<?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.2016.77057</article-id><article-id pub-id-type="publisher-id">AM-65958</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>
 
 
  Solution of Linear Dynamical Systems Using Lucas Polynomials of the Second Kind
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>ierpaolo</surname><given-names>Natalini</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>Paolo</surname><given-names>E. Ricci</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>International Telematic University UniNettuno, Roma, Italia</addr-line></aff><aff id="aff1"><addr-line>Dipartimento di Matematica e Fisica, Largo San Leonardo Murialdo, Università degli Studi Roma Tre, Roma, Italia</addr-line></aff><pub-date pub-type="epub"><day>18</day><month>04</month><year>2016</year></pub-date><volume>07</volume><issue>07</issue><fpage>616</fpage><lpage>628</lpage><history><date date-type="received"><day>23</day>	<month>February</month>	<year>2016</year></date><date date-type="rev-recd"><day>accepted</day>	<month>24</month>	<year>April</year>	</date><date date-type="accepted"><day>27</day>	<month>April</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><html>
 <head></head>
 
  The use 
  <img src="Edit_390b5122-5d44-43db-9731-f38f3ae95e06.bmp" alt="" /> of functions, expressible in terms of Lucas polynomials of the second kind, allows us to write down the solution of linear dynamical systems—both in the discrete and continuous case—avoiding the Jordan canonical form of involved matrices. This improves the computational complexity of the algorithms used in literature.
 
</html></p></abstract><kwd-group><kwd>Matrix Powers</kwd><kwd> Linear Dynamical Systems</kwd><kwd> Exponential Matrix</kwd><kwd> Lucas Polynomials of the Second Kind</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Even in recent books (see e.g. [<xref ref-type="bibr" rid="scirp.65958-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.65958-ref2">2</xref>] ), the solution of linear dynamical systems, both in the discrete or continuous time case, is expressed by using all powers of the considered matrix<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x7.png" xlink:type="simple"/></inline-formula>. As a consequence, if we want to write down explicitly the solution, it is necessary to construct the Jordan canonical form of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x8.png" xlink:type="simple"/></inline-formula> and, in the case of a defective matrix (i.e. if non trivial Jordan blocks appear in its canonical form), this implies cumbersome computations.</p><p>In order to avoid this serious problem, we propose here an alternative method, based on recursion, using the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x9.png" xlink:type="simple"/></inline-formula> functions, which are essentially linked to Lucas polynomials of the second kind [<xref ref-type="bibr" rid="scirp.65958-ref3">3</xref>] (i.e. the basic solution of a homogeneous linear recurrence relation with constant coefficients [<xref ref-type="bibr" rid="scirp.65958-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.65958-ref5">5</xref>] ), and to the multi-variable Chebyshev polynomials [<xref ref-type="bibr" rid="scirp.65958-ref6">6</xref>] .</p><p>After recalling the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x10.png" xlink:type="simple"/></inline-formula> functions and their connections with matrix powers [<xref ref-type="bibr" rid="scirp.65958-ref7">7</xref>] , we can show, in Section 2, that the use of matrix powers and matrix function representations (see e.g. [<xref ref-type="bibr" rid="scirp.65958-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.65958-ref8">8</xref>] ) gives us the possibility to use only powers of the considered matrix up to (at most) the order<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x11.png" xlink:type="simple"/></inline-formula>. This is a trivial consequence of the Cayley-Hamilton theorem, and should be used, in our opinion, to reduce the computational cost of solutions. Another shown possibility is the use of the Riesz-Fantappi&#232; formula, by means of which the Taylor expansion of solution is completely avoided.</p><p>In Section 3, we prove our main results, relevant to an alternative method for the solution of linear dynamical systems, both in the discrete and continuous time case and via the Riesz-Fantappi&#232; formula, also known in literature as the Dunford-Schwartz formula [<xref ref-type="bibr" rid="scirp.65958-ref9">9</xref>] , (but the priority of the first Authors is undubtable).</p><p>Some concrete examples of computation are presented in Section 4, showing the more simple complexity of our procedure with respect to the traditional algorithms, as they appear in the above mentioned books.</p><p>We want to remark explicitly that, in our article, by using the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x12.png" xlink:type="simple"/></inline-formula> functions (essentially linked to Lucas polynomials of the second kind), our methodology builds a bridge, to our knowledge not previously well known, between the Theory of Matrices and that of Special Functions, which are usually considered as very different fields. Furthermore, the use of the Riesz-Fantappi&#232; formula reduces to a finite computation the algorithms used in literature, making use of series expansions, and consequently dramatically improves the computation com- plexity of the considered problem.</p><sec id="s1_1"><title>1.1. Recalling F<sub>k</sub><sub>,n</sub> Functions</title><p>Consider the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x13.png" xlink:type="simple"/></inline-formula>-terms homogeneous linear bilateral recurrence relation with (real or complex) constant (with respect to n) coefficients <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x14.png" xlink:type="simple"/></inline-formula> where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x15.