection of particles representing the states of our interest, including firm values. At each time step, particles are randomly selected by sampling with replacement, placing more weight on particles that experienced increase in default probability in the previous period. The new generation of selected particles is then evolved over the next period based on the standard transition lows and at the end of the period a selection takes place again. The selection procedure adaptively forces the process into the regime of interest and therefore reduces variance.</p><p>The rest of this paper is organized as follows. Section 2 introduce our model and deduces an expression for the conditional joint distribution of the default thresholds. Section 3 develops standard Monte Carlo simulation algorithm. Section 4 gives an overview of Feynman-Kac path measure which plays a central role of the Interacting Particle System and how the algorithm can be applied to the model. Section 5 provides numerical examples and Section 6 concludes.</p></sec><sec id="s2"><title>2. Incomplete Information Credit Risk Model</title><p>Uncertainty is modeled by a probability space <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\966d1211-b498-474f-bce8-6093590ef1c5.png" xlink:type="simple"/></inline-formula> equipped with a filtration <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\26fee22d-1a1e-4945-b428-a64e6a312ce3.png" xlink:type="simple"/></inline-formula> that describes the</p><p>information flow over time. We impose two additional technical conditions, often called the usual conditions. The first is that <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\48e3f2ff-3f76-4715-b6f2-b2fee180d393.png" xlink:type="simple"/></inline-formula> is right-continuous and the second is that <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\70b423d5-e97b-4afa-927e-6dec5572bb06.png" xlink:type="simple"/></inline-formula> contains all <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\71d98fbe-6737-4e5d-8649-8d2169cf8be6.png" xlink:type="simple"/></inline-formula>-null sets, meaning that one can always identify a sure event. Without mentioning it again, these conditions will be imposed on every filtration that we introduce in the sequel. The probability measure <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\98ba5832-fcd2-44ae-a82e-a001427f248e.png" xlink:type="simple"/></inline-formula> serve as the statistical real world measure in risk management applications, while in derivatives pricing applications, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\315a6267-4a11-4ca0-bb44-9f9a43fb194d.png" xlink:type="simple"/></inline-formula>is a risk-neutral pricing measure. On the financial market, investors can trade credit risky securities such as bonds and loans issued by several firms indexed by<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\64cdd94d-bbb0-4a04-8b45-bf5f52b159f3.png" xlink:type="simple"/></inline-formula>. In the following, we extend the CreditGrades model in the sense that we consider more than two firms in the portfolio and their asset correlation as well as the dependence structure of the default barriers. Furthermore, we give a slight modification of the CreditGrades model reflecting the fact that the surviving firm’s default barrier is lower than its historical path of asset value.</p><sec id="s2_1"><title>2.1. Model Setting</title><p>Let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\9e4254e8-c378-45dd-8326-41aaf8027c09.png" xlink:type="simple"/></inline-formula> represent the time <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\b9b24fed-7066-4f76-bbe7-934fae8ef6ab.png" xlink:type="simple"/></inline-formula> asset value of the firm <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\747dd38b-60df-4ce8-aa53-9b6246ed97b6.png" xlink:type="simple"/></inline-formula> on a per share basis which solves the</p><p>next stochastic differential equation</p><disp-formula id="scirp.46378-formula1"><label>(0.1)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\383bcafa-b6b9-4496-b64d-f9a64ed71961.png"/></disp-formula><disp-formula id="scirp.46378-formula2"><label>(0.2)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\ac405414-76b8-43a9-836f-8450bddefb25.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\da9094df-8377-4798-b8c2-8288d34de364.png" xlink:type="simple"/></inline-formula> is the asset volatility and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3356f846-ff7c-4f22-b154-556ab94f3e56.png" xlink:type="simple"/></inline-formula> is the firm value at time 0 at which we stand. We assume that the</p><p>asset value processes have correlations, i.e., <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\76e993cc-d50f-49ff-ae2e-19fd9b38bdf4.png" xlink:type="simple"/></inline-formula>, where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\0eee1dd7-375c-4b14-a9bb-777a0852c273.png" xlink:type="simple"/></inline-formula> is the quadratic</p><p>covariation. Filtrations generated by observed asset values are denoted by<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\b2d890c2-199d-4592-814c-77977c3d1f6d.png" xlink:type="simple"/></inline-formula>. There is a</p><p>random default threshold <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\8172c9ca-25df-4181-aa48-002e8c4058ed.png" xlink:type="simple"/></inline-formula> such that firm <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\172a7f65-284f-472b-ba63-fabccab0e9ee.png" xlink:type="simple"/></inline-formula> default as soon as the asset value falls to the level<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\4fe94a84-749a-4e6b-a5d6-f7c8467ba245.png" xlink:type="simple"/></inline-formula>, where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\1d2768bd-42f6-421e-9065-f73baa69a798.png" xlink:type="simple"/></inline-formula> denotes the recovery rate at default and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\c5f5481f-729f-43a6-ad1a-f8f2e7871748.png" xlink:type="simple"/></inline-formula> is a positive constant representing debt per share, which may given by accounting reports. Then the default time of the firm <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\a248e8e3-6aff-41b2-9b07-1a01b929d597.png" xlink:type="simple"/></inline-formula> is a random variable <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\ccf1b986-1864-400a-99a4-1658c3b6aecf.png" xlink:type="simple"/></inline-formula> given by</p><disp-formula id="scirp.46378-formula3"><label>(0.3)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\97ca1fda-75e6-4c2e-8fba-98487d145d41.png"/></disp-formula><p>Here random variables <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\0e356868-d68c-44de-b31d-0f9ba5f997be.png" xlink:type="simple"/></inline-formula> are mutually independent of the<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\941ff856-7445-4a60-9db6-1f93ee6f6bae.png" xlink:type="simple"/></inline-formula>. More complicated stochastic processes for <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\97ac28a3-c054-47ec-9872-59878836c93f.png" xlink:type="simple"/></inline-formula> such as stochastic volatility may be possible, however, we shed</p><p>lights to the multi-name setting and model the so-called default contagion. Let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\599e6aaf-e3bf-4c47-a62b-912956c2323a.png" xlink:type="simple"/></inline-formula> be a right-continuous</p><p>process which indicate the default status of the firm <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\93f69959-f2ea-4791-8410-9154e57e9dc8.png" xlink:type="simple"/></inline-formula> at time <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\a01cb2ab-ea69-437c-b35a-913696724212.png" xlink:type="simple"/></inline-formula> and we denote by <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\1e14ad64-b720-44f8-a7e9-f6969bb26842.png" xlink:type="simple"/></inline-formula> the associated filtration.</p></sec><sec id="s2_2"><title>2.2. Incomplete Information</title><p>With the view to analyzing how the period of past default memories affect succeeding defaults, we consider the incomplete information framework which is known to represent default contagion. In order to depict the incomplete information structure more concretely, in addition to the assumption of the randomness of the default threshold, we postulate the following assumptions.</p><p>Assumption 1 Public investors can observe firm values and default events although they can not directly</p><p>observe the firm’s default thresholds <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\fde01591-6826-469d-a97e-e6645b8209ff.png" xlink:type="simple"/></inline-formula> except for the default time<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\75e59f31-f685-431b-9b33-c960dc06dd6b.png" xlink:type="simple"/></inline-formula>.</p><p>Define the set of survived firms <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\d323bf94-cf7a-48bf-8bcb-1b835b4f1327.png" xlink:type="simple"/></inline-formula> and the set of defaulted firms</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\e3fd4b07-0245-4b1e-946b-d1a7ad6c7528.png" xlink:type="simple"/></inline-formula>at the time<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\85514727-6e7c-444b-a453-fa98d201e801.png" xlink:type="simple"/></inline-formula>. We write<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\ffd95e30-2779-43cf-9714-27996ea01589.png" xlink:type="simple"/></inline-formula>, the number of elements in the set<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\1dcdb45a-0ca8-4a8e-8272-0972e6ef92ae.png" xlink:type="simple"/></inline-formula>. Since</p><p>investors have knowledge that the surviving firms have lower default barrier than their running minimum of the firm value processes, it is natural to suppose the next assumption.</p><p>Assumption 2 At time<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\eb888ed4-402d-48d4-bd21-b3969b580f2f.png" xlink:type="simple"/></inline-formula>, we assume every firm in the portfolio are surviving, i.e., <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\d5c8d710-0787-4de6-a675-585049894069.png" xlink:type="simple"/></inline-formula>and then the</p><p>inequality <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\e89807be-d2b5-445a-a20a-2bd4983b04db.png" xlink:type="simple"/></inline-formula> holds for all <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\789edbfb-b171-44e6-875c-fddb42b59ba2.png" xlink:type="simple"/></inline-formula> under the condition<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\bb17b7d1-c3f0-44cc-8415-7f0b715cd8e9.png" xlink:type="simple"/></inline-formula>.</p><p>Let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\f7394d3d-0fd9-4ae9-8eb1-016a50d87ea1.png" xlink:type="simple"/></inline-formula> be normally distributed random variable with mean vector</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\43506ac2-d659-4436-8b7c-f39e2da16fe9.png" xlink:type="simple"/></inline-formula>and variance-covariance matrix<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5abdf3d1-02d4-454e-9e76-e6cd75149041.png" xlink:type="simple"/></inline-formula>. Here, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\31b95668-0245-4cfd-a1d9-a135cc5a0613.png" xlink:type="simple"/></inline-formula>, are</p><p>some constants. And we assume that <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\da5ea0ec-f380-4e08-8e33-3471a4201e18.png" xlink:type="simple"/></inline-formula> be the truncation of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\2c1e216a-bd3b-4929-80d0-88252aa0cd9b.png" xlink:type="simple"/></inline-formula> above</p><p><img src="htmlimages\5-1490275x\db821250-4663-423e-b94e-fe04003caa3a.png" width="347.874984741211" height="54.1249990463257" />. We denote<img src="htmlimages\5-1490275x\8daacc84-2dac-4234-8347-71bf57d32b10.png" width="112.624998092651" height="54.1249990463257" />.