<?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">JAMP</journal-id><journal-title-group><journal-title>Journal of Applied Mathematics and Physics</journal-title></journal-title-group><issn pub-type="epub">2327-4352</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jamp.2015.35070</article-id><article-id pub-id-type="publisher-id">JAMP-56756</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>
 
 
  Neutrality Criteria for Stability Analysis of Dynamical Systems through Lorentz and Rossler Model Problems
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>vgeniy</surname><given-names>Perevoznikov</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Olga</surname><given-names>Mikhailova</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>St. Petersburg State University of Trade and Economics, Petersburg, Russia</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>eperevoznikov@yandex.ru(VP)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>11</day><month>05</month><year>2015</year></pub-date><volume>03</volume><issue>05</issue><fpage>569</fpage><lpage>576</lpage><history><date date-type="received"><day>18</day>	<month>March</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>24</month>	<year>May</year>	</date><date date-type="accepted"><day>28</day>	<month>May</month>	<year>2015</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>
 
 
  Two methods of stability analysis of systems described by dynamical equations are being considered. They are based on an analysis of eigenvalues spectrum for the evolutionary matrix or the spectral equation and they allow determining the conditions of stability and instability, as well as the possibility of chaotic behavior of systems in case of a stability loss. The methods are illustrated for nonlinear Lorenz and Rossler model problems.
 
</p></abstract><kwd-group><kwd>Nonlinear Dynamical Systems</kwd><kwd> Stability Analysis Methods</kwd><kwd> Dynamical Chaos</kwd><kwd> Lorenz and R&#246;ssler Model Problems</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The work is dedicated to the methods of practical stability analysis for systems described by nonlinear autonomous equations. The analysis of such systems is of a particular interest due to the dynamical chaos phenomena, which can be observed in cases of stability loss [<xref ref-type="bibr" rid="scirp.56756-ref1">1</xref>] -[<xref ref-type="bibr" rid="scirp.56756-ref3">3</xref>] . A stability analysis of nonlinear Lorenz and R&#246;ssler systems [<xref ref-type="bibr" rid="scirp.56756-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.56756-ref3">3</xref>] is used as an example, illustrating the possibilities of the suggested methods.</p></sec><sec id="s2"><title>2. Stability Analysis Methods</title><p>The more common methods of system stability investigation are the spectral methods, which consist of dynamics spectrum analysis for small perturbations. The problem is defined in the following way.</p><p>Let’s assume that the system state is defined by a combination of macroscopic characteristics <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x5.png" xlink:type="simple"/></inline-formula> complying with the motion equations</p><disp-formula id="scirp.56756-formula775"><label>. (1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x6.png"  xlink:type="simple"/></disp-formula><p>The linearization of these equations leads to a system of equations describing the dynamics of small perturbations <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x7.png" xlink:type="simple"/></inline-formula> of the initial state <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x8.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.56756-formula776"><label>. (2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x9.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.56756-formula777"><graphic  xlink:href="http://html.scirp.org/file/13-1720246x10.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x11.png" xlink:type="simple"/></inline-formula>―are the elements of the evolutionary matrix operator, which in general depend on initial state parameters, coordinates―<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x12.png" xlink:type="simple"/></inline-formula>, time―<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x13.png" xlink:type="simple"/></inline-formula>, gradients―<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x14.png" xlink:type="simple"/></inline-formula>, integral operators of space and time convolution type―<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x15.png" xlink:type="simple"/></inline-formula>.</p><p>The condition of solvability of the system (2) which is its spectral equation―(SE)</p><disp-formula id="scirp.56756-formula778"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x16.png"  xlink:type="simple"/></disp-formula><p>defines the eigenvalues spectrum―<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x17.png" xlink:type="simple"/></inline-formula>of the evolutionary operator and the stability of the initial state―<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x18.png" xlink:type="simple"/></inline-formula>.</p><p>In the Fourier-Laplace transform for the perturbations in case of stationary initial states and also in cases when the initial dependences are weak in comparison with the high-speed and high-gradient perturbations (method of local dispersion relation (LDR)), the spectral equation acquires polynomial form</p><disp-formula id="scirp.56756-formula779"><label>, (4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x19.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x20.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x21.png" xlink:type="simple"/></inline-formula>―are the parameters of the Fourier-Laplace transform,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x22.png" xlink:type="simple"/></inline-formula>―are the complex coefficients of SE.</p><p>In the classical posing of the stability analysis problem, it comes down to the analysis of spectral equation roots.