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.65958-formula2721"><label>(1.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403103x16.png"  xlink:type="simple"/></disp-formula><p>Supposing the coefficients vary, its solution is given by every bilateral sequence <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x17.png" xlink:type="simple"/></inline-formula> such</p><p>that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x18.png" xlink:type="simple"/></inline-formula> consecutive terms satisfy Equation (1.1).</p><p>A basis for the r-dimensional vectorial space <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x19.png" xlink:type="simple"/></inline-formula> of solutions is given by the functions <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x20.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x21.png" xlink:type="simple"/></inline-formula>, defined by the initial conditions below:</p><disp-formula id="scirp.65958-formula2722"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x22.png"  xlink:type="simple"/></disp-formula><p>Since<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x23.png" xlink:type="simple"/></inline-formula>, the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x24.png" xlink:type="simple"/></inline-formula> functions can be defined even if<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x25.png" xlink:type="simple"/></inline-formula>, by means of the positions:</p><disp-formula id="scirp.65958-formula2723"><label>(1.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403103x26.png"  xlink:type="simple"/></disp-formula><p>Therefore, assuming the initial conditions <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x27.png" xlink:type="simple"/></inline-formula> the general solution of the recurrence (1.1), <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x28.png" xlink:type="simple"/></inline-formula>, is given by</p><disp-formula id="scirp.65958-formula2724"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x29.png"  xlink:type="simple"/></disp-formula><p>For further considerations, relevant to the classical method for solving the recurrence (1.1), see [<xref ref-type="bibr" rid="scirp.65958-ref5">5</xref>] .</p><p>An important result, originally stated by &#201; Lucas [<xref ref-type="bibr" rid="scirp.65958-ref3">3</xref>] (in the particular case<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x30.png" xlink:type="simple"/></inline-formula>), is given by the equations</p><disp-formula id="scirp.65958-formula2725"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x31.png"  xlink:type="simple"/></disp-formula><p>showing that all <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x32.png" xlink:type="simple"/></inline-formula> functions are expressed through the only bilateral sequence<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x32.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x33.png" xlink:type="simple"/></inline-formula>.</p><p>Therefore, we assume the following</p><p>Definition 1-The bilateral sequence<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x34.png" xlink:type="simple"/></inline-formula>, solution of (1.1) corresponding to the initial conditions:</p><disp-formula id="scirp.65958-formula2726"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x35.png"  xlink:type="simple"/></disp-formula><p>is called the fundamental solution of (1.1) (“fonction fondamentale” by &#201;. Lucas [<xref ref-type="bibr" rid="scirp.65958-ref3">3</xref>] ), [<xref ref-type="bibr" rid="scirp.65958-ref4">4</xref>] .</p><p>For the connection with Chebyshev polynomials of the second kind in several variables, see [<xref ref-type="bibr" rid="scirp.65958-ref6">6</xref>] .</p></sec><sec id="s1_2"><title>1.2. Matrix Powers Representation</title><p>In preceding articles [<xref ref-type="bibr" rid="scirp.65958-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.65958-ref7">7</xref>] , the following result is proved:</p><p>Theorem 1 Given an <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x36.png" xlink:type="simple"/></inline-formula> matrix<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x37.png" xlink:type="simple"/></inline-formula>, putting by definition<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x38.png" xlink:type="simple"/></inline-formula>, and denoting by</p><disp-formula id="scirp.65958-formula2727"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x39.png"  xlink:type="simple"/></disp-formula><p>its characteristic polynomial (or possibly its minimal polynomial, if this is known), the matrix powers<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x40.png" xlink:type="simple"/></inline-formula>, with integral exponent n, are given by the equation:</p><disp-formula id="scirp.65958-formula2728"><label>(1.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403103x41.png"  xlink:type="simple"/></disp-formula><p>where the functions <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x42.png" xlink:type="simple"/></inline-formula> are defined in Section 1.1.</p><p>Moreover, if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x43.png" xlink:type="simple"/></inline-formula> is not singular, i.e.<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x44.png" xlink:type="simple"/></inline-formula>, Equation (1.3) still works for negative integers n, assuming the definition (1.2) for the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x45.png" xlink:type="simple"/></inline-formula> functions.</p><p>It is worth to recall that the knowledge of eigenvalues is equivalent to that of invariants, since the second ones are the elementary symmetric functions of the first ones.