<?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.2015.36081</article-id><article-id pub-id-type="publisher-id">JAMP-57473</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>
 
 
  Improvement of Harmonic Balance Using Jacobian Elliptic Functions
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>erge</surname><given-names>Bruno Yamgoué</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>Bonaventure</surname><given-names>Nana</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>Olivier</surname><given-names>Tiokeng Lekeufack</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>Laboratory of Mechanics, Department of Physics, Faculty of Science, The University of Yaoundé 1, Yaoundé, Cameroon</addr-line></aff><aff id="aff1"><addr-line>Department of Physics, Higher Teacher Training College-Bambili, The University of Bamenda, Bamenda, Cameroon</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>sergebruno@yahoo.fr(EBY)</email>;<email>na1bo@yahoo.fr(BN)</email>;<email>lekeufackolivier@gmail.com(OTL)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>17</day><month>06</month><year>2015</year></pub-date><volume>03</volume><issue>06</issue><fpage>680</fpage><lpage>690</lpage><history><date date-type="received"><day>29</day>	<month>May</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>22</month>	<year>June</year>	</date><date date-type="accepted"><day>26</day>	<month>June</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>
 
 
  We propose a method for finding approximate analytic solutions to autonomous single degree-of-freedom nonlinear oscillator equations. It consists of the harmonic balance with linearization in which Jacobian elliptic functions are used instead of circular trigonometric functions. We show that a simple change of independent variable followed by a careful choice of the form of anharmonic solution enable to obtain highly accurate approximate solutions. In particular our examples show that the proposed method is as easy to use as existing harmonic balance based methods and yet provides substantially greater accuracy.
 
</p></abstract><kwd-group><kwd>Harmonic Balance</kwd><kwd> Linearization</kwd><kwd> Continuous Force Function</kwd><kwd> Single Degree-of-Freedom</kwd><kwd> Conservative System</kwd><kwd> Jacobian Elliptic Functions</kwd><kwd> Symmetric Oscillations</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Ordinary differential equations (ODEs in short) are ubiquitous in fundamental science as well as in engineering. Indeed they commonly arise as direct results of the application of some fundamental laws in the various fields of science or engineering. A classical example here is Newton’s second law of motion. They also often arise indirectly, for example, in the intermediate steps of solving other types of problems such as partial differential equations (PDEs). Solving ODEs, especially analytically, thus appears to be of great importance for gaining insights into real-world or engineering problems. This is yet a very challenging task since the ODEs of interest, being usually nonlinear, are rarely susceptible to exact analytical solutions. In fact, the lack of a general and systematic methodology for solving these nonlinear equations is probably the most important difficulty in the determination of their analytical solutions. So, for the important class of ODEs associated with oscillatory behaviors, numerous techniques which enable to obtain some approximations to the desired solutions have been developed. These techniques may be classified in two groups: perturbation and non-perturbation.</p><p>The most famous of perturbation approaches include the Lindstedt-Poincar&#233; (LP) method, the method of multiple scales (MMS) and the Krylov-Bogoliubov-Mitropolsky (KBM) method. These now classical methods are known to have some serious limitations. For instance they are useless for equations which describe essentially nonlinear oscillators, such as (1) below with<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x5.png" xlink:type="simple"/></inline-formula>.</p><p>In contrast, non-perturbation techniques of which the method of harmonic balance (HB) is a well-known example, do not suffer these limitations. But the straightforward application of this last method leads to systems of nonlinear algebraic equations for the coefficients of the truncated Fourier series assumed for the solutions; which are still very difficult to solve. However the acuteness of this difficulty can now be reduced considerably thanks to the idea proposed initially by Wu and Li [<xref ref-type="bibr" rid="scirp.57473-ref1">1</xref>] and further refined by Wu and co-workers [<xref ref-type="bibr" rid="scirp.57473-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.57473-ref3">3</xref>] . It consists of linearizing the governing equations before applying the HB itself, which then leads to linear algebraic equations instead of nonlinear ones. The resulting method, harmonic balance with linearization (HBwL), has been applied to various types of conservative symmetric oscillators and appears to be both quite efficient and very simple [<xref ref-type="bibr" rid="scirp.57473-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.57473-ref3">3</xref>] , and references therein. Considering these two interesting properties, the method of HBwL is a good candidate for improvements which can make it to be more versatile than just conservative or symmetric systems. In this respect it has been adapted to handling dissipation terms in ODEs [<xref ref-type="bibr" rid="scirp.57473-ref4">4</xref>] , and more recently to solving asymmetric oscillator equations [<xref ref-type="bibr" rid="scirp.57473-ref5">5</xref>] .</p><p>Another important class of non-perturbative techniques involves the approximation of the nonlinear restoring force in a given oscillator ODE by some simple forms for which the exact solution can be readily obtained. The most common technique in this class is the method of equivalent linearization. In this approach the approximate ODE has the simple form of a linear harmonic oscillator equation [<xref ref-type="bibr" rid="scirp.57473-ref6">6</xref>] . Besides the method of equivalent linearization is the so-called method of “cubication” in which the restoring force function is expanded up to third order in Chebyshev polynomials. The method of cubiccation thus approximates a given ODE by a cubic Duffing equation whose exact solution is the approximate solution to the original ODE. It is well known that the exact solution of the Duffing equation can be expressed in explicit form using Jacobian elliptic functions [<xref ref-type="bibr" rid="scirp.57473-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.57473-ref8">8</xref>] .