</p><p>Remark 1 The definition of the mean vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\a71b469a-6148-4e65-8a1a-c9512135fea7.png" xlink:type="simple"/></inline-formula> is given along the line of</p><p>original CreditGrades model. Finger, Finkelstein, Pan, Lardy and Ta [<xref ref-type="bibr" rid="scirp.46378-ref12">12</xref>] proposed that the random recovery</p><p>rate <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5a39f88a-1a53-42d8-9be4-4cb3ccaf2789.png" xlink:type="simple"/></inline-formula> is modeled as <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\9ed848f0-4e83-44d8-84da-67deadd44a52.png" xlink:type="simple"/></inline-formula> with<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\a930bc19-b8a5-428e-a75f-cf07ffd611ba.png" xlink:type="simple"/></inline-formula>, where<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\df46f323-4e10-46c8-9833-7e6e3934043f.png" xlink:type="simple"/></inline-formula>.</p><p>Assumption 3 There is a consensus on the prior joint distribution of firm’s default thresholds among the public investors. More concretely, investor’s uncertainty about the default thresholds <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7496f7fc-d7bf-4370-8423-2dacf97590af.png" xlink:type="simple"/></inline-formula> is expressed by</p><disp-formula id="scirp.46378-formula4"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5635c5c1-a679-4519-ab4e-fdaef8d29929.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7de51be0-4300-4b16-9b86-7bf096d7d63b.png" xlink:type="simple"/></inline-formula> is a <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\b0237e79-f5be-4a1a-96a8-5dc65f233546.png" xlink:type="simple"/></inline-formula>-dimensional Normal distribution.</p><p>Assumption 4 For each default time<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\15e0cb3e-8227-43a5-bd0a-6be9e9cfa753.png" xlink:type="simple"/></inline-formula>, public investors update their belief on the joint distribution function of surviving firm’s default thresholds based on the Assumption 3 and newly arrived information, i.e., the realized recovery rate<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\2b59e489-4e78-4cba-8ff6-1b9128c58344.png" xlink:type="simple"/></inline-formula>.</p><p>Remark 2 Since public investors observe all the history of the firm value, they know that the unobservable threshold should be located below the running minimum of the firm value. Despite these knowledge, we assume that public investors treat the logarithm of the recovery rate <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\9e757b50-6f3d-4e79-9444-69910491d045.png" xlink:type="simple"/></inline-formula> as normally distributed random variable.</p><p>Assumption 1, Assumption 3 and Assumption 4 provide the default contagion mechanism; The default of a firm reveals information about the default threshold and then public investors update their beliefs on surviving firm’s joint distribution of thresholds. From public investors’ perspective, this naturally causes the sudden change of default probabilities of survived firms, which is just what we wanted to model. The situation of contagious defaults can be translated to the recession, however, it will not continue forever. In our model, we further assume that public investors view the crisis will return to normal condition after some finite time interval.</p><p>Assumption 5 The covariance parameter jumps from <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\6fef8b0b-3820-4910-9610-2b5831e1a313.png" xlink:type="simple"/></inline-formula> to <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\780fc879-30b8-429b-8fe3-1a9dc3dc5a2f.png" xlink:type="simple"/></inline-formula> at time <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\0c45d404-1fa6-4d7f-ac00-93edcd0df171.png" xlink:type="simple"/></inline-formula> for some</p><p>constants <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\56fadd90-4d33-47c6-9434-04b6c9e3f1cf.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\6b5a57b3-daba-430f-b190-9663c6f9e35b.png" xlink:type="simple"/></inline-formula>. This can be captured by introducing time-depending covariance parameters <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\bfe708db-578f-43a2-9c6e-b622b047d590.png" xlink:type="simple"/></inline-formula> defined as</p><disp-formula id="scirp.46378-formula5"><label>(0.4)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\d7d1bfbe-51d6-4754-b804-d12572243801.png"/></disp-formula><p>and then assume that the elements of the variance-covariance matrix <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\d9a6f9d9-546e-4c42-984f-bfd1426efe85.png" xlink:type="simple"/></inline-formula> are given by (0.4). We call <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\6706d50c-f5f4-40c6-9205-f2cb6f8c529c.png" xlink:type="simple"/></inline-formula> the memory period of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7a50986e-9c76-4e87-9229-1952c8e679da.png" xlink:type="simple"/></inline-formula> after<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\a9ed8a12-f134-4f64-afad-7402a1d94f4a.png" xlink:type="simple"/></inline-formula>.</p><p>Thus the mean vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\9bb71145-8cce-4465-911b-4ba5c4e2d740.png" xlink:type="simple"/></inline-formula> and the variance-covariance matrix <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7861e503-e52d-4b4f-8ed5-7e8c845ad11c.png" xlink:type="simple"/></inline-formula> at time <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\8d646ae6-7130-452e-91c4-ac41969f0ee6.png" xlink:type="simple"/></inline-formula> can be defined as</p><disp-formula id="scirp.46378-formula6"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\89aab414-2fb0-4d5f-94e9-b1e057a485f8.png"/></disp-formula><p>Assumption 6 <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\62f7992b-fc2e-441c-9548-12527ec3fbfb.png" xlink:type="simple"/></inline-formula> for<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\ef18f98e-b6ad-4106-b535-22154e8d9e95.png" xlink:type="simple"/></inline-formula>.</p><p>Define the set <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\741f1a62-65d3-4cf2-8fce-f2c520862328.png" xlink:type="simple"/></inline-formula> at time <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5d2788d6-27cd-44c6-91aa-1483c7074bf2.png" xlink:type="simple"/></inline-formula> and let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3aa3252b-3533-4abc-8c78-21afac6143c0.png" xlink:type="simple"/></inline-formula> be the number of</p><p>elements in the set<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\af65d3f1-c43b-4d46-9506-f171a851798b.png" xlink:type="simple"/></inline-formula>. Rearrange the order of firm identity numbers in such a way that the elements of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5462858f-874b-4386-a078-ea249f94b1f3.png" xlink:type="simple"/></inline-formula></p><p>come after the elements of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\56b565bc-2cee-485c-a615-a0471e06d99b.png" xlink:type="simple"/></inline-formula> and the elements of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\44512a71-15a6-46ab-8e6e-e4e57563c086.png" xlink:type="simple"/></inline-formula> are located the last. Let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\6fe9e262-3396-46a2-a5b9-be28d0e9369b.png" xlink:type="simple"/></inline-formula> be a <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\9001f177-5c28-442f-89ab-54d01964767a.png" xlink:type="simple"/></inline-formula></p><p>submatrix formed by selecting the rows and columns from the subset <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\210f9c26-3095-424a-be6b-c1100c408258.png" xlink:type="simple"/></inline-formula> and let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\a68be258-c88d-49fb-bcf7-811c1bb67b9d.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\4cab7235-1eab-4682-9d63-c2507db21985.png" xlink:type="simple"/></inline-formula> be corres-</p><p>ponding <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\b5c8ad32-e5b2-4735-9d36-3dfe3284b047.png" xlink:type="simple"/></inline-formula>-dimensional vectors respectively.</p><disp-formula id="scirp.46378-formula7"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5d4c6de6-53fe-4b23-8088-b7dbec7f7444.png"/></disp-formula><disp-formula id="scirp.46378-formula8"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5d4c6de6-53fe-4b23-8088-b7dbec7f7444.png"/></disp-formula><p>Assumption 6 implies that during the memory period, public investors remember the firm values at which the defaults occurred. We note that</p><disp-formula id="scirp.46378-formula9"><label>(0.5)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\c0e32aa6-b191-4040-a485-dad2fa5fa871.png"/></disp-formula><p>By virtue of Assumption 3, we can deduce the conditional joint distribution of the default thresholds as follows. Here we don’t eliminate the possibility of simultaneous defaults, i.e., we don’t need to assume<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\b0a34190-97ac-48de-8f2f-da9b3a766480.png" xlink:type="simple"/></inline-formula>.</p><p>Proposition 1 Let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\60ef1d68-72b6-4bb5-8e20-0833e640f6b5.png" xlink:type="simple"/></inline-formula> be a <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\1598ac36-8546-4ca5-aca9-398f89ff2a34.png" xlink:type="simple"/></inline-formula>-dimensional vector consists of the logarithm of the realized recovery rate at time<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\666e0502-33bf-4655-a10d-019b3005af82.png" xlink:type="simple"/></inline-formula>. Partition the vector<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3826f400-2459-4d87-80c8-f05cfcb32074.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\18c7947b-d549-4bb3-96de-a34bea057be8.png" xlink:type="simple"/></inline-formula>and the matrix <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\2f0c8a3d-e0bc-4746-846d-465fdaf36007.png" xlink:type="simple"/></inline-formula> into</p><disp-formula id="scirp.46378-formula10"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\f9ee077a-763e-4926-bfed-fdcda071ebeb.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\e7d23bed-a30a-4eeb-a2a9-139e8027111a.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\608bbee3-ffc5-4b2d-b2f6-570126261603.png" xlink:type="simple"/></inline-formula> are <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\b5ecd060-e26a-44c8-ae9d-9247b7ab6355.png" xlink:type="simple"/></inline-formula> dimensional vectors, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\6643ac11-da4c-4ccd-8a41-6f54cc794442.