</p><p>Remark 1 Note that, as a consequence of the above result, the higher powers of matrix <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x46.png" xlink:type="simple"/></inline-formula> are always expressible in terms of the lower ones (at most up to the dimension of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x46.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x47.png" xlink:type="simple"/></inline-formula>).</p></sec></sec><sec id="s2"><title>2. Matrix Functions Representation</title><p>It is well known that an analytic function f of a matrix<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x48.png" xlink:type="simple"/></inline-formula>, i.e.<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x49.png" xlink:type="simple"/></inline-formula>, is the matrix polynomial obtained from the scalar polynomial interpolating the function f on the eigenvalues of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x50.png" xlink:type="simple"/></inline-formula> (see e.g. the Gantmacher book [<xref ref-type="bibr" rid="scirp.65958-ref8">8</xref>] ), however, in many books (see e.g. [<xref ref-type="bibr" rid="scirp.65958-ref1">1</xref>] ), the series expansion</p><disp-formula id="scirp.65958-formula2729"><label>(2.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403103x51.png"  xlink:type="simple"/></disp-formula><p>is assumed for defining (and computing)<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x52.png" xlink:type="simple"/></inline-formula>. So, apparently, the series expansion for the exponential of a matrix is “hard to die”.</p><p>Let <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x53.png" xlink:type="simple"/></inline-formula> the spectrum of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x54.png" xlink:type="simple"/></inline-formula>. Denoting by</p><disp-formula id="scirp.65958-formula2730"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x55.png"  xlink:type="simple"/></disp-formula><p>the polynomial interpolating <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x56.png" xlink:type="simple"/></inline-formula> on<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x57.png" xlink:type="simple"/></inline-formula>, i.e. such that:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x57.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x58.png" xlink:type="simple"/></inline-formula>,</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x59.png" xlink:type="simple"/></inline-formula>, then</p><disp-formula id="scirp.65958-formula2731"><label>(2.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403103x60.png"  xlink:type="simple"/></disp-formula><p>If the eigenvalues are all distinct, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x61.png" xlink:type="simple"/></inline-formula>coincides with the Lagrange interpolation polynomial and (2.2) is the Lagrange-Sylvester formula. In case of multiple eigenvalues, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x62.png" xlink:type="simple"/></inline-formula>is the Hermite interpolation polynomial, and (2.2) reduces to Arthur Buchheim's formula, generalizing the preceding one.</p><p>This avoids the use of higher powers of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x63.png" xlink:type="simple"/></inline-formula> in the Taylor expansion (2.1). In any case, the possibility to write<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x64.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x65.png" xlink:type="simple"/></inline-formula>, in an easy block form, requires not only the knowledge of the spectrum, but even the Jordan canonical form of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x66.png" xlink:type="simple"/></inline-formula>. It is necessary to compute the eigenvectors and moreover the principal vectors, if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x66.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x67.png" xlink:type="simple"/></inline-formula> is defective. A known machinery which implies a lot of computations.</p>The Riesz-Fantappi&#232; Formula<p>A classical result is as follows:</p><p>Theorem 2 Under the hypotheses and definitions considered above, the resolvent matrix <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x68.png" xlink:type="simple"/></inline-formula> can be represented as</p><disp-formula id="scirp.65958-formula2732"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x69.png"  xlink:type="simple"/></disp-formula><p>Then, by the Riesz-Fantappi&#232; formula, we recover the classical result:</p><p>Theorem 3 If <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x70.png" xlink:type="simple"/></inline-formula> is a holomorphic function in the domain <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x71.png" xlink:type="simple"/></inline-formula> and denoting by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x72.png" xlink:type="simple"/></inline-formula> (with<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x73.png" xlink:type="simple"/></inline-formula>) a closed set whose boundary is a piecewise simple Jordan contour <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x74.png" xlink:type="simple"/></inline-formula> encompassing the spectrum <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x75.png" xlink:type="simple"/></inline-formula> of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x75.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x76.png" xlink:type="simple"/></inline-formula>, the matrix function <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x75.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x77.png" xlink:type="simple"/></inline-formula> can be represented by:</p><disp-formula id="scirp.65958-formula2733"><label>(2.