</p><p>In this paper, we investigate a further generalization of the HBwL by using Jacobian elliptic functions instead of circular trigonometric functions [<xref ref-type="bibr" rid="scirp.57473-ref7">7</xref>] . Our objective is to develop a higher order approximation than the single cnoidale elliptic function which is obtained when a given ODE is first approximated by a Duffing equation. We achieve this goal through a simple change of variable based on the properties of the Jacobian elliptic functions, which results to an ODE in which the restoring force is not approximated and which is solved approximately following the method of HBwL or other generalizations of the method of HB such as the rational HB.</p><p>The paper is organized as follows. The main idea sustaining the elliptic harmonic balance is introduced in the next section. The illustrations are presented next in Section 3, where examples of oscillators with polynomial and rational restoring force functions are considered. Section 4 contains the conclusion of the paper.</p></sec><sec id="s2"><title>2. Presentation of the Approach</title><p>We consider a nonlinear second-order differential equation of the general form</p><disp-formula id="scirp.57473-formula1784"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x6.png"  xlink:type="simple"/></disp-formula><p>which governs the time (t) evolution of the state of the state (x) of a conservative single degree-of-freedom system. Here, an overdot denotes differentiation with respect to time t. Thus, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x7.png" xlink:type="simple"/></inline-formula>is a real function. We assume without loss of generality that<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x8.png" xlink:type="simple"/></inline-formula>. The restoring force function f is a general nonlinear function of x which is required to be continuous and to satisfy <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x9.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x10.png" xlink:type="simple"/></inline-formula> for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x11.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x12.png" xlink:type="simple"/></inline-formula>; where x<sub>1</sub> and x<sub>2</sub> are two constants. For simplicity we shall restrict ourselves in this paper to the case where f is additionally odd,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x13.png" xlink:type="simple"/></inline-formula>; so that the system oscillates symmetrically around<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x14.png" xlink:type="simple"/></inline-formula>. Our objective is to determine an approximate analytic solution to the periodic solution of the above equation. It is customary in classical techniques [<xref ref-type="bibr" rid="scirp.57473-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.57473-ref9">9</xref>] - [<xref ref-type="bibr" rid="scirp.57473-ref12">12</xref>] to introduce a time scaling according to</p><disp-formula id="scirp.57473-formula1785"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x15.png"  xlink:type="simple"/></disp-formula><p>Here, T and w are the unknown time-period and angular frequency of the sought periodic solution. Under this scaling, (1) becomes</p><disp-formula id="scirp.57473-formula1786"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x16.png"  xlink:type="simple"/></disp-formula><p>where we have set<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x17.png" xlink:type="simple"/></inline-formula>, and a prime denotes a differentiation with respect to τ. The periodic solutions of this latter equation are 2π-periodic in τ.</p><p>In this paper we use a different time-scaling than (2) which is simply linear in τ. Following Yuste Bravo [<xref ref-type="bibr" rid="scirp.57473-ref7">7</xref>] , we consider the generally nonlinear transformation given by</p><disp-formula id="scirp.57473-formula1787"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x18.png"  xlink:type="simple"/></disp-formula><p>where am is the Jacobian elliptic amplitude function of parameter m while K is the complete elliptic integral of the first kind. In this paper we adopt the notation of [<xref ref-type="bibr" rid="scirp.57473-ref13">13</xref>] for designating elliptic functions. The parameter m is an additional unknown to be determined as part of the solution. It should be noted that (2) is a particular case of (4), corresponding to the fixed value m = 0. Using the following well-known property of the am function</p><disp-formula id="scirp.57473-formula1788"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x19.png"  xlink:type="simple"/></disp-formula><p>one can easily show that the nonlinear time-scaling (4) transforms (1) into</p><disp-formula id="scirp.57473-formula1789"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x20.png"  xlink:type="simple"/></disp-formula><p>Notice that (6) reduces to (3) for m = 0. The former differs from the latter only by two terms which are parametrically linear in the derivatives. Thus if the HB can be applied to the latter, which requires that one be able to compute the Fourier series of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x21.png" xlink:type="simple"/></inline-formula> for a given truncation of the 2π-periodic Fourier expansion of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x22.png" xlink:type="simple"/></inline-formula>, then it should equally be applicable to (6). Once the solution is obtained in terms of τ, its expression is transformed into a polynomial in <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x22.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x23.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x22.