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\f080c50f-a256-4408-ab3b-d88a7b98af3d.png" xlink:type="simple"/></inline-formula> are <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\8f8beb71-5c40-4d1c-a3b7-10beb0de0794.png" xlink:type="simple"/></inline-formula> dimensional vectors, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7f4c6e35-6adb-4bbd-95ff-22dcac8af61d.png" xlink:type="simple"/></inline-formula>is a</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\91dbf842-e696-4413-8ccb-d7914426ac6b.png" xlink:type="simple"/></inline-formula>matrix, and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7ece4f8e-84a2-42d3-9224-855266c87b99.png" xlink:type="simple"/></inline-formula> is a <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\6189fab1-5cfb-4e40-bccb-d456619d8828.png" xlink:type="simple"/></inline-formula> matrix. Then <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\8ed2142d-04be-4cc1-8ed1-2ed7f46338ba.png" xlink:type="simple"/></inline-formula>-conditional joint density of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5a7cd2a8-fe7b-4b29-8581-33c61c6d72bf.png" xlink:type="simple"/></inline-formula> is given by</p><disp-formula id="scirp.46378-formula11"><label>(0.6)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\adbc85b7-b296-44ff-aefc-10f268756361.png"/></disp-formula><p>where</p><disp-formula id="scirp.46378-formula12"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5788a033-ead9-4eb3-9c7b-9eca27526729.png"/></disp-formula><disp-formula id="scirp.46378-formula13"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5788a033-ead9-4eb3-9c7b-9eca27526729.png"/></disp-formula><disp-formula id="scirp.46378-formula14"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5788a033-ead9-4eb3-9c7b-9eca27526729.png"/></disp-formula><disp-formula id="scirp.46378-formula15"><label>(0.7)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7f2ba411-1bca-4efc-85de-ef2857fd62bc.png"/></disp-formula><p>Proof 1 From the continuity of the asset process <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\8120d640-2a90-4e2c-b9bf-c9498144fc4d.png" xlink:type="simple"/></inline-formula> and Equation (0.5), public investors know that</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3f8efcd7-689a-4431-b892-817612326f87.png" xlink:type="simple"/></inline-formula>for all defaulted firms <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\4b884e50-2b07-4341-9b99-2a93d90447f2.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\34af05b2-28b1-49f5-aa52-10747733bf98.png" xlink:type="simple"/></inline-formula> for all survived firms<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\1aa584a0-2b78-46c6-b222-75205df02262.png" xlink:type="simple"/></inline-formula>.</p><p>Here, whenever defaults occur, let the order of the firms be rearranged in such a way that the elements of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\842edcc9-aaa6-46be-8370-93d74c066007.png" xlink:type="simple"/></inline-formula> come after the elements of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3b03cbcb-0838-4704-a7f2-67969dfbd156.png" xlink:type="simple"/></inline-formula>. Define the set</p><disp-formula id="scirp.46378-formula16"><label>(0.8)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\e021ee34-ac2a-41e6-bd4a-9cbbfc653b60.png"/></disp-formula><disp-formula id="scirp.46378-formula17"><label>(0.9)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\b94cf3bf-6f03-4385-85d1-37b9ccaf2999.png"/></disp-formula><p>with the special case</p><disp-formula id="scirp.46378-formula18"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\dd3f99e7-ce84-4382-b80b-d97d6d9d603f.png"/></disp-formula><p>to be the possible range of the recovery rate vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7c304450-24a6-48ca-9954-e76c9f04d020.png" xlink:type="simple"/></inline-formula> under the condition of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\fa1d96a2-e57c-400c-a645-263f684d9757.png" xlink:type="simple"/></inline-formula>. In particular,</p><p>for<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\b7d07988-f652-4abf-9909-30e05c06399a.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\9c451477-a1a0-4227-ae8c-39b6eb20c4db.png" xlink:type="simple"/></inline-formula>takes value<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\2c91cad8-37e9-4e84-8d6c-6898c774bace.png" xlink:type="simple"/></inline-formula>. Let<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\37c24a4c-e304-47d6-a9d2-e8f8b8b24a78.png" xlink:type="simple"/></inline-formula>. As in the proof of the Lemma 4.1 of [<xref ref-type="bibr" rid="scirp.46378-ref5">5</xref>],</p><p>from Bayes’ Theorem,</p><disp-formula id="scirp.46378-formula19"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\627f901d-d53b-4ece-a6d2-2670b99925ac.png"/></disp-formula><p>The last equality holds because <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\1646799c-e618-437a-a163-f95981f7cfcd.png" xlink:type="simple"/></inline-formula> is independent of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\a75233c3-03ef-499e-9fdb-867d597c03ff.png" xlink:type="simple"/></inline-formula>. Hence the joint distribution of the surviving firm’s</p><p>logarithm of recovery rates are given by the conditional distribution of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\e839cd2f-b3e3-41f0-8f9e-161d8552d176.png" xlink:type="simple"/></inline-formula> given <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\ff04864a-f6c5-496d-881c-6f11488a51f6.png" xlink:type="simple"/></inline-formula> at which the realization</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\69cfcde7-c46d-4aa8-b896-a9bc4e69328a.png" xlink:type="simple"/></inline-formula>hold for all<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\d4fdd79e-644e-4de0-873f-0fafc2bda794.png" xlink:type="simple"/></inline-formula>. Conditional distributions of the multivariate normal distribution are</p><p>well known. See for example [<xref ref-type="bibr" rid="scirp.46378-ref13">13</xref>] for details. However, from Assumption 1, public investors have already know the following inequalities hold.</p><disp-formula id="scirp.46378-formula20"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\2adddeae-9f31-4cc9-9f01-df3334bd59e2.png"/></disp-formula><p>Therefore the conditional distribution <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\09f79369-2693-46a7-8dde-0f6c32f6a92c.png" xlink:type="simple"/></inline-formula> should be truncated above <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\22e38e3f-6983-42c6-9169-65308b3cd307.png" xlink:type="simple"/></inline-formula> given by (0.7).</p><p>Remark 3 In the case <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\0ed7a8db-1c11-4592-bc81-2d6a3b06e5a6.png" xlink:type="simple"/></inline-formula> for all<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5940bbec-1762-4507-a190-20336077e057.png" xlink:type="simple"/></inline-formula>, the problem become quite easy because first-passage time of 1-dimensional Geometric Brownian motion is well known. In fact, in such a case, Giesecke and Goldberg [<xref ref-type="bibr" rid="scirp.46378-ref6">6</xref>]</p><p>showed that the counting process <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\4493102f-dbe2-41cd-9e5f-06b3f84c2c04.png" xlink:type="simple"/></inline-formula> has intensity process and they proposed the simulation method</p><p>based on the total hazard with the case <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\0d6439be-cd0b-4229-91a9-73230a14d3b4.png" xlink:type="simple"/></inline-formula> are not observable.</p><p>Let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\715ecbe9-6bd5-4ce7-a129-7972dbd93d61.png" xlink:type="simple"/></inline-formula> be an ordered default times of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\adf39ce8-f488-49f3-93a3-2277d0ea7a74.png" xlink:type="simple"/></inline-formula>. <xref ref-type="fig" rid="fig1">Figure 1</xref> illustrate an example of sequence of</p><p>defaults with <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\88489655-bf3f-4001-8ef2-8568af52983e.png" xlink:type="simple"/></inline-formula> and the corresponding memory periods. At time 0, since all the firms are active and then</p><p>the unconditional joint density of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\963f2346-0673-4c83-9287-08bbeb43fe9e.png" xlink:type="simple"/></inline-formula> is given by</p><disp-formula id="scirp.46378-formula21"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\9b954088-fffc-49a2-b05a-439e32021eac.png"/></disp-formula><p>For example, square bracket <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\ca48367e-56d0-4a02-b7c6-4b52b0185237.png" xlink:type="simple"/></inline-formula> bottom of the figure indicate that the random vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\fb4cf4bf-4718-4d30-b88f-db4b9ba7a81a.png" xlink:type="simple"/></inline-formula> should be sampled under the condition <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\625395b8-e020-4eaa-b2f5-0b0d84548718.png" xlink:type="simple"/></inline-formula> at time<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\316f2bbb-9928-422d-98c8-acd9a4bf6cd6.png" xlink:type="simple"/></inline-formula>. At the first default time<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\251abc18-241a-429f-93a6-a62f0f44ec22.png" xlink:type="simple"/></inline-formula>, updated default threshold is sampled under the condition <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\aa26210c-1bb7-4ea0-9963-b76eec7f591d.png" xlink:type="simple"/></inline-formula> and this</p><fig id="fig1"><label>Figure 1</label><caption><p> Sequence of defaults and the corresponding memory periods</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\0de958c0-c9ff-4701-9253-97d99e7a30ae.png"/></fig><p>condition remains effective until<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7722ac54-3ddd-4961-a7b3-94397bd2056b.png" xlink:type="simple"/></inline-formula>. This is shown by a square bracket <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\8c62dca2-db23-4e3b-b218-659cdb07f0bb.png" xlink:type="simple"/></inline-formula> which</p><p>indicate that the random vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\ff09f84d-63b1-46b3-b3d1-34e4d53cd35b.png" xlink:type="simple"/></inline-formula> should be sampled under the condition <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\8b28d89b-d8d7-47e4-84d3-5d04e8f659dd.png" xlink:type="simple"/></inline-formula></p><p>at time<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\f5f0367b-36df-417c-9cc2-a1c396a09cd3.png" xlink:type="simple"/></inline-formula>. If the second default occurred at time<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\80936967-9756-4b1a-8b46-1c7cc2f59467.png" xlink:type="simple"/></inline-formula>, then the updated default threshold at</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\600cd0eb-34d8-40c9-aa91-18b582f2b390.png" xlink:type="simple"/></inline-formula>should be sampled under the condition<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\de5c3afa-7736-4831-8f32-bb539028c374.png" xlink:type="simple"/></inline-formula>. However, at the</p><p>third default time<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\fc2c708f-c150-42d8-ae90-72a5c93796a4.png" xlink:type="simple"/></inline-formula>, investor’s interest have changed from the first default to the second default</p><p>completely, i.e., the memory period of 5 after <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\478ff7a5-598f-4b77-939d-5269404584cc.png" xlink:type="simple"/></inline-formula> have finished. Therefore updated default threshold should be</p><p>sampled under the condition<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\4a85c11e-3c66-4413-bd9f-ad6b558b8059.png" xlink:type="simple"/></inline-formula>. Notice also that <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\a4e451ae-b4e8-4295-bd4a-231c85eb5035.png" xlink:type="simple"/></inline-formula></p><p>In this subsection we see how the conditional distribution of the default threshold change at the default time.</p></sec><sec id="s2_3"><title>2.3. Default Contagion</title><p>In this subsection we see how the conditional distribution of the default threshold change at the default time.