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403103x78.png"  xlink:type="simple"/></disp-formula><p>In particular:</p><disp-formula id="scirp.65958-formula2734"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x79.png"  xlink:type="simple"/></disp-formula><p>Remark 2 If the eigenvalues of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x80.png" xlink:type="simple"/></inline-formula>, are known, Equation (2.3), by the residue theorem, gives back the Lagrange-Sylvester representation. However, for computing the integrals appearing in Equation (2.3) it is sufficient the knowledge of a circle D, (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x81.png" xlink:type="simple"/></inline-formula>), containing the spectrum of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x82.png" xlink:type="simple"/></inline-formula> (by using the Gerschgorin theorem, and then knowing only the entries of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x82.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x83.png" xlink:type="simple"/></inline-formula>, without computing its eigenvalues). Therefore, this approach is computationally more convenient with respect to the Lagrange-Sylvester formula.</p></sec><sec id="s3"><title>3. Solution of Linear Dynamical Systems Via F<sub>k</sub><sub>,n</sub> Functions</title><p>As a consequence of the above recalled results, we can prove our main results both in the discrete and continuous time case.</p><sec id="s3_1"><title>3.1. The Discrete Time Case</title><p>Theorem 4 Consider the dynamical problem for the homogeneous linear recurrence system</p><disp-formula id="scirp.65958-formula2735"><label>(3.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403103x84.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.65958-formula2736"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x85.png"  xlink:type="simple"/></disp-formula><p>Let</p><disp-formula id="scirp.65958-formula2737"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x86.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2738"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x87.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2739"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x88.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2740"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x89.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2741"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x90.png"  xlink:type="simple"/></disp-formula><p>denote by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x91.png" xlink:type="simple"/></inline-formula> the invariants of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x91.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x92.png" xlink:type="simple"/></inline-formula>, and recall the generalized Lucas polynomials<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x91.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x92.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x93.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x91.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x92.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x93.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x94.png" xlink:type="simple"/></inline-formula>, defined in Section 1.1.</p><p>Define the vector</p><disp-formula id="scirp.65958-formula2742"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x95.png"  xlink:type="simple"/></disp-formula><p>and the matrix</p><disp-formula id="scirp.65958-formula2743"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x96.png"  xlink:type="simple"/></disp-formula><p>then, the solution of problem (3.1) can be written</p><disp-formula id="scirp.65958-formula2744"><label>(3.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403103x97.png"  xlink:type="simple"/></disp-formula><p>That is, for the components:</p><disp-formula id="scirp.65958-formula2745"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x98.png"  xlink:type="simple"/></disp-formula><p>Proof It is well known that the solution of problem (3.1) is given by</p><disp-formula id="scirp.65958-formula2746"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x99.png"  xlink:type="simple"/></disp-formula><p>From the results about matrix powers, it follows that</p><disp-formula id="scirp.65958-formula2747"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x100.png"  xlink:type="simple"/></disp-formula><p>Then, taking into account the above definitions of vectors <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x101.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x102.png" xlink:type="simple"/></inline-formula> our result follows.</p><p>Remark 3 Note that, even if this is unrealistic, solution (3.2) still holds for negative values of n, assuming definition (1.2) for the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x103.png" xlink:type="simple"/></inline-formula> functions when<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x103.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x104.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s3_2"><title>3.2. The Continuous Time Case</title><p>Theorem 5 Consider the Cauchy problem for the homogeneous linear differential system</p><disp-formula id="scirp.65958-formula2748"><label>(3.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403103x105.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x106.png" xlink:type="simple"/></inline-formula> is the same matrix considered in the discrete time case.</p><p>Let</p><disp-formula id="scirp.65958-formula2749"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x107.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2750"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x108.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2751"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x109.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2752"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x110.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2753"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x111.png"  xlink:type="simple"/></disp-formula><p>denote by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x112.png" xlink:type="simple"/></inline-formula> the invariants of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x112.