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x24.png" xlink:type="simple"/></inline-formula> using the expansions [<xref ref-type="bibr" rid="scirp.57473-ref14">14</xref>]</p><disp-formula id="scirp.57473-formula1790"><label>(7a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x25.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.57473-formula1791"><label>(7b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x26.png"  xlink:type="simple"/></disp-formula><p>Then, by making the substitutions <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x27.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x28.png" xlink:type="simple"/></inline-formula> one can express the approximate solution in terms of t. Here cn and sn are respectively the Jacobian elliptic cosine and the Jacobian elliptic sine functions [<xref ref-type="bibr" rid="scirp.57473-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.57473-ref14">14</xref>] . It is worth to mention that in basic introduction to Jacobian elliptic functions it is supposed that<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x29.png" xlink:type="simple"/></inline-formula>. However this assumption is not a real restriction for our investigation. In effect, as the approximate solutions considered here are ultimately expressed in terms of cn and sn, the following transformations ( [<xref ref-type="bibr" rid="scirp.57473-ref13">13</xref>] , p. 573)</p><disp-formula id="scirp.57473-formula1792"><label>(8a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x30.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.57473-formula1793"><label>(8b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x31.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.57473-formula1794"><label>(8c)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x32.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.57473-formula1795"><label>(9a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x33.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.57473-formula1796"><label>(9b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x34.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.57473-formula1797"><label>(9c)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x35.png"  xlink:type="simple"/></disp-formula><p>are applicable respectively for m &lt; 0 and m &gt; 1. Thus the results that would be obtained using the proposed approach are valid for all real values of such that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x36.png" xlink:type="simple"/></inline-formula> (for this valueof , the Jacobian elliptic functions become hyperbolic and nonperiodic). Moreover, the Jacobi’s imaginary transformation ( [<xref ref-type="bibr" rid="scirp.57473-ref13">13</xref>] , p. 574)</p><disp-formula id="scirp.57473-formula1798"><label>(10a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x37.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.57473-formula1799"><label>(10b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x38.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.57473-formula1800"><label>(10c)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x39.png"  xlink:type="simple"/></disp-formula><p>in which <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x40.png" xlink:type="simple"/></inline-formula> can be applied when the value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x41.png" xlink:type="simple"/></inline-formula> is negative; as long as the expression of the approximate analytical solution to the ODE involves only cosine terms. Note that in (8)-(10),<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x42.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s3"><title>3. Illustrations</title><p>Two examples are now presented for illustration.</p><sec id="s3_1"><title>3.1. The Cubic-Quintic Duffing Oscillator</title><p>Our first example involve the cubic-quintic Duffing oscillator described by (1) with f defined such that</p><disp-formula id="scirp.57473-formula1801"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x43.png"  xlink:type="simple"/></disp-formula><p>Since<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x44.png" xlink:type="simple"/></inline-formula>, the oscillations will be symmetric within the bounds<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x45.png" xlink:type="simple"/></inline-formula>. It is well known that the Fourier expansion of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x46.png" xlink:type="simple"/></inline-formula> contains only odd harmonics in this case [<xref ref-type="bibr" rid="scirp.57473-ref15">15</xref>] . The simplest truncation of this expansion which satisfies the prescribed initial conditions consists of the fundamental harmonic only,</p><disp-formula id="scirp.57473-formula1802"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x47.png"  xlink:type="simple"/></disp-formula><p>Substituting this in (6) with the above form of f and equating the coefficients of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x48.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x49.png" xlink:type="simple"/></inline-formula> to zero, we obtain</p><disp-formula id="scirp.57473-formula1803"><label>(13a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x50.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.57473-formula1804"><label>(13b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x51.png"  xlink:type="simple"/></disp-formula><p>The solution of this set of equations is found to be (recall that<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x52.png" xlink:type="simple"/></inline-formula>)</p><disp-formula id="scirp.57473-formula1805"><label>(14a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x53.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.57473-formula1806"><label>(14b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x54.png"  xlink:type="simple"/></disp-formula><p>The explicit solution associated with (12) is as in (18a) below. Some limiting cases can be verified readily: For<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x55.png" xlink:type="simple"/></inline-formula>, the solution becomes <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x55.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x56.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x55.