</p><p>Suppose that the first default occurred at time<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\4f9951f1-272d-4ccd-b5c4-2af144f49ea7.png" xlink:type="simple"/></inline-formula>. Let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\ed3605e9-c990-43cd-9997-ef8ff3600048.png" xlink:type="simple"/></inline-formula> denote the unconditional density of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\9d80bed2-9a28-40de-8095-bed5d2efe366.png" xlink:type="simple"/></inline-formula></p><p>and let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\a1dc4b78-7d30-4b13-bab8-19f7daf978a6.png" xlink:type="simple"/></inline-formula> denote the conditional density of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\9afaf9ee-498f-449d-8025-ea50cbd80a19.png" xlink:type="simple"/></inline-formula> given<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\1611deb7-131e-4148-a539-42a2932f381a.png" xlink:type="simple"/></inline-formula>. The distributions of</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3d41a366-4ac7-41c9-98e7-5e4ce1b1cf32.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\6b780222-10e7-4bd4-b4c1-bfe35adf0cee.png" xlink:type="simple"/></inline-formula>change at <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\9c9ad939-3a8a-432c-9775-95c20e53ee5f.png" xlink:type="simple"/></inline-formula> from <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3414f462-dd66-4a8c-82e9-225633102eb5.png" xlink:type="simple"/></inline-formula> to <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3a4098f5-3ce1-427b-92ce-5553ecc81a8d.png" xlink:type="simple"/></inline-formula> then the default probabilities</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3abc9582-aeec-4554-a933-95e3da2b4e5b.png" xlink:type="simple"/></inline-formula>, which is restricted before<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\bc957a20-c0e5-4385-808f-cc10be9b1069.png" xlink:type="simple"/></inline-formula>, change from</p><disp-formula id="scirp.46378-formula22"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\271fb341-7f96-4b3e-9972-40a417133a59.png"/></disp-formula><p>to</p><disp-formula id="scirp.46378-formula23"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5245e65f-3715-4c7e-bcfe-d309d30a8d3c.png"/></disp-formula><p><xref ref-type="fig" rid="fig2">Figure 2</xref> and <xref ref-type="fig" rid="fig3">Figure 3</xref> show the conditional distribution of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\6fd259af-59c6-4173-aa47-afdb2a61d129.png" xlink:type="simple"/></inline-formula> at <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\54b1b1c1-eb65-4055-8f9c-0a3d0d5fc772.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\0c955599-e85e-440f-adec-406e57b339f3.png" xlink:type="simple"/></inline-formula> with</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\93e4c0d2-aa96-4b22-a660-d1646d27fedc.png" xlink:type="simple"/></inline-formula>. Distributions are truncated above the running minimum of the firm value</p><p>0.95. We see that the <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\53176b48-e437-4900-b9d5-e5215e08ade2.png" xlink:type="simple"/></inline-formula> control the contagion impact effectively.</p><p>Remark 4 Giesecke [<xref ref-type="bibr" rid="scirp.46378-ref5">5</xref>] showed that <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\016475b5-8a55-41b6-9f48-4125c7a43359.png" xlink:type="simple"/></inline-formula> does not admit the default intensity. Define the supermartingale <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\a48c8923-9fc3-4270-a2ad-a8d3e5e8fd38.png" xlink:type="simple"/></inline-formula> with respect to <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\354b4736-1f34-4421-9149-d13358fb6d4b.png" xlink:type="simple"/></inline-formula> as</p><disp-formula id="scirp.46378-formula24"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\58fc3bf0-8f26-40ca-baa5-3eda17144694.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\f01327f4-5f5c-4a10-9a60-2b8280006f66.png" xlink:type="simple"/></inline-formula> then <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\6a9626a8-d084-4e18-b32a-526a7d653ff5.png" xlink:type="simple"/></inline-formula> can be expressed as</p><disp-formula id="scirp.46378-formula25"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\9e49dd76-de0c-42d2-8463-1376a94c09e3.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\b4a51c78-ef02-464b-9336-072f2a14f93b.png" xlink:type="simple"/></inline-formula> is cumulative distribution function of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\84ea759c-3c82-4760-a7e7-4729a0889228.png" xlink:type="simple"/></inline-formula>. Define the nondecreasing process <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7ed57234-8cde-4e16-b6fb-ae720a19480a.png" xlink:type="simple"/></inline-formula> by the Stiel- tjes integral</p><disp-formula id="scirp.46378-formula26"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\b189dfca-72bc-48f9-a0b0-95975c2c0a7b.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\b13b423e-719a-4bb1-8153-793fc4f3bb0b.png" xlink:type="simple"/></inline-formula> is the compensator of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\d39a8f60-91cc-4ae9-9e5d-fb5ad0c7852b.png" xlink:type="simple"/></inline-formula>. Therefore</p><disp-formula id="scirp.46378-formula27"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\d419d11d-cfda-4e74-b96e-042f84f65ba1.png"/></disp-formula><p>Consequently, by introducing the density function <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5409ca22-1c87-443d-8cd2-fa18f8294c77.png" xlink:type="simple"/></inline-formula> of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\91587939-fdeb-4eca-926d-4ad263264d4e.png" xlink:type="simple"/></inline-formula>, one can obtain</p><disp-formula id="scirp.46378-formula28"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\b8d476be-cff6-46d1-a706-45b7c72f53bf.png"/></disp-formula><p>which implies that <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\db6c73d6-68f3-4fb3-aec0-8adcb4eb3443.png" xlink:type="simple"/></inline-formula> is singular because <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\f0bc85e5-e273-4188-834f-b50c53d1accf.png" xlink:type="simple"/></inline-formula> is concentrated on the set<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\e32074e0-5e72-42cf-bd85-c205b866d464.png" xlink:type="simple"/></inline-formula>, which has</p><fig id="fig2"><label>Figure 2</label><caption><p> g<sub>i</sub>(x) and g<sub>i</sub>(x|T<sub>1</sub> = T<sub>j</sub>) whith r<sub>ij</sub> = 0.01</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\d89c6690-927e-4559-b387-53670aa6cca9.png"/></fig><fig id="fig3"><label>Figure 3</label><caption><p> g<sub>i</sub>(x) and g<sub>i</sub>(x|T<sub>1</sub> = T<sub>j</sub>) whith r<sub>ij</sub> = 0.04</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\207964e6-ad19-4eee-afc8-337603842758.png"/></fig><p>Lebesgue masure 0. Therefore <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7fe38077-ab51-42d1-8415-877b477f7945.png" xlink:type="simple"/></inline-formula> does not admit the representation<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\d2e69aa5-6077-4206-8b6f-ad591c5ce4f3.png" xlink:type="simple"/></inline-formula>. This is the reason why</p><p>we argue the default probabilities instead of the default intensities in our model.</p></sec></sec><sec id="s3"><title>3. Monte Carlo Method</title><p>This section develops a numerical method to compute the distribution of the number of defaults via Monte Carlo simulation. Complicating matters is the fact that new information of defaults changes the mean and covariance of the joint distribution of the thresholds. At each moment, covariance matrix should be calculated relying upon whether the memory period have terminated or not. Therefore, the simulation depends on the path, i.e. the order of occurrence of sequential defaults.</p><p>The time interval <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\62472805-9c61-4b9c-980c-723fa0a64796.png" xlink:type="simple"/></inline-formula> is partitioned into sub-intervals of equal length <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\910aed0f-be0d-41d5-be0c-240f4dae28b8.png" xlink:type="simple"/></inline-formula> and firm value processes evolve along the discretized time step<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\9c12c15e-09ee-4da9-aa64-3bdd5ab387f7.png" xlink:type="simple"/></inline-formula>, where<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\e3eecc18-c0f8-43a6-a474-f3fe98380d17.png" xlink:type="simple"/></inline-formula>. With the discretization of the time variable, we redefine the default time as</p><disp-formula id="scirp.46378-formula29"><label>(0.10)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\373f64c4-964d-4467-868f-d7fb3fa5f66a.png"/></disp-formula><p>in analogy with its continuous time version (0.3). As mentioned in Carmona, Forque and Vestal [<xref ref-type="bibr" rid="scirp.46378-ref14">14</xref>] , we do not have to correct for the bias introduces by the discretization of a continuous time boundary crossing problem.</p><p>Algorithm 1 To generate a one sample path of the total default<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\d4d70a00-e036-4fb1-8600-bd0ea98d626e.png" xlink:type="simple"/></inline-formula>, perform the following:</p><p>Step 0. Initialize<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\08351818-bc7c-4b61-90a3-d22cddb31636.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\52788239-caa2-46ea-aa93-df724057e21c.png" xlink:type="simple"/></inline-formula>. Set<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\01e295eb-1928-42ab-8c48-dd6e9841e91d.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\04f08f32-7aa8-4508-80b8-c6b2579a87aa.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\b5f4397f-02bd-4256-aa2c-f9d10137b028.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\6f3bb6b6-e0ce-4492-9ba1-4c9e5fe8d3f9.png" xlink:type="simple"/></inline-formula>. Draw the random barrier</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\c8729200-fb0a-456e-9394-eee4409ee060.png" xlink:type="simple"/></inline-formula>for all firms in portfolio and fix them until the first default occurred.</p><p>Step 1. Generate the <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\445eb3aa-4852-4f16-8517-461d1c3d18b7.png" xlink:type="simple"/></inline-formula>-dimensional path <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\2ddc789a-ce2c-4d28-bcef-f70ff5a22b80.png" xlink:type="simple"/></inline-formula> and calculate the running minimum</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\69027766-ca69-4c27-b167-c0541a607df3.png" xlink:type="simple"/></inline-formula>for each<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\8b342b35-1776-4aec-ad46-ca5330cf4014.png" xlink:type="simple"/></inline-formula>.</p><p>Step 2. Determine whether default occurred or not at time <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\82f37ceb-ca8e-4924-91aa-0ea200dacc5d.png" xlink:type="simple"/></inline-formula>and renew the set <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\74928610-dc3b-42e2-bb2a-70d93719da0b.png" xlink:type="simple"/></inline-formula> as follows.</p><p>If<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3fb1d3de-c6d5-463b-933b-1bdd6a089949.png" xlink:type="simple"/></inline-formula>, then the firm <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\1a05511a-4215-41a5-8506-3eea1dd9cae5.png" xlink:type="simple"/></inline-formula> gets default at time<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\bc2bad59-f63b-4dc3-a94c-fe15bbd8dc9a.png" xlink:type="simple"/></inline-formula>, and then set<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\e28ac17d-a880-4858-a18d-d2b892c29914.png" xlink:type="simple"/></inline-formula>.