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x113.png" xlink:type="simple"/></inline-formula>, and recall again the generalized Lucas polynomials<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x112.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x113.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x114.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x112.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x113.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x114.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x115.png" xlink:type="simple"/></inline-formula>.</p><p>Introduce the matrix <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x116.png" xlink:type="simple"/></inline-formula> and define the vector function</p><disp-formula id="scirp.65958-formula2754"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x117.png"  xlink:type="simple"/></disp-formula><p>then, the solution of problem (3.3) can be written</p><disp-formula id="scirp.65958-formula2755"><label>(3.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403103x118.png"  xlink:type="simple"/></disp-formula><p>Proof-It is well known that the solution of problem (3.3) is given by</p><disp-formula id="scirp.65958-formula2756"><label>(3.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403103x119.png"  xlink:type="simple"/></disp-formula><p>From the results about matrix exponential, it follows that</p><disp-formula id="scirp.65958-formula2757"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x120.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.65958-formula2758"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x121.png"  xlink:type="simple"/></disp-formula><p>so that Equation (3.5) becomes</p><disp-formula id="scirp.65958-formula2759"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x122.png"  xlink:type="simple"/></disp-formula><p>and taking into account the above positions, it follows</p><disp-formula id="scirp.65958-formula2760"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x123.png"  xlink:type="simple"/></disp-formula><p>Then, Equation (3.4) immediately follows by introducing the vector function <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x124.png" xlink:type="simple"/></inline-formula> and the matrix <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x124.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x125.png" xlink:type="simple"/></inline-formula> defined above.</p><p>Remark 4 Note that the convergence of the vectorial series in any compact set K of the space <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x126.png" xlink:type="simple"/></inline-formula> is guaranteed, as the components of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x126.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x127.png" xlink:type="simple"/></inline-formula> are polynomials of weight not exceeding<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x126.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x127.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x128.png" xlink:type="simple"/></inline-formula>, and consequently are bounded in K.</p></sec><sec id="s3_3"><title>3.3. The Continuous Case, Via the Riesz-Fantappi&#232; Formula</title><p>By using the Riesz-Fantappi&#232; it is possible to avoid series expansions. Indeed, we can prove the following result.</p><p>Theorem 6 The solution of the Cauchy problem (3.3) can be found in the form</p><disp-formula id="scirp.65958-formula2761"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x129.png"  xlink:type="simple"/></disp-formula><p>where we denoted by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x130.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x130.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x131.png" xlink:type="simple"/></inline-formula>the invariants of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x130.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x131.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x132.png" xlink:type="simple"/></inline-formula> and by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x130.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x131.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x132.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x133.png" xlink:type="simple"/></inline-formula> its characteristic polynomial.</p><p>Proof It is a straightforward application of the Riesz-Fantappi&#232; formula, taking into account the definition of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x134.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x134.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x135.png" xlink:type="simple"/></inline-formula>.</p></sec></sec><sec id="s4"><title>4. Worked Examples</title><p>We show that the above results are easier with respect to the methods usually presented in literature ( [<xref ref-type="bibr" rid="scirp.65958-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.65958-ref2">2</xref>] ). Our technique is as follows: if the matrix <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x136.png" xlink:type="simple"/></inline-formula> has a low dimension (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x136.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x137.png" xlink:type="simple"/></inline-formula>), its invariants can be computed directly by hand. If <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x136.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x137.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x138.png" xlink:type="simple"/></inline-formula> it is more easy to compute the eigenvalues by using one of the classical numerical methods, and then the invariants are found as the elementary symmetric functions (with alternate sign) of the eigenvalues. This completely avoids the construction of the Jordan canonical form. No necessity to compute higher powers of matrix<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x136.