</p><p>The indication of an instability is the presence of a SE root with positive real part Re<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x23.png" xlink:type="simple"/></inline-formula>. If all the SE roots have negative real parts, the initial state described by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x24.png" xlink:type="simple"/></inline-formula>―is stable.</p><p>Due to the fact that the exact solution of Equation (4) with complex coefficients for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x25.png" xlink:type="simple"/></inline-formula> is impossible to obtain, fixed sign property criteria of real part of the root are being used-Routh-Hurwitz criterion, D-decompo- sition method, frequency criteria. However, their effectiveness is not very high because of their crockness and calculation complexity, especially during the analysis of significantly instable systems. In actual practice, it is more common to use numerical methods or look for special criteria applied to several problem types (energy in the theory of plasma stability and hydrodynamics, criteria for negative differential conductivity in problems on the carrier drift stability in strong energy fields/4/). But any specific criterion is not universal; numeric solutions do not allow obtaining stability conditions in analytical form and viewing their dependencies on parameters. They require a large amount of calculations.</p><p>In studies [<xref ref-type="bibr" rid="scirp.56756-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.56756-ref5">5</xref>] two methods of practical stability analysis for systems described by Equation (1) are suggested. They are called-the neutrality criteria. In studies [<xref ref-type="bibr" rid="scirp.56756-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.56756-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.56756-ref7">7</xref>] examples of their appliance is demonstrated. The essence of these methods lies in the determination of the neutral surface―a border separating the areas of stability and instability in the parametric space―using the dynamical equations coefficients (2) or the spectral equations coefficients (4).</p><p>1) NSE (neutrality, separation, exclusion) method is based on the spectral Equation (4) and it is implemented according to the following outline <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x26.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.56756-formula780"><graphic  xlink:href="http://html.scirp.org/file/13-1720246x27.png"  xlink:type="simple"/></disp-formula><p>(5.1), (5.2), (5.3), (5.4)</p><p>(5.1) Neutrality―the condition of the real part of SE roots being equal to zero;</p><p>(5.2) The separation of the spectral equation into two if the neutrality condition is fulfilled;</p><p>(5.3) The exclusion of frequency or one of the parameters from the equations and obtaining of a neutral surface―<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x28.png" xlink:type="simple"/></inline-formula>and the critical frequency―<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x29.png" xlink:type="simple"/></inline-formula>;</p><p>(5.4) Indication of stability and instability areas in relation to the neutral surface.</p><p>The NSE outline is fully realized for the polynomial SE. The general neutrality conditions (3.3) in this case are given by</p><disp-formula id="scirp.56756-formula781"><label>, (6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x30.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x31.png" xlink:type="simple"/></inline-formula>―the resultant, а NOD-GCD―the greatest common divisor of polynomials <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x32.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x32.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x33.png" xlink:type="simple"/></inline-formula>.</p><p>Specifically for a third order system the conditions (6) are</p><disp-formula id="scirp.56756-formula782"><graphic  xlink:href="http://html.scirp.org/file/13-1720246x34.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.56756-formula783"><label>. (7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x35.png"  xlink:type="simple"/></disp-formula><p>2) The<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x36.png" xlink:type="simple"/></inline-formula>―criterion method is expressed by the determinant of block <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x37.png" xlink:type="simple"/></inline-formula> matrix</p><disp-formula id="scirp.56756-formula784"><label>, (8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x38.png"  xlink:type="simple"/></disp-formula><p>which consists of the evolutionary matrix <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x39.png" xlink:type="simple"/></inline-formula> and its coefficients <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x40.png" xlink:type="simple"/></inline-formula> unity matrix,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x41.png" xlink:type="simple"/></inline-formula>―complex conjugate elements of the matrix<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x42.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x43.png" xlink:type="simple"/></inline-formula>―its eigenvalues.</p><p>The neutrality criterion and the equation for the critical frequencies in this method have the following form</p><disp-formula id="scirp.56756-formula785"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x44.png"  xlink:type="simple"/></disp-formula><p>The commutation of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x45.png" xlink:type="simple"/></inline-formula> matrix blocks allows operating them the same way as numbers and in particular reducing the order of its determinant. As a result, the<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x46.png" xlink:type="simple"/></inline-formula>―criterion comes down to the following form</p><disp-formula id="scirp.56756-formula786"><graphic  xlink:href="http://html.scirp.org/file/13-1720246x47.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x48.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x49.png" xlink:type="simple"/></inline-formula>―are the coefficients of the spectral equation.