</p><p>Else, set<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\90995c7f-9cec-4639-b14d-473c775fae82.png" xlink:type="simple"/></inline-formula>.</p><p>Let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\9ec3fa8f-203c-4f27-82a9-06f27bcd01c7.png" xlink:type="simple"/></inline-formula> be a set consists of defaulted firms at time <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3590d16c-6371-4e0a-a1de-7123e6e2f3ca.png" xlink:type="simple"/></inline-formula> and go to Step 3.</p><p>If <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\6ab5f0d6-8fad-467a-affd-cb35e18107f5.png" xlink:type="simple"/></inline-formula> hold for all<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\8e1dff4b-39c1-4942-9fef-873f414fb7b4.png" xlink:type="simple"/></inline-formula>, set <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\53058b88-bef6-4b26-993b-a97b27466994.png" xlink:type="simple"/></inline-formula> for all <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\d1bb349d-6c1e-4dab-b832-528c63b160f1.png" xlink:type="simple"/></inline-formula> and go to Step 1.</p><p>Step 3. Determine <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3783cb19-7e09-4312-85f5-cecbf36d9982.png" xlink:type="simple"/></inline-formula> for all defaulted firms and calculate the realized barrier for the defaulted</p><p>firms and store<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\1aeda28f-9939-4bac-aaea-9eb902e2c694.png" xlink:type="simple"/></inline-formula>.</p><p>Step 4. Renew the matrix <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\6922b70b-9960-4df3-bd52-fafdf77693c0.png" xlink:type="simple"/></inline-formula> and the set<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\a92ee077-b6e3-456c-a5c7-550cac5f85c7.png" xlink:type="simple"/></inline-formula>. Draw the random barrier <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\8ea2bf69-736a-4000-a5e5-7d714ab805f2.png" xlink:type="simple"/></inline-formula> for all</p><p>survived firms <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\0d069ed8-83f8-41f4-a55f-002d60ab4231.png" xlink:type="simple"/></inline-formula> and fix them until next default occurred. Sampling is based on the distribu-tion truncat-</p><p>ed above<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\47bb1f5d-5313-429a-9479-979866b0a7ca.png" xlink:type="simple"/></inline-formula>.</p><p>Step 5. Set <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\aec11f78-951f-4d74-898a-7f15d6f7b30f.png" xlink:type="simple"/></inline-formula> and go to Step1.</p></sec><sec id="s4"><title>4. Interacting Particle System</title><p>In credit risk management, it is important to measure how often the rare but crucial events will occur. However, standard Monte Carlo algorithm in Section 3 may be inefficient in some situations such as the portfolio constituents have small default probabilities. This is because, in order to estimate accurately the probability of rare events, a large number of trials may be required with Algorithm 3.1.</p><p>In an effort to estimate the accurate probabilities within a reasonable computational time, we embed IPS to original standard Monte Carlo simulation algorithm. In the following two subsections, we provide a quick overview of the IPS inspired by the pioneering work Del Moral and Garnier [<xref ref-type="bibr" rid="scirp.46378-ref15">15</xref>] and subsequent papers Carmona, Forque and Vestal [<xref ref-type="bibr" rid="scirp.46378-ref14">14</xref>] , Carmona and Crepey [<xref ref-type="bibr" rid="scirp.46378-ref16">16</xref>] and Giesecke et al. [<xref ref-type="bibr" rid="scirp.46378-ref7">7</xref>] .</p><sec id="s4_1"><title>4.1. Feynman-Kac Path Measures</title><p>Let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3e255112-ae72-4e50-a174-b64f659a13ef.png" xlink:type="simple"/></inline-formula> be the time horizon. Partition the interval <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7ca97889-fc82-42de-a6b2-6263adc0dce8.png" xlink:type="simple"/></inline-formula> into <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\1b3e1767-193b-40ac-aec7-38831194fee6.png" xlink:type="simple"/></inline-formula> subintervals of length<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\e1fbcb8a-ca9e-4593-9c97-667bd7040919.png" xlink:type="simple"/></inline-formula>. Let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\0aef10fa-0c87-4fe8-85bd-3ed3c6d53c62.png" xlink:type="simple"/></inline-formula> be</p><p>the discrete time Markov chain given by <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\f1595999-f441-4bd9-9671-b4da4e45b31b.png" xlink:type="simple"/></inline-formula> where, in our model, continuous time</p><p>Markov chain <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7bb76697-7d01-4d45-8aa6-22d0e44c3443.png" xlink:type="simple"/></inline-formula> is given by</p><disp-formula id="scirp.46378-formula30"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\d0c25f4e-92cb-44e2-b22b-9e42787c4585.png"/></disp-formula><p>which will be discussed later. In general, the random element <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\920b38ad-2c07-4880-8373-c196b789f660.png" xlink:type="simple"/></inline-formula> takes values in some measurable state space</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\97db2d6d-f829-45b3-8273-135e530f5eb5.png" xlink:type="simple"/></inline-formula>that can change with<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\ad348ea3-7c28-43c1-9064-fd494a48c502.png" xlink:type="simple"/></inline-formula>. We denote by <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5eaadc39-2417-4177-bb63-8a25c33cc0e7.png" xlink:type="simple"/></inline-formula> the transition kernels of the Markov chain</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\16aadb59-296a-4fc6-b9f7-506bda351840.png" xlink:type="simple"/></inline-formula>at time<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\4444a6f3-491d-4384-befe-e07e34b3e83b.png" xlink:type="simple"/></inline-formula>, and we denote by <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\e0abbae5-9eb5-462d-ba0b-aeb9e5fb72ac.png" xlink:type="simple"/></inline-formula> the historical process of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\d8357b21-53c6-40bc-a5b9-25bfb7e946c1.png" xlink:type="simple"/></inline-formula> defined by</p><disp-formula id="scirp.46378-formula31"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\c6e925d8-0db3-4dd6-91e6-5ceeed90546a.png"/></disp-formula><p>Next, we let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\9d4683d1-35c4-430f-b210-f007eec9c071.png" xlink:type="simple"/></inline-formula> denote the transition kernels of the inhomogeneous Markov chain<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\4584d04e-4626-4e3e-a7cb-e0a0497681a5.png" xlink:type="simple"/></inline-formula>. We</p><p>finally let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\0474149a-4221-4ea9-bb12-f73ed7b6a93f.png" xlink:type="simple"/></inline-formula> be the space of all bounded measurable functions on some measurable space<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\0a46d34b-c98d-40b7-9d41-4a57efffcc86.png" xlink:type="simple"/></inline-formula>, and we equip <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\ba808859-78d5-4294-ba9d-10bb328e1411.png" xlink:type="simple"/></inline-formula> with the uniform norm.</p><p>The Interacting Particle System consists of a set of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3a7e6243-5617-4c4b-ad4f-846ea8898c4d.png" xlink:type="simple"/></inline-formula> path-particles <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\1a8b7f6a-0cfd-41c9-a0e0-110d7d520201.png" xlink:type="simple"/></inline-formula> evolving from time</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\d8ceeffb-658c-4d23-8be3-6cea739ae645.png" xlink:type="simple"/></inline-formula>to<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7bf9f059-3904-47b2-8435-7e597f1fb16b.png" xlink:type="simple"/></inline-formula>. The initial generation at time <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\abab1b4d-e07b-4a01-98c1-033a1ad0a9e8.png" xlink:type="simple"/></inline-formula> is a set of independent copies of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\b4ca3de6-8d5c-4047-a336-d47fcc0cd64b.png" xlink:type="simple"/></inline-formula> and the system evolves as if strong animals produce many offsprings, however the rest die.</p><p>For each<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\f8165dd4-4fb0-4688-88a6-f3188d4afb72.png" xlink:type="simple"/></inline-formula>, we consider non-negative measurable functions <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5c1838ed-d150-4890-bfbb-f760a17c844b.png" xlink:type="simple"/></inline-formula> defined on <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7c7d9543-7c47-4c23-9d16-246e2b3bf86f.png" xlink:type="simple"/></inline-formula> equipped with the product <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\4757343d-4f89-484f-b656-277e9ba0866d.png" xlink:type="simple"/></inline-formula>-algebra, and we call these functions as potential functions. We associate to the pair of potentials and</p><p>transitions <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\43696de3-6ac5-43a2-9de3-c0a449e05b60.png" xlink:type="simple"/></inline-formula> the Feynman-Kac path measure defined for any test function <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\f8619244-607c-468a-bfef-b8008ea71b17.png" xlink:type="simple"/></inline-formula> by the</p><p>formula</p><disp-formula id="scirp.46378-formula32"><label>(0.11)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\238f3e32-7ac4-4a4b-ae70-c231e05532f2.png"/></disp-formula><p>We also introduce the corresponding normalized measure</p><disp-formula id="scirp.46378-formula33"><label>(0.12)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\98bcb587-1b3d-49c7-a9ae-3b0b73aaf323.png"/></disp-formula><p>Note that</p><disp-formula id="scirp.46378-formula34"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\faf3bb90-b5d0-4f94-8e31-e2d1d594d03e.png"/></disp-formula><p>Therefore, for any given bounded measurable function<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\01429b8a-a595-4eee-b9d2-470f7337b310.png" xlink:type="simple"/></inline-formula>, we have</p><disp-formula id="scirp.46378-formula35"><label>(0.13)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5e902c32-6037-416f-be9f-350bacbe4228.png"/></disp-formula><p>The above relationship has the merit of relating the un-normalized expectations in the left hand side to nor-</p><p>malized expectations in the right hand side. Furthermore, for any path<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\56dbc4cb-ef10-4193-9d87-beeecff78080.png" xlink:type="simple"/></inline-formula>, we define the</p><p>weighted indicator function</p><disp-formula id="scirp.46378-formula36"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\1bb9b147-7763-4136-ae6a-0f2f808d1df9.png"/></disp-formula><disp-formula id="scirp.46378-formula37"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\1bb9b147-7763-4136-ae6a-0f2f808d1df9.png"/></disp-formula><p>Then we see that</p><disp-formula id="scirp.46378-formula38"><label>(0.14)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\e670da9e-fca0-4861-ae81-5faebb279f90.png"/></disp-formula><p>This formula can be applied to the situation that the <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\0398f27c-6837-406e-8bc4-7c06e59e4f96.png" xlink:type="simple"/></inline-formula> are the rare events and it can be</p><p>computed via computation of normalized measures. It is known (see Del Moral and Garnier [<xref ref-type="bibr" rid="scirp.46378-ref15">15</xref>] ) that the computation of the sequence of normalized measures is achieved by the following non-linear recursive equation</p><disp-formula id="scirp.46378-formula39"><label>(0.15)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\12f5c542-1540-4961-9738-b14537fecbc2.png"/></disp-formula><p>starting from<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\9ba0fa15-4803-4f3f-a616-14f7653ab1a5.png" xlink:type="simple"/></inline-formula>. Equation (0.15) has the differential form</p><disp-formula id="scirp.46378-formula40"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\f672bda7-2159-4e43-99dc-c8619d0e5fd3.png"/></disp-formula><p>which can be easily seen by substituting</p><disp-formula id="scirp.46378-formula41"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3eeedd42-957c-48e6-a9ee-6c20746467cb.png"/></disp-formula><p>and</p><disp-formula id="scirp.46378-formula42"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\a8e76422-4eeb-4c5d-8d0b-0248e396e2ed.png"/></disp-formula><p>into the integrand of the right hand side of (0.15).