<?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">AM</journal-id><journal-title-group><journal-title>Applied Mathematics</journal-title></journal-title-group><issn pub-type="epub">2152-7385</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/am.2016.714130</article-id><article-id pub-id-type="publisher-id">AM-69843</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  About the Mean Difference of the Inverse Normal Distribution
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Giovanni</surname><given-names>Girone</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Angela</surname><given-names>Maria D’Uggento</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Department of Economics and Mathematical Methods, University of Bari Aldo Moro, Bari, Italy</addr-line></aff><pub-date pub-type="epub"><day>17</day><month>08</month><year>2016</year></pub-date><volume>07</volume><issue>14</issue><fpage>1504</fpage><lpage>1509</lpage><history><date date-type="received"><day>9</day>	<month>June</month>	<year>2016</year></date><date date-type="rev-recd"><day>accepted</day>	<month>15</month>	<year>August</year>	</date><date date-type="accepted"><day>18</day>	<month>August</month>	<year>2016</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>
 
 
  The calculation of the mean difference for the inverse normal distribution can be obtained by a transformation of variable or a hard integration by parts. This paper shows a simpler formula of the mean difference of the inverse normal distribution that highlights the role of the two parameters on the mean difference of the model. It makes it easier to study the relation of the mean difference with the other indexes of variability for the inverse normal distribution.
 
</p></abstract><kwd-group><kwd>Mean Difference</kwd><kwd> Inverse Normal Distribution</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>In 1911, Corrado Gini published his study on the mean introducing an index, later called Gini’s mean difference, as a measure of inequality of a series of values instead of other indexes of variability which measure the spread of the values around a position index. The proposal of Gini is easily extended to the measure of inequality of a random variable. In the most important essays about continuous and discrete distributions [<xref ref-type="bibr" rid="scirp.69843-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.69843-ref2">2</xref>] no reference can be found to Gini mean difference Δ, while the other variability indexes, in particular the standard deviation and the mean deviation, are widely dealt with. The compact expressions of the mean difference for the normal distribution, for the uniform distribution and for the exponential distribution had long been known. In several recent studies [<xref ref-type="bibr" rid="scirp.69843-ref3">3</xref>] - [<xref ref-type="bibr" rid="scirp.69843-ref8">8</xref>] , compact expressions of the mean difference for almost all the continuous and discrete distribution models have been obtained. About a century after the proposal of Gini, those papers aimed at enhancing an index to measure the variability in the sense of the inequality rather than the spread. The formula of the mean difference of the inverse normal distribution is useful to analyze its relation with the parameters of the model and compare this behavior with those of other variability indexes (standard deviation, mean deviation). Further purpose is to integrate the characterization of the distribution models more than the other indexes of variability do. The above mentioned studies do not treat the formula of the mean difference for the Wald inverse normal distribution. The aim of this paper is to partly fill in this gap.</p></sec><sec id="s2"><title>2. The Inverse Normal Distribution</title><p>The density function of the inverse normal distribution is</p><disp-formula id="scirp.69843-formula681"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x6.png"  xlink:type="simple"/></disp-formula><p>The cumulative distribution function of the inverse normal distribution is</p><disp-formula id="scirp.69843-formula682"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x7.png"  xlink:type="simple"/></disp-formula><p>The cumulative distribution function can also be written as</p><disp-formula id="scirp.69843-formula683"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x8.png"  xlink:type="simple"/></disp-formula><p>in which</p><disp-formula id="scirp.69843-formula684"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x9.png"  xlink:type="simple"/></disp-formula><p>is the cumulative distribution function of the standard normal distribution.</p><p>The mean and the variance of this distribution are, respectively,</p><disp-formula id="scirp.69843-formula685"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x10.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.69843-formula686"><label>. (6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x11.png"  xlink:type="simple"/></disp-formula></sec><sec id="s3"><title>3. Calculation Procedure for the Mean Difference of a Continuous Distribution</title><p>A continuous distribution is characterized by the density function</p><disp-formula id="scirp.69843-formula687"><label>, (7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x12.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.69843-formula688"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x13.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.69843-formula689"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x14.png"  xlink:type="simple"/></disp-formula><p>or by the cumulative distribution function</p><disp-formula id="scirp.69843-formula690"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x15.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.69843-formula691"><label>, (11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x16.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.69843-formula692"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x17.png"  xlink:type="simple"/></disp-formula><p>Moreover, the first incomplete moment is</p><disp-formula id="scirp.69843-formula693"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x18.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.69843-formula694"><label>(14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x19.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.69843-formula695"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x20.png"  xlink:type="simple"/></disp-formula><p>In the previous formulas, a can be also equal to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403236x21.png" xlink:type="simple"/></inline-formula> and b equal to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403236x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403236x22.png" xlink:type="simple"/></inline-formula>.</p><p>To compute the mean difference of a continuous distribution between the two values x and y of the same random variable, one of the following four formulas can be used.</p><p>The direct formula is</p><disp-formula id="scirp.69843-formula696"><label>(16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x23.png"  xlink:type="simple"/></disp-formula><p>the formula based on the density function and the cumulative distribution function is</p><disp-formula id="scirp.69843-formula697"><label>(17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x24.png"  xlink:type="simple"/></disp-formula><p>another option is the formula based on the density function, the cumulative distribution function and the first incomplete moment is</p><disp-formula id="scirp.69843-formula698"><label>(18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x25.png"  xlink:type="simple"/></disp-formula><p>and, finally, the formula based solely on the cumulative distribution function is</p><disp-formula id="scirp.69843-formula699"><label>(19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x26.png"  xlink:type="simple"/></disp-formula><p>The previous four formulas are completely equivalent, although, depending on the models whose mean difference has to be calculated, some of them are easier to apply if compared to the others.