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x137.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x138.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x139.png" xlink:type="simple"/></inline-formula>.</p><sec id="s4_1"><title>4.1. Example 1 (Discrete Time Case)</title><p>We consider the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x140.png" xlink:type="simple"/></inline-formula> system</p><disp-formula id="scirp.65958-formula2762"><label>(4.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403103x141.png"  xlink:type="simple"/></disp-formula><p>with matrix<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x142.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.65958-formula2763"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x143.png"  xlink:type="simple"/></disp-formula><p>The invariants of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x144.png" xlink:type="simple"/></inline-formula> are by definition:</p><disp-formula id="scirp.65958-formula2764"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x145.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2765"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x146.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2766"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x147.png"  xlink:type="simple"/></disp-formula><p>We will consider, the initial conditions:</p><disp-formula id="scirp.65958-formula2767"><label>(4.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403103x148.png"  xlink:type="simple"/></disp-formula><p>Then, as a consequence, we have:</p><disp-formula id="scirp.65958-formula2768"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x149.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.65958-formula2769"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x150.png"  xlink:type="simple"/></disp-formula><p>Starting from the initial conditions:</p><disp-formula id="scirp.65958-formula2770"><label>(4.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403103x151.png"  xlink:type="simple"/></disp-formula><p>and by means of the recurrence relation</p><disp-formula id="scirp.65958-formula2771"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x152.png"  xlink:type="simple"/></disp-formula><p>with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x153.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x153.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x154.png" xlink:type="simple"/></inline-formula>, we find the following solution of the discrete dynamical system problem (4.1)-(4.2)</p><disp-formula id="scirp.65958-formula2772"><label>(4.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403103x155.png"  xlink:type="simple"/></disp-formula><p>The (4.4) coincides with the following solution of the problem (4.1)-(4.2) obtained with the classical method of eigenvalues</p><disp-formula id="scirp.65958-formula2773"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x156.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2774"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x157.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2775"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x158.png"  xlink:type="simple"/></disp-formula></sec><sec id="s4_2"><title>4.2. Example 2 (Continuous Time Case)</title><p>We consider the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x159.png" xlink:type="simple"/></inline-formula> system</p><disp-formula id="scirp.65958-formula2776"><label>(4.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403103x160.png"  xlink:type="simple"/></disp-formula><p>with matrix<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x161.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.65958-formula2777"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x162.png"  xlink:type="simple"/></disp-formula><p>The invariants of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x163.png" xlink:type="simple"/></inline-formula> are by definition:</p><disp-formula id="scirp.65958-formula2778"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x164.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2779"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x165.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2780"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x166.png"  xlink:type="simple"/></disp-formula><p>We will consider, the Cauchy problem with initial conditions:</p><disp-formula id="scirp.65958-formula2781"><label>(4.6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403103x167.png"  xlink:type="simple"/></disp-formula><p>Then, as a consequence, we have:</p><disp-formula id="scirp.65958-formula2782"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x168.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.65958-formula2783"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x169.png"  xlink:type="simple"/></disp-formula><p>Starting from the initial conditions (4.3) and by means of the recurrence relation</p><disp-formula id="scirp.65958-formula2784"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x170.png"  xlink:type="simple"/></disp-formula><p>with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x171.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x171.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x172.png" xlink:type="simple"/></inline-formula>, we find the following first values for the generalized Lucas polynomials <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x171.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x172.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x173.