</p></sec><sec id="s4_2"><title>4.2. Interacting Particle Interpretation</title><p>For the purpose of numerical computations of the rare events of the form (0.14), we introduce an interacting particle system. We choose a large integer <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3caa81f5-b54e-426b-be7f-6fc30f34f269.png" xlink:type="simple"/></inline-formula> which we shall interpret as the number of particles. We construct</p><p>a Markov chain <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\8d44c6cb-c60e-41a7-a39d-1c04f063003d.png" xlink:type="simple"/></inline-formula> whose state <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\4b2656cc-6dee-4186-a75a-bb6688fce5af.png" xlink:type="simple"/></inline-formula> at time <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\0744231b-cce7-4fff-8230-426a1f4d92f5.png" xlink:type="simple"/></inline-formula> can be interpreted as a set of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\714aa2c7-9c3e-4742-8429-234b7167e9ba.png" xlink:type="simple"/></inline-formula> samples of</p><p>particles with respect to the measure<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\26e811f5-c14a-42e1-bc80-d4e307a64424.png" xlink:type="simple"/></inline-formula>,</p><disp-formula id="scirp.46378-formula43"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\1c885e8b-a4af-4b9a-86f1-59f758a4908c.png"/></disp-formula><p>We start with an initial configuration <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\6a1d62a5-ae00-4d25-a082-8bd9d02c4380.png" xlink:type="simple"/></inline-formula> that consists of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\b49731a4-b082-4e9e-8a3c-8d2c9397055c.png" xlink:type="simple"/></inline-formula> independent and identically distri-</p><p>buted random samples from the distribution</p><disp-formula id="scirp.46378-formula44"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3a6aef3b-eb78-4323-b826-54b41aa854a8.png"/></disp-formula><p>i.e., <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\bbbd8b76-71e9-4da7-802e-87947bd96b65.png" xlink:type="simple"/></inline-formula>where the <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\83c3c2e8-b3db-427b-a67b-f0ccf17a6933.png" xlink:type="simple"/></inline-formula> are drawn independently of each other from the</p><p>distribution<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\b9aeadc9-a129-4d4b-8bd3-292e5eecb97a.png" xlink:type="simple"/></inline-formula>. The transitions of particles from <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\54f3fdfa-f044-4e4d-9549-b687737efe38.png" xlink:type="simple"/></inline-formula> into <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\84bfe3a4-db3f-46ed-8835-8c2777a602f4.png" xlink:type="simple"/></inline-formula> are defined by</p><disp-formula id="scirp.46378-formula45"><label>(0.16)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\b259150c-1d90-4953-bdc5-c3bd6952276d.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\80b4632f-b9e9-4c6a-b7aa-754773c74bfc.png" xlink:type="simple"/></inline-formula> is the empirical measure defined by</p><disp-formula id="scirp.46378-formula46"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\09558c02-73d7-403c-8095-74fe20722464.png"/></disp-formula><p>and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\fd381f49-3a10-4969-9a61-d114176ddee7.png" xlink:type="simple"/></inline-formula> represents an infinitesimal neighborhood of the point<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\e5c21c13-9c63-415c-ae23-20a767ce6a37.png" xlink:type="simple"/></inline-formula>. By the definition</p><p>of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\38160892-7cc3-4460-8691-e9de1895a3a1.png" xlink:type="simple"/></inline-formula>, one sees that (0.16) is the superposition of two identifiable transitions, a selection followed by a mutation as shown below.</p><disp-formula id="scirp.46378-formula47"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5bece249-c0fc-4432-b603-ed9b2f3e737e.png"/></disp-formula><p>The selection stage is performed by choosing randomly and independently <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\050717b6-c686-4da4-9355-9089a6fdb16f.png" xlink:type="simple"/></inline-formula> particles</p><disp-formula id="scirp.46378-formula48"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\1e9d7c00-bfc5-4444-a74e-70739d7d2eed.png"/></disp-formula><p>according to the Boltzmann-Gibbs measure</p><disp-formula id="scirp.46378-formula49"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\06678fb0-29cf-4091-a583-79f5c67a4925.png"/></disp-formula><p>During the mutation stage, each selected particle <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\ae08d755-1d1c-4629-9bd5-03d09e579e50.png" xlink:type="simple"/></inline-formula> is extended in time by an elementary <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\d48dcae0-1d24-4dae-b1e4-7d1a57ed2c2a.png" xlink:type="simple"/></inline-formula>-transition.</p><p>In other words, we set</p><disp-formula id="scirp.46378-formula50"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\deb3fb58-bdd5-4666-ac90-0cce251217a3.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\55644996-68ab-412e-b17e-3b41d2153329.png" xlink:type="simple"/></inline-formula> is a random variable with distribution<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\ee46286c-a415-4325-b5d5-bb0c28edf885.png" xlink:type="simple"/></inline-formula>. The mutations are performed independently.</p><p>A result of [<xref ref-type="bibr" rid="scirp.46378-ref17">17</xref>] reproduced in [<xref ref-type="bibr" rid="scirp.46378-ref15">15</xref>] states that for each fixed time<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5bf83183-75ab-4dd6-868e-4500513ceb09.png" xlink:type="simple"/></inline-formula>, the empirical measure converges in distribution, as<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7d608188-37d7-4a6a-a71e-ee8550fd6599.png" xlink:type="simple"/></inline-formula>, toward the normalized Feynman-Kac measure<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\8588badc-c11d-44be-8778-5999cec664ed.png" xlink:type="simple"/></inline-formula>, i.e.,</p><disp-formula id="scirp.46378-formula51"><label>(0.17)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\067fcbf5-47b1-4dc6-8d9b-48792d0c52c4.png"/></disp-formula><p>Mimicking (0.13), unbiased particle approximation measures <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\27d6f82a-4f83-4e29-9a9a-4321f467dbc8.png" xlink:type="simple"/></inline-formula> of the un-normalized measure <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\229339e8-ad0d-4628-a067-b11c0e2f452f.png" xlink:type="simple"/></inline-formula> are defined as</p><disp-formula id="scirp.46378-formula52"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\cb941a51-8d45-4b12-87bb-010d9c3765fe.png"/></disp-formula><p>and then, by (0.14), we can get the particle approximation of the rare event probabilities. More precisely, if we let</p><disp-formula id="scirp.46378-formula53"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\4501868e-c574-4b18-96ad-b5018af47c69.png"/></disp-formula><p>then <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\8e12bf84-e5eb-47c2-924c-a8ea36ece281.png" xlink:type="simple"/></inline-formula> is an unbiased estimator of the rare event probabilities <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\98016884-9e4f-4619-ae6b-1f05bb00cfcc.png" xlink:type="simple"/></inline-formula> such that</p><disp-formula id="scirp.46378-formula54"><label>(0.18)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\e006e9bb-2406-4904-b334-f9b872f9c173.png"/></disp-formula><p>We refer to Del Moral [<xref ref-type="bibr" rid="scirp.46378-ref17">17</xref>] and Del Moral and Garnier [<xref ref-type="bibr" rid="scirp.46378-ref15">15</xref>] for the details of the convergence results. Their complete proofs rely on a precise propagation of chaos type analysis and they can be found in Section 7.4 on Pages 239-241 and Theorem 7.4.1 on Page 232 in Del Moral [<xref ref-type="bibr" rid="scirp.46378-ref17">17</xref>] .</p></sec><sec id="s4_3"><title>4.3. IPS Algorithm and Potential Functions</title><p>We introduce special notations <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\e4deca48-1786-4497-818d-ac3e787b8afe.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\22711f57-7bb4-4aa3-914e-0be463690136.png" xlink:type="simple"/></inline-formula> which indicate that these are the input to the selection stage, while another notation <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\266f8bef-d4c3-4eda-8377-6a845aab5476.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\4568e9ab-564b-482d-9478-09f47b649874.png" xlink:type="simple"/></inline-formula> indicate that these are the input to the mutation stage of the IPS algorithm. Here, as we will describe later, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\4e6c62a7-b0ea-4f0a-89e5-631935a60b85.png" xlink:type="simple"/></inline-formula>indicate the parent of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\06ce6a0c-f449-4455-9884-49616129b703.png" xlink:type="simple"/></inline-formula>.</p><p>According to Del Moral and Garnier [<xref ref-type="bibr" rid="scirp.46378-ref15">15</xref>], one of the recommended potential functions are of the form</p><disp-formula id="scirp.46378-formula55"><label>(0.19)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\d26fc2d2-e30c-4d1f-ac7d-df19fc82745d.png"/></disp-formula><p>for some <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\72a3c553-60c1-4ea6-a8fb-21491897a887.png" xlink:type="simple"/></inline-formula> and suitable function <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\074623a2-bc4a-4a45-ace4-2291abeecb08.png" xlink:type="simple"/></inline-formula> so as to satisfying</p><disp-formula id="scirp.46378-formula56"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\0b5a5f66-ca80-484a-8601-ea1d89b61844.png"/></disp-formula><p>This regularity condition ensures that the normalizing constants <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\c4691338-3477-4f34-b1da-aad4b093bd15.png" xlink:type="simple"/></inline-formula> and the measure <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3a872f1f-f622-4242-ab16-463f26c1888a.png" xlink:type="simple"/></inline-formula> are bounded and positive. Thanks to the form of this potential function, we note that we need only to keep track of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3aaeafa4-26bf-419b-9a20-6f9e2b4db928.