</p></sec><sec id="s4"><title>4. Calculation Procedure for the Mean Difference of the Inverse Normal Distribution</title><p>If we consider the formula based on the cumulative distribution function, the mean difference is</p><disp-formula id="scirp.69843-formula700"><label>(20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x27.png"  xlink:type="simple"/></disp-formula><p>Replacing the cumulative distribution function of the inverse normal distribution, leads to</p><disp-formula id="scirp.69843-formula701"><label>, (21)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x28.png"  xlink:type="simple"/></disp-formula><p>in which there are the error function</p><disp-formula id="scirp.69843-formula702"><label>(22)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x29.png"  xlink:type="simple"/></disp-formula><p>and the complementary error function</p><disp-formula id="scirp.69843-formula703"><label>(23)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x30.png"  xlink:type="simple"/></disp-formula><p>The Error function is encountered in integrating the normal distribution, which is a normalized form of the Gaussian function. Then, introducing the transformation of the variable</p><disp-formula id="scirp.69843-formula704"><label>(24)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x31.png"  xlink:type="simple"/></disp-formula><p>and denoting</p><disp-formula id="scirp.69843-formula705"><label>(25)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x32.png"  xlink:type="simple"/></disp-formula><p>this formula is obtained</p><disp-formula id="scirp.69843-formula706"><label>(26)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x33.png"  xlink:type="simple"/></disp-formula><p>in which the integral depends solely on the parameter ϕ.</p><p>The function to be integrated, unless the constant 1/2, has the structure<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403236x34.png" xlink:type="simple"/></inline-formula>.</p><p>Introducing the transformation of variable</p><disp-formula id="scirp.69843-formula707"><label>(27)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x35.png"  xlink:type="simple"/></disp-formula><p>after heavy but direct calculations, the following expression is achieved</p><disp-formula id="scirp.69843-formula708"><label>(28)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x36.png"  xlink:type="simple"/></disp-formula><p>For simplicity, in the above formula the following transformation of the variable should be introduced</p><disp-formula id="scirp.69843-formula709"><label>(29)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x37.png"  xlink:type="simple"/></disp-formula><p>which, after further heavy but direct calculations, leads to</p><disp-formula id="scirp.69843-formula710"><label>(30)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x38.png"  xlink:type="simple"/></disp-formula><p>in which the integral exists for any value of μ and for φ &gt; 0. The analytical value of Δ is not known but its value can be easily numerically calculated.</p><p>The obtained expression is the simplest formula enabling to compute the mean difference of the inverse normal distribution. The above formula clearly highlights the role of the two parameters: one, μ, is a multiplicative factor and the other one, ϕ, is part of the function to be integrated.</p><p><xref ref-type="fig" rid="fig1">Figure 1</xref> shows the trend of the mean difference of the inverse normal distribution as function of the parameters μ and ϕ. It can be observed that Δ increases with the parameter μ and decreases as the parameter ϕ increases.</p><p>Through a transformation of variable or an integration by parts, several other equivalent formulas can be obtained, all of them needing an integration. Some of them are shown in the Appendix.</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Trend of the mean difference Δ of inverse normal distribution as function of the parameters μ and ϕ</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/5-7403236x39.png"/></fig></sec><sec id="s5"><title>5. Conclusive Remarks</title><p>In this paper, a simple formula of the mean difference of the inverse normal distribution is achieved. The formula is simpler than those obtainable by a transformation of variable or an integration by parts of the same. Even if the formula contains an integration to be computed, it is undoubtedly easy to calculate and allows to highlight the role of the two parameters on the mean difference of the model. It makes it easier to study the relation of the mean difference with the other indexes of variability for the inverse normal distribution.</p></sec><sec id="s6"><title>Cite this paper</title><p>Giovanni Girone,Angela Maria D’Uggento, (2016) About the Mean Difference of the Inverse Normal Distribution. Applied Mathematics,07,1504-1509. doi: 10.4236/am.2016.714130</p></sec><sec id="s7"><title>Appendix: Alternative Formulas for Calculating Δ for the Inverse Normal Distribution</title><disp-formula id="scirp.69843-formula711"><label>(31)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x40.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.69843-formula712"><label>(32)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x41.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.69843-formula713"><label>(33)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x42.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.69843-formula714"><label>(34)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x43.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.69843-formula715"><label>(35)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x44.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.69843-formula716"><label>(36)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x45.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.69843-formula717"><label>(37)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x46.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.69843-formula718"><label>(38)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x47.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.69843-formula719"><label>(39)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x48.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.69843-formula720"><label>(40)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x49.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.69843-formula721"><label>(41)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x50.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.69843-formula722"><label>(42)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x51.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.69843-formula723"><label>(43)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403236x52.png"  xlink:type="simple"/></disp-formula><p>Attributions Girone Sections 1, 2, 3 and the Appendix, D’Uggento Sections 4 and 5.</p></sec></body><back><ref-list><title>References</title><ref id="scirp.69843-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Norman, J.L., Samuel, K. and Narayanaswamy, B. 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