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x57.png" xlink:type="simple"/></inline-formula> leading as expected to the solution of the linear harmonic oscillator (assuming<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x55.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x57.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x58.png" xlink:type="simple"/></inline-formula>). Similarly, for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x55.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x57.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x58.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x59.png" xlink:type="simple"/></inline-formula> but<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x55.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x57.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x58.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x59.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x60.png" xlink:type="simple"/></inline-formula>, (1) with (11) reduces to the cubic Duffing oscillator; and the expressions of w and m above with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x55.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x57.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x58.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x59.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x60.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x61.png" xlink:type="simple"/></inline-formula> yield the exact solution [<xref ref-type="bibr" rid="scirp.57473-ref16">16</xref>] .</p><p>The results obtained at this level are exactly the same that would be obtained by cubication [<xref ref-type="bibr" rid="scirp.57473-ref16">16</xref>] . In effect, the third order Chebyshev expansion of (11) in the range of interest, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x62.png" xlink:type="simple"/></inline-formula>, is given by</p><disp-formula id="scirp.57473-formula1807"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x63.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x64.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x65.png" xlink:type="simple"/></inline-formula> are the Chebyshev polynomials of degrees 1 and 3 respectively:</p><disp-formula id="scirp.57473-formula1808"><label>(16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x66.png"  xlink:type="simple"/></disp-formula><p>The method of cubication therefore approximates (1) with (11) by</p><disp-formula id="scirp.57473-formula1809"><label>(17a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x67.png"  xlink:type="simple"/></disp-formula><p>with</p><disp-formula id="scirp.57473-formula1810"><label>(17b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x68.png"  xlink:type="simple"/></disp-formula><p>The solution of (17a) can be written explicitly as [<xref ref-type="bibr" rid="scirp.57473-ref16">16</xref>]</p><disp-formula id="scirp.57473-formula1811"><label>(18a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x69.png"  xlink:type="simple"/></disp-formula><p>with</p><disp-formula id="scirp.57473-formula1812"><label>(18b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x70.png"  xlink:type="simple"/></disp-formula><p>One can easily verify that for μ and λ defined by (17b) the expressions of and in (18b) and (14) are the same. This shows that the method of cubication and the lowest order harmonic balance in our proposed approach are equivalent. But unlike the method of cubication whose results would be limited to the above, the transformation proposed herein allows for further improvments. For instance, the approximate solution to (6) can be sought directly in the form</p><disp-formula id="scirp.57473-formula1813"><label>(19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x71.png"  xlink:type="simple"/></disp-formula><p>The required Fourier series expansion is quite easily calculated for polynomial restoring force functions. By equating the coefficients of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x72.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x73.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x74.png" xlink:type="simple"/></inline-formula> of this Fourier series to zero, one then establishes the equations for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x75.png" xlink:type="simple"/></inline-formula>. These may always be reduced to a single polynomial equation in d which can be solved approximately under the assumption that<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x75.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x76.png" xlink:type="simple"/></inline-formula>. In particular for the cubic-quintic Duffing oscillator (11), by letting</p><disp-formula id="scirp.57473-formula1814"><label>(20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x77.png"  xlink:type="simple"/></disp-formula><p>we can express w and m as follows</p><disp-formula id="scirp.57473-formula1815"><label>(21a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x78.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.57473-formula1816"><label>(21b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x79.png"  xlink:type="simple"/></disp-formula><p>where d solves the polynomial equation</p><disp-formula id="scirp.57473-formula1817"><label>(22a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x80.png"  xlink:type="simple"/></disp-formula><p>The coefficients of the above polynomial equations are as follows:</p><disp-formula id="scirp.57473-formula1818"><label>(22b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x81.png"  xlink:type="simple"/></disp-formula><p>Since<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x82.png" xlink:type="simple"/></inline-formula>, we may neglect higher powers of d in (22). Thus the solution is obtained approximately as</p><disp-formula id="scirp.57473-formula1819"><label>(23)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x83.png"  xlink:type="simple"/></disp-formula><p>Using (7a) for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x84.png" xlink:type="simple"/></inline-formula> and the substitution<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x84.