</p></sec><sec id="s3"><title>3. Nonlinear Systems</title><p>Assuming that Equation (1), which describe the system that is being analyzed in terms of stability, represent a combination of nonlinear autonomic equations</p><disp-formula id="scirp.56756-formula787"><label>. (10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x50.png"  xlink:type="simple"/></disp-formula><p>The perturbation dynamics of system (10) in this case are described by Equation (11)</p><disp-formula id="scirp.56756-formula788"><label>, (11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x51.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x52.png" xlink:type="simple"/></inline-formula>―are the elements of evolutionary matrix, which depend on dynamical variables <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x52.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x53.png" xlink:type="simple"/></inline-formula> and time―<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x52.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x54.png" xlink:type="simple"/></inline-formula>.</p><p>If all the time derivatives in (11) are negative, the perturbations attenuate and the system is Lyapunov stable. If there is at least one positive derivative, the solution curves scatter; the system is not stable. The correlation of derivative signs allows to determine the possibility of chaotic behavior and the formation of complex localized structures―strange attractors [<xref ref-type="bibr" rid="scirp.56756-ref3">3</xref>] (see <xref ref-type="fig" rid="fig1">Figure 1</xref> and <xref ref-type="fig" rid="fig2">Figure 2</xref>) in the phase space.</p><p>In these cases, the spectral equation method (4) and NSE method (5) for the stability analysis in their classical forms are not applicable.</p><p>Due to the fact that the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x55.png" xlink:type="simple"/></inline-formula>-criterion is directly expressed by the dynamical equation coefficients, it is possible to generalize it for the stability analysis of nonlinear systems by introducing generalized eigenvalues of the evolutionary matrix<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x55.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x56.png" xlink:type="simple"/></inline-formula>. At this, the former will be time functions, the sign of which is determined unequivocally by the sign of the time derivatives <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x55.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x57.png" xlink:type="simple"/></inline-formula> and which automatically become normal eigenvalues in case of stationary states. This way, the form and the meaning of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x55.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x57.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x58.png" xlink:type="simple"/></inline-formula>-criterion in regard to the generalized eigenvalues are reserved.</p><disp-formula id="scirp.56756-formula789"><label>. (12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x59.png"  xlink:type="simple"/></disp-formula><p>Specifically, the criterion (12) being equal to zero corresponds to the presence of zero-order derivatives (eigen- values), the criterion sign change-corresponds to a sign change of time derivatives in dynamical Equation (11). As a result, the multiplication factor analysis in (12) represents an analysis of evolutionary matrix eigenvalues spectrum for a nonlinear system and therefore, an analysis of time derivatives signs in Equation (11).</p><p>Such generalization can technically be conducted for the NSE (5) and spectral Equation (4) methods, but in that case<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x60.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x60.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x61.png" xlink:type="simple"/></inline-formula>are not the parameters of Laplace transform, which is not applicable in these circumstances, they are the generalized eigenvalues<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x60.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x62.png" xlink:type="simple"/></inline-formula>.</p><p>So now we will use the generalized NSE and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x63.png" xlink:type="simple"/></inline-formula>-criterion methods for a stability analysis of nonlinear Lorenz and R&#246;ssler model systems and we also will evaluate the possibilities of the suggested methods to determine the presence of dynamical chaos.</p></sec><sec id="s4"><title>4. Lorenz Model Problem [<xref ref-type="bibr" rid="scirp.56756-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.56756-ref3">3</xref>]</title><p>The Lorenz problem is of a particular interest because nonlinear equations of Lorenz model result from the dynamics equations of a whole range of physical systems: The convection inside a fluid layer heated from underneath, a single-mode laser, water-wheel and other. Besides that, it demonstrates the formation of chaotic dyna- mics (<xref ref-type="fig" rid="fig1">Figure 1</xref>).</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x64.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x65.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x66.png" xlink:type="simple"/></inline-formula></p><p>The Lorenz model equations have the following form</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Lorenz attractor for “classical” values of parameters σ = 10, b = 8/3, r = 28</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/13-1720246x67.png"/></fig><disp-formula id="scirp.56756-formula790"><label>, (13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x68.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x69.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x70.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x71.png" xlink:type="simple"/></inline-formula>―are the dynamical variables,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x72.png" xlink:type="simple"/></inline-formula>―are the parameters, where the controlling parameter, representing the intensity is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x73.png" xlink:type="simple"/></inline-formula>.