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\c53bdf57-c36f-4bb6-8fcd-feb6f4f77c97.png" xlink:type="simple"/></inline-formula>, and then the selection would be implemented with those two particles. The form of the distribution (0.17) shows that in order to have more simulation paths realizing great many defaults, it is important to choose a potential function becoming larger as the likelihood of default increases. To meet our purpose, we choose the function <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\06f34af8-ff3f-4ae9-96e5-579eac8f44ca.png" xlink:type="simple"/></inline-formula> as follows.</p><disp-formula id="scirp.46378-formula57"><label>(0.20)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\60305235-7fa9-472d-9da9-20810bd66dcb.png"/></disp-formula><p>Then our potential function is given by</p><disp-formula id="scirp.46378-formula58"><label>(0.21)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\f34b340c-dc82-4eea-9bdf-6f4ce720f18d.png"/></disp-formula><p>The first term of (0.21) reflects the fact that the high weights are assigned to the particle which had renewed the running minimum during the period<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\1a0613ce-05e2-46aa-9df9-f8628b48a017.png" xlink:type="simple"/></inline-formula>. When <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\e98445ac-9936-4bc3-b9c0-0315995a5732.png" xlink:type="simple"/></inline-formula> is not random, i.e., the default barrier is</p><p>observable, it is known that the IPS is effective to simulate the counting process <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\0b09445c-a912-4080-979d-99ae02d997fa.png" xlink:type="simple"/></inline-formula> with reasonable</p><p>accuracy by Carmona, Fouque and Vestal [<xref ref-type="bibr" rid="scirp.46378-ref14">14</xref>] . We borrowed the form of potential function from Carmona, Fouque and Vestal [<xref ref-type="bibr" rid="scirp.46378-ref14">14</xref>] . Detailed IPS algorithm is summarized as follows.</p><p>Algorithm 2 Assume that we have a set of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\544af569-f610-46c6-813c-e40ac722d8b7.png" xlink:type="simple"/></inline-formula> particles at time <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\fba2a470-4db2-4bb4-89ff-5e4b818cb538.png" xlink:type="simple"/></inline-formula> denoted by<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5a7a2361-525f-46ba-93af-acdba321479d.png" xlink:type="simple"/></inline-formula>. We</p><p>define the Markov process</p><disp-formula id="scirp.46378-formula59"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\4c3b8ae9-e26d-46f6-b4c7-52b28ba67b3c.png"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\f5416f43-ac6f-4504-a480-10a93578e0ac.png" xlink:type="simple"/></inline-formula>, and define the discrete time Markov process<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\368b7344-09b2-41d2-b78c-9c0c89592ae2.png" xlink:type="simple"/></inline-formula>.</p><p>To generate an estimate of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\70788287-98d5-4c15-8005-1f1307dcfcae.png" xlink:type="simple"/></inline-formula> for<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5951918d-ac2d-40ec-a2a3-5923d416a939.png" xlink:type="simple"/></inline-formula>, perform the following:</p><p>Step 0. Initialize the particles <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7eef4fe7-febf-48d9-93ff-8dffb43326ee.png" xlink:type="simple"/></inline-formula> and indicators<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\00948d7d-dc9e-4bcc-85de-3a3ac069108c.png" xlink:type="simple"/></inline-formula>. Choose <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\042632b9-75ba-4d93-a026-29b7f013b646.png" xlink:type="simple"/></inline-formula> as a discretized time step for the</p><p>firm value processes, to be some small value. We start with a set of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\cf776c70-b414-4190-a956-aa5fd38bf8a6.png" xlink:type="simple"/></inline-formula> i.i.d. initial conditions<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\2c92fe0b-aaa7-4f62-8272-e184e0cbf0f5.png" xlink:type="simple"/></inline-formula>,</p><p>chosen according to the initial distribution of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\251e3b2f-badc-42a4-9ea1-37432eba0cac.png" xlink:type="simple"/></inline-formula>.</p><p>Set <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\219451ed-4540-44a8-8b59-948f78aea4dd.png" xlink:type="simple"/></inline-formula> (initial value of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\39cf64be-6ba2-404c-b03a-0eb58065319d.png" xlink:type="simple"/></inline-formula>) for all <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\1133fea2-53f1-49f2-a00b-2ef2e3e14ac9.png" xlink:type="simple"/></inline-formula> and then form a set of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\f09b89d1-fb34-4f2b-a0f5-10fffb542e45.png" xlink:type="simple"/></inline-formula> particles <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\efab73d0-caa3-49fa-b0b1-5d3dccae9916.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.46378-formula60"><label>.</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\9a481dc1-1648-4ff4-a274-2a709be1cf15.png"/></disp-formula><p>Step 1. For each step<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\eb300af8-20a7-4200-9337-da7bd0c2824b.png" xlink:type="simple"/></inline-formula>, repeat the following steps.</p><p>• Selection.</p><p>Compute the normalizing constant</p><disp-formula id="scirp.46378-formula61"><label>(0.22)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\39e06903-0bef-4df2-8c2a-ba2962838e62.png"/></disp-formula><p>and choose independently <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7aff8640-8f5e-4202-ae47-4c0fbd7621c2.png" xlink:type="simple"/></inline-formula> particles according to the empirical distribution</p><disp-formula id="scirp.46378-formula62"><label>(0.23)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\d13a4d8a-d93e-492b-aeef-39d9be450b4a.png"/></disp-formula><p>The new particles are denoted by<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\a95f6022-afb5-473b-8363-4edde8847cc0.png" xlink:type="simple"/></inline-formula>.</p><p>• Mutation.</p><p>For every<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\cce71d39-cbe4-4948-a8d0-ec1b2ee7d78e.png" xlink:type="simple"/></inline-formula>, using the Algorithm 3.1, the particle <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\98dafc0c-15f6-4f14-9d5a-b3f3b1bf992f.png" xlink:type="simple"/></inline-formula> is transformed into</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\cb856752-2197-4fe7-9c33-15c9232d675c.png" xlink:type="simple"/></inline-formula>independently by</p><disp-formula id="scirp.46378-formula63"><label>(0.24)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\ef3f9045-1371-4aac-a88c-c973c466ce61.png"/></disp-formula><p>and set<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\fe2cf95f-457f-46b1-abc7-649d8b8563da.png" xlink:type="simple"/></inline-formula>.</p><p>Step 2. The estimator of the probability <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5ae67f20-4708-482e-a23b-c6d2bce5ae2d.png" xlink:type="simple"/></inline-formula> is given by</p><disp-formula id="scirp.46378-formula64"><label>(0.25)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\d6fb819c-47f3-4688-8734-567b22f21ffc.png"/></disp-formula><p>It is known that this estimator is unbiased in the sense that <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\f9ec1f4d-f148-40d9-8d06-7807dcda06fd.png" xlink:type="simple"/></inline-formula> and satisfies the central limit</p><p>theorem. (Refer to [<xref ref-type="bibr" rid="scirp.46378-ref15">15</xref>] [<xref ref-type="bibr" rid="scirp.46378-ref17">17</xref>] )</p><p>Instead of explicit calculation of the asymptotic variance, we notice that the approximate variance <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\2223940c-2aa4-43ea-9a87-93ef72cb9bd3.png" xlink:type="simple"/></inline-formula></p><p>defined by</p><disp-formula id="scirp.46378-formula65"><label>(0.26)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\f79c91d4-0f29-41de-9f48-a971454cebb4.png"/></disp-formula><p>can be easily calculated within the above IPS algorithm. This provides criteria to choose the parameter <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\4f13cb64-1467-4c86-b949-b47b19a63bfc.png" xlink:type="simple"/></inline-formula> to be a suitable level.</p></sec></sec><sec id="s5"><title>5. Numerical Examples</title><p>This section demonstrates the performance of the IPS algorithm through numerical examples with a sample portfolio consists of 25 firms. We consider portfolio consisting of high credit quality names with high correlations <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\60f7a46f-3861-41a2-9a3a-a78835e630bc.png" xlink:type="simple"/></inline-formula> of their firm value processes, as well as high correlations <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\2dc83da8-fa45-4a24-b784-effadff6fbdf.png" xlink:type="simple"/></inline-formula> of the default thresholds. The parameters of the model are summarized as follows.</p><p>• <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\24ce51f0-155f-44bd-9a37-ffdedb29841c.png" xlink:type="simple"/></inline-formula>for all<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\60cede1f-3c26-4eb8-b85a-678f73f5cac2.png" xlink:type="simple"/></inline-formula>,</p><p>• <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3b41e61d-de14-4ef4-a1f4-a9e8f5ff51ed.png" xlink:type="simple"/></inline-formula>for <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7ddbd4a8-82b8-4fec-96c9-bb7e71d0c498.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\096d4159-20ca-4991-9840-a7091e737a6b.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\f4d6160e-4d4e-476c-ab64-2e7f46cbdda2.png" xlink:type="simple"/></inline-formula>for <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\8bb29767-8eff-4831-8206-3ad7bb29d4c1.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\896713d1-e799-4040-9c91-a6dfdb46ae95.png" xlink:type="simple"/></inline-formula>.</p><p>Those parameters are set with the intention to notice rare default events. As Carmona, Fouque and Vestal [<xref ref-type="bibr" rid="scirp.46378-ref14">14</xref>] reports, the number of selections/mutations which is equal to <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\f769e4c4-4baf-42b2-88d4-7a2d6cc0feae.png" xlink:type="simple"/></inline-formula> in Algorithm 4.1 will not have so significant impact to numerical results then we set <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\2d440e33-7cae-445d-8068-228c9afb6712.png" xlink:type="simple"/></inline-formula> per one year. Here we set<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7125d886-d597-4f7a-9f4e-6409fd344a32.png" xlink:type="simple"/></inline-formula>.</p><p>First we compare the results of the IPS algorithm to the results obtained by the standard Monte Carlo algorithm in case of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\92dd6e9f-dd5e-4fd2-8ab3-c3a91ce228c9.png" xlink:type="simple"/></inline-formula> years. For the standard Monte Carlo, we run 10,000 trials and in addition, 500,000 trials that will be expected to achieve reasonably accurate values. As for IPS algorithm, we set <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\8e7a9466-06c6-42a4-a38b-572348f1fbee.