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x85.png" xlink:type="simple"/></inline-formula>, one obtains the explicit form of (19) as</p><disp-formula id="scirp.57473-formula1820"><label>(24)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x86.png"  xlink:type="simple"/></disp-formula><p>It appears obviously from (23) that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x87.png" xlink:type="simple"/></inline-formula> for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x87.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x88.png" xlink:type="simple"/></inline-formula> as expected. Then from (20), <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x87.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x88.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x89.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x87.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x88.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x90.png" xlink:type="simple"/></inline-formula>so that (21) reduce as expected to the exact expressions for the cubic Duffing oscillator. The limiting case <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x87.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x88.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x90.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x91.png" xlink:type="simple"/></inline-formula> can also be deduced from those expressions.</p><p>It deserves to point out here that one could have considered the improved solution in the form</p><disp-formula id="scirp.57473-formula1821"><label>(25)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x92.png"  xlink:type="simple"/></disp-formula><p>as was suggested by Yuste Bravo [<xref ref-type="bibr" rid="scirp.57473-ref7">7</xref>] . The expression of b following the linearization procedure is found in this case to be</p><disp-formula id="scirp.57473-formula1822"><label>(26)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x93.png"  xlink:type="simple"/></disp-formula><p>As can be seen, this expression is independent of the coefficient of the linear term α in contrast to (23). The consequence of this is that (25) is less versatile than (19) to accurately approximate the solutions of the Duffing oscillator for all combinations of the coefficients of its terms. In effect, we have noticed that (25) is very poor when <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x94.png" xlink:type="simple"/></inline-formula> as can be observed in <xref ref-type="fig" rid="fig1">Figure 1</xref>. Even worse, it becomes completely divergent for some combinations of parameters values and oscillation amplitude A. This behavior can be understood by observing that the Fourier series of the residual of (6) with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x94.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x95.png" xlink:type="simple"/></inline-formula> and Ω and m given by (14) does not contain the third harmonic. We may conclude that in the HBwL in general, the harmonics to include in the correction to a given stage should be higher than or equal to the least harmonic of the residual terms of that stage. Thus in the remaining part of this work, we consider only the most versatile expression (19) in our discussion.</p><p>To further appreciate the accuracy of the various approximations obtained above, we use the relative error</p><disp-formula id="scirp.57473-formula1823"><label>(27)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x96.png"  xlink:type="simple"/></disp-formula><p>to compare the approximate period</p><disp-formula id="scirp.57473-formula1824"><label>(28)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x97.png"  xlink:type="simple"/></disp-formula><p>to the exact period</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Comaprison of the approximate solutions to the exact solution for the cubic- quintic Duffing oscillator for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x99.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x100.png" xlink:type="simple"/></inline-formula>. Solid black line is from exact numerical solution while magenta dashed-line, red solid line and blue solid line correspond respectively to (12), (25) and (19)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-1720314x98.png"/></fig><disp-formula id="scirp.57473-formula1825"><label>(29)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x101.png"  xlink:type="simple"/></disp-formula><p>Consider first the case <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x102.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x103.png" xlink:type="simple"/></inline-formula>. The exact period can be expressed analytically in terms of the beta function B as</p><disp-formula id="scirp.57473-formula1826"><label>(30)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x104.png"  xlink:type="simple"/></disp-formula><p>Calculations using the approximate expressions derived above show that the relative errors of the first-order and second-order analytical approximations as compared to the exact solution are respectively less than 0.37% and 0.072%. In comparison it would be necessary to proceed up to the third-order approximation of the standard HBwL to obtain a result just better than our least accurate first-order result; with a relative error of 0.23% [<xref ref-type="bibr" rid="scirp.57473-ref17">17</xref>] .</p><p>In <xref ref-type="fig" rid="fig2">Figure 2</xref> we compare the relative errors of the single harmonic approximation or cubication, the standard HBwL, and the anharmonic solution when<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x105.png" xlink:type="simple"/></inline-formula>. All the three approximations are highly accurate for small values but yet of order O(1) of A. For larger values of the amplitude, the second order approximation of our present approach appears to yield the smallest relative error of 0.072% for the whole range of allowed oscillation amplitudes for the parameter values chosen. This last observation concerning large is the same for all combination of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x105.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x106.png" xlink:type="simple"/></inline-formula> with<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x105.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x106.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x107.png" xlink:type="simple"/></inline-formula>.