</p><p>In the phase space of variables <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x74.png" xlink:type="simple"/></inline-formula> the system state can be represented by a velocities vector,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x75.png" xlink:type="simple"/></inline-formula>―the divergence of which characterizes the dissipativity of the system and can be one of the stability conditions.</p><disp-formula id="scirp.56756-formula791"><label>. (14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x76.png"  xlink:type="simple"/></disp-formula><p>If <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x77.png" xlink:type="simple"/></inline-formula> the phase volume decreases, the trajectories come closer to each other. If <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x77.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x78.png" xlink:type="simple"/></inline-formula> the phase volume increases, the trajectories scatter―the system looses stability. From Equation (13) we have</p><disp-formula id="scirp.56756-formula792"><graphic  xlink:href="http://html.scirp.org/file/13-1720246x79.png"  xlink:type="simple"/></disp-formula><p>i.e. the Lorenz system is dissipative.</p><p>The system (13) has two stationary solutions-stationary states<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x80.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x81.png" xlink:type="simple"/></inline-formula>,</p><disp-formula id="scirp.56756-formula793"><label>. (15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x82.png"  xlink:type="simple"/></disp-formula><p>The linearization of system (13) in relation to a solution<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x83.png" xlink:type="simple"/></inline-formula>, for which any, including stationary, solution can be chosen, produces a system of equations for perturbations (11), where the evolutionary matrix is</p><disp-formula id="scirp.56756-formula794"><label>. (16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x84.png"  xlink:type="simple"/></disp-formula><p>The spectral equation and its coefficients in a stationary case are <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x85.png" xlink:type="simple"/></inline-formula></p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x86.png" xlink:type="simple"/></inline-formula>;</p><disp-formula id="scirp.56756-formula795"><label>. (17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x87.png"  xlink:type="simple"/></disp-formula><p>(It should be noted that the dissipation condition coincides in absolute value with the first coefficient of the spectral equation and is equal to the sum of eigenvalues of the evolutionary matrix. It may be shown that there is a common result.)</p><p>The NSE method for SE (17) produces two critical-neutral modes</p><p>1)<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x88.png" xlink:type="simple"/></inline-formula>, (18)</p><p>2)<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x89.png" xlink:type="simple"/></inline-formula>. (19)</p><p>The mode (18) occurs for the first stationary state and corresponds to its instability when<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x90.png" xlink:type="simple"/></inline-formula>, the eigenvalues in this case are</p><disp-formula id="scirp.56756-formula796"><label>. (20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x91.png"  xlink:type="simple"/></disp-formula><p>The mode (19) occurs for the second stationary state and for the classical values of Lorenz parameters the critical values of frequency and the parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x92.png" xlink:type="simple"/></inline-formula> are</p><disp-formula id="scirp.56756-formula797"><label>. (21)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x93.png"  xlink:type="simple"/></disp-formula><p>When <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x94.png" xlink:type="simple"/></inline-formula> the second stationary state becomes unstable, in this case <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x94.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x95.png" xlink:type="simple"/></inline-formula> the real part of the second and third eigenvalues becomes positive, i.e. slow-growing oscillations appear. For example, when</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x96.png" xlink:type="simple"/></inline-formula>,.</p><p>The <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x98.png" xlink:type="simple"/></inline-formula>-criterion for states (15) correspondingly produces expressions</p><disp-formula id="scirp.56756-formula798"><label>, (22)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x99.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.56756-formula799"><label>. (23)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x100.png"  xlink:type="simple"/></disp-formula><p>As could be expected, the criterion (22) shows an instability of the first stationary state (15) when<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x101.png" xlink:type="simple"/></inline-formula>. From (23) it follows that the instability of the second stationary state (existing when<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x102.png" xlink:type="simple"/></inline-formula>) occurs when <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x103.png" xlink:type="simple"/></inline-formula> and that it complies with the NSE criterion and the spectrum. In the criterion (23) there are three multiplier factors changing their sign, which corresponds to the signs of three time derivatives in the initial equations of the system (13). When <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x103.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x104.png" xlink:type="simple"/></inline-formula> the first multiplier factor is positive, the second one equals to zero, the third one is negative. Therefore, the combination of derivative signs corresponds to the occurrence condition for chaotic dynamics in the system, see [<xref ref-type="bibr" rid="scirp.56756-ref3">3</xref>] . Specifically, if the eigenvalues signs <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x103.