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.65958-formula2785"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x174.png"  xlink:type="simple"/></disp-formula><p>Here we compute an approximation of the solution of the Cauchy problem obtained by a suitable truncation of order N of the Taylor expansion</p><disp-formula id="scirp.65958-formula2786"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x175.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2787"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x176.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2788"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x177.png"  xlink:type="simple"/></disp-formula><p>The exact solution of the Cauchy problem (4.5)-(4.6) is</p><disp-formula id="scirp.65958-formula2789"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x178.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2790"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x179.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2791"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x180.png"  xlink:type="simple"/></disp-formula><p>such that we can compute, by using a Mathematica program, the approximation error obtained, for some values of N, in a fixed points t of the real axes. For example for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x181.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x181.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x182.png" xlink:type="simple"/></inline-formula> we obtain</p><disp-formula id="scirp.65958-formula2792"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x183.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2793"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x184.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2794"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x185.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2795"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x186.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2796"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x187.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2797"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x188.png"  xlink:type="simple"/></disp-formula></sec><sec id="s4_3"><title>4.3. Example 3 (Continuous Time Case)</title><p>We consider the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x189.png" xlink:type="simple"/></inline-formula> system</p><disp-formula id="scirp.65958-formula2798"><label>(4.7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403103x190.png"  xlink:type="simple"/></disp-formula><p>with matrix<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x191.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.65958-formula2799"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x192.png"  xlink:type="simple"/></disp-formula><p>The invariants of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x193.png" xlink:type="simple"/></inline-formula> are:</p><disp-formula id="scirp.65958-formula2800"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x194.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2801"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x195.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2802"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x196.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2803"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x197.png"  xlink:type="simple"/></disp-formula><p>We will consider, the Cauchy problem with initial conditions:</p><disp-formula id="scirp.65958-formula2804"><label>(4.8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-7403103x198.png"  xlink:type="simple"/></disp-formula><p>Then, as a consequence, we have:</p><disp-formula id="scirp.65958-formula2805"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x199.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2806"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x200.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.65958-formula2807"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x201.png"  xlink:type="simple"/></disp-formula><p>Starting from the initial conditions:</p><disp-formula id="scirp.65958-formula2808"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x202.png"  xlink:type="simple"/></disp-formula><p>and by means of the recurrence relation</p><disp-formula id="scirp.65958-formula2809"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x203.png"  xlink:type="simple"/></disp-formula><p>with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x204.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x204.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x205.png" xlink:type="simple"/></inline-formula>, we find the following first values for the generalized Lucas polynomials<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x204.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x205.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x206.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.65958-formula2810"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x207.png"  xlink:type="simple"/></disp-formula><p>Here we compute an approximation of the solution of the Cauchy problem obtained by a suitable truncation of the Taylor expansion</p><disp-formula id="scirp.65958-formula2811"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x208.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2812"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x209.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2813"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x210.