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\c686d0ea-d095-4dfa-af0b-d0751d556d1f.png" xlink:type="simple"/></inline-formula> and take <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\779a69aa-cfda-46d8-bde7-f5f692fc998f.png" xlink:type="simple"/></inline-formula> for number of the particles. <xref ref-type="fig" rid="fig4">Figure 4</xref> illustrates the probability of defaults</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\48d2bb1c-81ac-48e5-847d-64ede041dc94.png" xlink:type="simple"/></inline-formula>for <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5af01fbb-23ca-4392-b346-96e069f1bdca.png" xlink:type="simple"/></inline-formula> for <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\72416ce4-c48e-4c8e-a0bd-5a40b046d15f.png" xlink:type="simple"/></inline-formula> with <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\f7f5dca0-4115-469d-9e93-5c76f8584fe4.png" xlink:type="simple"/></inline-formula> for all<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\30ef6cd5-154e-4c85-bbf0-2ceb83540eb6.png" xlink:type="simple"/></inline-formula>. Thus the market participants memorize</p><p>all the default by the time horizon. <xref ref-type="fig" rid="fig5">Figure 5</xref> plot the log scale for these three cases of probabilities for comparison. One can see that the standard Monte Carlo with 10,000 trials has oscillating results for rare events although the IPS results shows similar shape as 500,000 trials of Monte Carlo. For this numerical calculation, 500,000 trials took about 8000 seconds, whereas the IPS algorithm took about 275 seconds with 3.4 GHz Intel Core i7 processor and 4 GB of RAM.</p><fig id="fig4"><label>Figure 4</label><caption><p> Default probabilities</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\a21ca032-cffb-4e62-a627-2d729a5f6618.png"/></fig><fig id="fig5"><label>Figure 5</label><caption><p> Default probabilities in log-scale</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3ed54ace-b1f0-4b1b-86d0-4674ef35688b.png"/></fig><p>These numerical results show that the standard Monte Carlo with 10,000 trials can not capture the occurrence of rare default events such as over 20 defaults, however, one sees that there exist very small probabilities for such events via 500,000 trials which is indicated by solid blue line in <xref ref-type="fig" rid="fig5">Figure 5</xref>. As expected, IPS algorithm can capture these rare event probabilities which are important for the credit risk management.</p><p>Next, we investigate how variance would reduced by IPS with following two cases</p><p>• Case 1: <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\58c4cf09-1c10-46b7-9583-34ec152b2fa3.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\685e0873-367e-4041-9bb1-6780e026eb06.png" xlink:type="simple"/></inline-formula> for all<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\387a9547-7e1e-465a-8776-ae89dad6ea58.png" xlink:type="simple"/></inline-formula>,</p><p>• Case 2: <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\fb4962e0-ac58-4760-91e7-a5ff040d27b8.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\92ca4d6e-2cc6-49f0-aa8b-2ca1833dfa16.png" xlink:type="simple"/></inline-formula> for all<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\91ee6ad2-6fe1-487d-b229-332fa5e53e28.png" xlink:type="simple"/></inline-formula>,</p><p>to see the difference with respect to time horizon with the same memory period. Preliminary version of this paper, Takada [<xref ref-type="bibr" rid="scirp.46378-ref11">11</xref>] illustrated how the default distributions change in response to the memory period <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\ab6f7bad-179e-4e66-84c9-15fa8d549f45.png" xlink:type="simple"/></inline-formula> based on the standard Monte Carlo. One sees that the first default occurs with the same probability for different <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5acd0de0-dc2c-46cc-a114-e5eb0aa22ffa.png" xlink:type="simple"/></inline-formula>s but the second default occurs with different probability because contagion effects are different in response to the memory period<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\709db605-4ef9-41ee-866e-b363451c5a5e.png" xlink:type="simple"/></inline-formula>; The larger the memory periods get, the more tail gets fat.</p><p>In contrast, current study focuses on how the variance is reduced with IPS algorithm compared to the standard Monte Carlo. Due mainly to the computation of sampling with replacement according to the distribution (0.23) in the selection stage, IPS algorithm generally requires more time than the standard Monte Carlo. Although it obviously depends on input parameters, with the above parameter set of 25 names and in case of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\9946171c-6449-4650-8643-923690ec70c3.png" xlink:type="simple"/></inline-formula>, the calculation in IPS took approximately 1.03 times longer than that of standard Monte Carlo. Thus, in the rest of the paper, for comparison for accuracy, we take the number of trials in Monte Carlo equals to the number of the particles in IPS. In order to see the effectiveness of the IPS, we run both the Monte Carlo with <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\86f46f5e-2e0a-4e16-adee-50a80d3c181c.png" xlink:type="simple"/></inline-formula> trials and the IPS with <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\7056e60d-6d4d-4c32-aaa7-d09044a73c31.png" xlink:type="simple"/></inline-formula> particles for 1000 times for each, and then compare the sample standard deviation</p><p>of the 1000 outcomes of the probabilities <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\32cf954f-c6d0-4ef4-a5eb-bcaa7369794b.png" xlink:type="simple"/></inline-formula> for all <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\8cdc9302-b0e7-4c03-805b-81a81891e1d9.png" xlink:type="simple"/></inline-formula> More specifically, let</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\98e34580-6e0e-43fd-8060-35ce12168df9.png" xlink:type="simple"/></inline-formula>be <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\90779fcd-fd00-465e-9137-cb5f3e0d7afe.png" xlink:type="simple"/></inline-formula>-th outcome of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\387aa216-fa9a-47c5-a94d-546fb9bbbc1d.png" xlink:type="simple"/></inline-formula> obtained by the standard Monte Carlo and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\12a5f71b-99b4-4bb7-ae02-48446f5c846f.png" xlink:type="simple"/></inline-formula> be <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\4e614cfb-e463-4faf-8eeb-ad9205624a79.png" xlink:type="simple"/></inline-formula>-th</p><p>outcome of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\4e11096b-6cfd-4647-9966-849dd9c37889.png" xlink:type="simple"/></inline-formula> obtained by the IPS. Calculate the sample standard deviation of</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\5e227660-0839-4123-aaa0-20ca6842e0cf.png" xlink:type="simple"/></inline-formula>, denoted by<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\08e8ee47-39f2-4ca1-86f0-6946f25a23ee.png" xlink:type="simple"/></inline-formula>, and also calculate the sample standard deviation of</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\127db044-a5b0-4111-86d1-218d4bdca037.png" xlink:type="simple"/></inline-formula>, denoted by<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\db3ca760-d489-4338-81a0-4488cb43bb04.png" xlink:type="simple"/></inline-formula>. Finally compare the two values <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\b4f26d40-39f7-465a-b478-db323990c312.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\3a2517b0-fe2f-4294-88ab-faab644fa51b.png" xlink:type="simple"/></inline-formula> for each</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\d1348ebd-3760-4e05-97ca-d14d21553950.png" xlink:type="simple"/></inline-formula>and then we see which algorithm achieves low standard deviation. <xref ref-type="fig" rid="fig6">Figure 6</xref> and <xref ref-type="fig" rid="fig7">Figure 7</xref> illustrate the</p><p>differences between <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\8963ce16-8337-4a60-9ba7-43ddbc641bc6.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\c1e2f8d0-68ec-498f-8459-13dd21cf0012.png" xlink:type="simple"/></inline-formula> in Case 1.</p><p>And figure 8 and figure 9 illustrate the differences between <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\76360479-4a5c-4d89-a140-de6a6c349707.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\4f0ccb64-973c-4b52-92e2-7286b1b0ba11.png" xlink:type="simple"/></inline-formula> in Case 2.</p><p>Remarkable feature is that the IPS algorithm reduces variance for the rare events, i.e., more than 10 defaults in our example, while instead, demonstrates weak performance for<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\a0e58429-e188-48fb-bf77-3e8a5f375977.png" xlink:type="simple"/></inline-formula>. Therefore, whether to chose IPS depends on the objective and its assesment(division) might depends on the portfolio and the parameters. Thus, although we need several trial runs for the first time with given portfolio, once we get the suitable control parameters such as<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\4407200a-3227-4b5e-970b-83b0e5d37ef4.png" xlink:type="simple"/></inline-formula>, reliable results would be obtained.</p><fig id="fig6"><label>Figure 6</label><caption><p> Case 1: 1 ≤ k ≤ 7</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\b4dc2ef2-9a25-4898-ab52-c99deb0055a1.png"/></fig><fig id="fig7"><label>Figure 7</label><caption><p> Case 1: 8 ≤ k ≤ 25</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\370f11e2-053b-4bd9-b5ab-0f28b88448e7.png"/></fig><fig id="fig8"><label>Figure 8</label><caption><p> Case 2: 1 ≤ k ≤ 7</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\04dd2abf-371a-4f63-80c0-f968a22e84e4.png"/></fig><fig id="fig9"><label>Figure 9</label><caption><p> Case 2: 8 ≤ k ≤ 25</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\5-1490275x\cd0dcebe-34a4-46f1-865e-54d8cb9ac606.png"/></fig></sec><sec id="s6"><title>6. Conclusion</title><p>This paper proposed incomplete information multi-name structural model and its efficient Monte Carlo algorithm based on the Interacting Particle System. We extend naturally the CreditGrades model in the sense that we consider more than two firms in the portfolio and their asset correlation as well as the dependence structure of the default thresholds. For this purpose, we introduced the prior joint distribution of default thresholds among the public investors described by truncated normal distribution. Numerical experience demonstrated that the IPS algorithm can generate rare default events which normally requires numerous trials if relying upon a simple Monte Carlo simulation. Finally we verified the IPS algorithm reduces variance for the rare events.</p></sec><sec id="s7"><title>Acknowledgements</title><p>The author is grateful to participants of the RIMS Workshop on Financial Modeling and Analysis (FMA2013) at Kyoto and participants of the Quantitative Methods in Finance 2013 Conference (QMF 2013) at Sydney for valuable comments which helped to improve this paper.</p></sec></body><back><ref-list><title>References</title><ref id="scirp.46378-ref1"><label>1</label><mixed-citation publication-type="journal" xlink:type="simple"><name name-style="western"><surname>DAVIS</surname><given-names> M. </given-names></name>,<name name-style="western"><surname> LO</surname><given-names> V. </given-names></name>,<etal>et al</etal>. (<year>2001</year>)<article-title>DAVIS, M. AND LO, V.  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