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x104.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x105.png" xlink:type="simple"/></inline-formula> are</p><disp-formula id="scirp.56756-formula800"><label>, (24)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x106.png"  xlink:type="simple"/></disp-formula><p>The dynamical mode is correspondingly</p><p>1) A stable point;</p><p>2) A boundary cycle;</p><p>3) An attractor (of chaotic dynamics).</p><p>This way, in the Lorenz system with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x107.png" xlink:type="simple"/></inline-formula> up to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x107.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x108.png" xlink:type="simple"/></inline-formula> a chaotic mode with a phase portrait exists <xref ref-type="fig" rid="fig1">Figure 1</xref>. When <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x107.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x108.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x109.png" xlink:type="simple"/></inline-formula> the third derivative changes sign and the system fully looses stability entering the field of complex irregular dynamics.</p><p>It should be noted that the criterion (23) includes the first critical mode <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x110.png" xlink:type="simple"/></inline-formula> related to the instability of the first stationary state; also it can be shown that the critical frequency calculated according to formula (7) coincides with the value determined using the spectrum (21).</p></sec><sec id="s5"><title>5. R&#246;ssler Model Problem</title><p>A nonlinear problem which has an evidentially expressed field of chaotic behavior with an attractor presented in <xref ref-type="fig" rid="fig2">Figure 2</xref>, see [<xref ref-type="bibr" rid="scirp.56756-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.56756-ref3">3</xref>] .</p><p>The R&#246;ssler model equations have the following form</p><disp-formula id="scirp.56756-formula801"><label>. (25)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x111.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x112.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x112.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x113.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x112.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x113.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x114.png" xlink:type="simple"/></inline-formula>―are the dynamical variables;<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x112.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x113.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x114.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x115.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x112.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x113.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x114.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x115.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x116.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x112.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x113.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x114.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x115.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x116.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x117.png" xlink:type="simple"/></inline-formula>―the parameters,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x112.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x113.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x114.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x115.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x116.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x117.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x118.png" xlink:type="simple"/></inline-formula>―the controlling parameter. The diver- gence of velocities vector <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x112.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x113.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x114.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x115.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x116.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x117.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x118.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x119.png" xlink:type="simple"/></inline-formula> characterizing the system dissipativity is</p><disp-formula id="scirp.56756-formula802"><label>. (26)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x120.png"  xlink:type="simple"/></disp-formula><p>From (26) it follows that the R&#246;ssler system is dissipative only in a limited field (<xref ref-type="fig" rid="fig2">Figure 2</xref>).</p><p>The system (25) has two stationary solutions-stationary states <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x121.png" xlink:type="simple"/></inline-formula></p><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> R&#246;ssler attractor when<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x123.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x123.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x124.png" xlink:type="simple"/></inline-formula></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/13-1720246x122.png"/></fig><disp-formula id="scirp.56756-formula803"><label>, (27)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x125.png"  xlink:type="simple"/></disp-formula><p>which are possible under the condition<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x126.png" xlink:type="simple"/></inline-formula>. For R&#246;sslerparameters<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x126.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x127.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x126.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x127.