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2814"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x211.png"  xlink:type="simple"/></disp-formula></sec><sec id="s4_4"><title>4.4. Example 4 (Using the Riesz-Fantappi&#232; Formula)</title><p>Consider the problem</p><disp-formula id="scirp.65958-formula2815"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x212.png"  xlink:type="simple"/></disp-formula><p>with matrix</p><disp-formula id="scirp.65958-formula2816"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x213.png"  xlink:type="simple"/></disp-formula><p>Characteristic polynomial</p><disp-formula id="scirp.65958-formula2817"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x214.png"  xlink:type="simple"/></disp-formula><p>Matrix eigenvalues</p><disp-formula id="scirp.65958-formula2818"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x215.png"  xlink:type="simple"/></disp-formula><p>Matrix invariants</p><disp-formula id="scirp.65958-formula2819"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x216.png"  xlink:type="simple"/></disp-formula><p>From the initial condition</p><disp-formula id="scirp.65958-formula2820"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x217.png"  xlink:type="simple"/></disp-formula><p>we find</p><disp-formula id="scirp.65958-formula2821"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x218.png"  xlink:type="simple"/></disp-formula><p>Riesz-Fantappi&#232; formula</p><disp-formula id="scirp.65958-formula2822"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x219.png"  xlink:type="simple"/></disp-formula><p>i.e.</p><disp-formula id="scirp.65958-formula2823"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x220.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2824"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x221.png"  xlink:type="simple"/></disp-formula><p>Integrals computation (using the Residue Theorem).</p><disp-formula id="scirp.65958-formula2825"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x222.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2826"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x223.png"  xlink:type="simple"/></disp-formula><p>Solution of the problem</p><disp-formula id="scirp.65958-formula2827"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x224.png"  xlink:type="simple"/></disp-formula><p>i.e.</p><disp-formula id="scirp.65958-formula2828"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x225.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2829"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x226.png"  xlink:type="simple"/></disp-formula><p>Checking our result</p><disp-formula id="scirp.65958-formula2830"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x227.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2831"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x228.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.65958-formula2832"><graphic  xlink:href="http://html.scirp.org/file/5-7403103x229.png"  xlink:type="simple"/></disp-formula></sec></sec><sec id="s5"><title>5. Conclusions</title><p>We have recalled that the exponential <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x230.png" xlink:type="simple"/></inline-formula> of a matrix <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x230.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x231.png" xlink:type="simple"/></inline-formula> can be written as a matrix polynomial, obtained from the scalar polynomial interpolating <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x230.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x231.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x232.png" xlink:type="simple"/></inline-formula> on the spectrum of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x230.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x231.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x232.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x233.png" xlink:type="simple"/></inline-formula>, and then avoiding the Taylor expansion for the exponential matrix.</p><p>By using the functions<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x234.png" xlink:type="simple"/></inline-formula>, and in particular the fundamental solution of a homogeneous linear recurrence relation, i.e. the generalized Lucas polynomials of the second kind, we have shown how to obtain the solution of vectorial dynamical problems, both in the discrete (3.1) and continuous (3.3) case, in terms of functions of the invariants of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x234.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x235.png" xlink:type="simple"/></inline-formula>, instead of powers of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x234.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x235.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x236.png" xlink:type="simple"/></inline-formula>. These functions are independent of the Jordan canonical form of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x234.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x235.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x236.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x237.png" xlink:type="simple"/></inline-formula>, and can be computed recursively, avoiding the knowledge of eigenvectors and principal vectors of the con- sidered matrices. Moreover, if the matrix is real, the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x234.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x235.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x236.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x237.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-7403103x238.png" xlink:type="simple"/></inline-formula> functions are real as well, and complex eigenvalues do not affect the form of the solution.</p><p>Furthermore, the use of the Riesz-Fantappi&#232; formula (Sections 3.3 and 4.4) reduces to a finite computation the algorithms used in literature.</p><p>Therefore, the methods considered in this article are more convenient, with respect to those usually found in literature, for solving linear dynamical systems.</p></sec><sec id="s6"><title>Cite this paper</title><p>Pierpaolo Natalini,Paolo E. 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