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x128.png" xlink:type="simple"/></inline-formula>, the stationary solutions take the following form</p><disp-formula id="scirp.56756-formula804"><label>. (28)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x129.png"  xlink:type="simple"/></disp-formula><p>The linearization of Equation (25) in relation to the solution<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x130.png" xlink:type="simple"/></inline-formula>, for which any, including stationary, solution can be chosen, produces a system of equations for perturbations (11), where the evolutionary matrix is</p><disp-formula id="scirp.56756-formula805"><label>. (29)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x131.png"  xlink:type="simple"/></disp-formula><p>The spectral equation of the system (25) and its coefficients for the stationary states are correspondingly</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x132.png" xlink:type="simple"/></inline-formula>;</p><disp-formula id="scirp.56756-formula806"><label>. (30)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x133.png"  xlink:type="simple"/></disp-formula><p>The NSE criterion for SE (30) produces two critical-neutral modes (18, 19), which in this case take the following form</p><disp-formula id="scirp.56756-formula807"><label>. (31)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x134.png"  xlink:type="simple"/></disp-formula><p>The analysis of conditions (31) combined with stationary conditions (27) shows that when <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x135.png" xlink:type="simple"/></inline-formula> both conditions (31) coincide and the SE roots (30) are</p><disp-formula id="scirp.56756-formula808"><label>. (32)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x136.png"  xlink:type="simple"/></disp-formula><p>The first critical mode occurs only for the second stationary state<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x137.png" xlink:type="simple"/></inline-formula>, which, when <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x137.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x138.png" xlink:type="simple"/></inline-formula> becomes unstable, and the SE roots, for example, when <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x137.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x138.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x139.png" xlink:type="simple"/></inline-formula> are correspondingly</p><disp-formula id="scirp.56756-formula809"><label>. (33)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x140.png"  xlink:type="simple"/></disp-formula><p>The second critical mode occurs for the first stationary state, which is also unstable when<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x141.png" xlink:type="simple"/></inline-formula>. And when <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x141.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x142.png" xlink:type="simple"/></inline-formula> the SE roots are</p><disp-formula id="scirp.56756-formula810"><label>. (34)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x143.png"  xlink:type="simple"/></disp-formula><p>This way both stationary states are unstable in different ways.</p><p>The L-criterion (12) regarding arbitrary solutions <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x144.png" xlink:type="simple"/></inline-formula> after several developments takes the following form <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x144.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x145.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.56756-formula811"><label>. (35)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x146.png"  xlink:type="simple"/></disp-formula><p>For stationary solutions (27) the criterion (35) is rearranged into</p><disp-formula id="scirp.56756-formula812"><label>. (36)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/13-1720246x147.png"  xlink:type="simple"/></disp-formula><p>As one would expect, the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x148.png" xlink:type="simple"/></inline-formula>-criterion contains both critical modes acquired using the NSE method (31), at this, one of the multipliers in the criterion coincides with the dissipation condition. The <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x148.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x149.png" xlink:type="simple"/></inline-formula>-criterion unlike the NSE method, the same way it was in the Lorenz problem, contains an additional-third multiplier which corresponds to the sign of the third time derivative in the initial equations. From (36) it follows that, for the R&#246;ssler model, depending on the (r, e, d) parameters, the occurrence of all three modes is possible (see (31)). For example when <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x148.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x149.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x150.png" xlink:type="simple"/></inline-formula> the multipliers signs in (36) and correspondingly the signs of time derivatives in the initial system are</p><disp-formula id="scirp.56756-formula813"><graphic  xlink:href="http://html.scirp.org/file/13-1720246x151.png"  xlink:type="simple"/></disp-formula><p>which indicates a chaotic behavior of the system with a phase portrait of the type illustrated in <xref ref-type="fig" rid="fig2">Figure 2</xref>.</p></sec><sec id="s6"><title>6. Conclusion</title><p>In conclusion, the use of modified NSE methods and the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/13-1720246x152.png" xlink:type="simple"/></inline-formula>-criterion for the stability analysis of nonlinear systems allows not only acquiring the stability and instability conditions, but also predicting the possibility of chaotic dynamics in the former.</p></sec></body><back><ref-list><title>References</title><ref id="scirp.56756-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Landa, I.P. (1997) Nonlinear Waves and Oscillations. Nauka, Moscow, 496 p.</mixed-citation></ref><ref id="scirp.56756-ref2"><label>2</label><mixed-citation publication-type="journal" xlink:type="simple"><name name-style="western"><surname>Feigenbaum</surname><given-names> M. </given-names></name>,<etal>et al</etal>. 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