</p><p>A further comparison is presented in <xref ref-type="fig" rid="fig3">Figure 3</xref> for situations where heteroclinic orbits connecting two distinct equilibrium points exist. Once again we observe that our approach generally provides the best accurate approximation. We should point out however that as the oscillation amplitude approaches critically the value for which heteroclinic trajectory is realized, the accuracy of the standard HBwL supersedes our result.</p></sec><sec id="s3_2"><title>3.2. An Oscillator with Rational Restoring Force</title><p>As a second example, we consider a conservative nonlinear oscillatory system in which the restoring force has a rational form. Specifically we choose</p><disp-formula id="scirp.57473-formula1827"><label>(31)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x108.png"  xlink:type="simple"/></disp-formula><p>A peculiarity of this function which is worth noting is that it is not dominated by odd-power monomials in both of the limiting cases <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x109.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x109.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x110.png" xlink:type="simple"/></inline-formula> in contrast to the cubic-quintic Duffing oscillator or other rational restroring force oscillators such as the Duffing-harmonic oscillator [<xref ref-type="bibr" rid="scirp.57473-ref16">16</xref>] . In effect while <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x109.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x110.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x111.png" xlink:type="simple"/></inline-formula> for small amplitude oscillations, on has <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x109.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x110.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x111.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x112.png" xlink:type="simple"/></inline-formula> for large amplitude oscillations.</p><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Comparison of the relative errors for the cubic-quintic Duffing oscillator for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x114.png" xlink:type="simple"/></inline-formula>. Green dash-dotted line, magenta dashed-line, and solid blue correspond respectively to third order standard HBwL and (12) and (19) of the present work</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-1720314x113.png"/></fig><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Comparison of the relative errors for the cubic-quintic Duffing oscillator for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x116.png" xlink:type="simple"/></inline-formula> and for amplitude close to the critical value for heteroclinic motion. Green dash-dotted line and solid blue correspond respectively to third order standard HBwL and second order of the present work</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-1720314x115.png"/></fig><p>For this form of the restoring force function the expressions of μ and λ in the cubic Duffing equation (17a) approximating (1) with (31) are given by</p><disp-formula id="scirp.57473-formula1828"><label>(32a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x117.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.57473-formula1829"><label>(32b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x118.png"  xlink:type="simple"/></disp-formula><p>It follows that the expressions of the parameters m and w of the approximate solution of the problem using the method of cubication are</p><disp-formula id="scirp.57473-formula1830"><label>(33)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x119.png"  xlink:type="simple"/></disp-formula><p>Again these expressions can also be obtained through the lowest order harmonic balance method for (6) with (31). They solve exactly the coefficients of the fundamental and third order harmonics in the residual of this equation when<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x120.png" xlink:type="simple"/></inline-formula>. Consequently, the higher order approximation to the solution is taken once again as in (19). It is obvious here that the determination of the Fourier expansion of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x120.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x121.png" xlink:type="simple"/></inline-formula> is untractable. One can first envisage to expand <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x120.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x121.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x122.png" xlink:type="simple"/></inline-formula> in power series of d prior to the computation of the Fourier coefficients. However, upon substituting (19) in (6) with (31), it is simple to reduce it to the same denominator and consider only its numerator. Then by considering the coefficients of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x120.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x121.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x122.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x123.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x120.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x121.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x122.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x123.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x124.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x120.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x121.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x122.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x123.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x124.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x125.png" xlink:type="simple"/></inline-formula> we find after some algebraic manipulations that</p><disp-formula id="scirp.57473-formula1831"><label>(34a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x126.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.57473-formula1832"><label>(34b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x127.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.57473-formula1833"><label>(34c)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x128.png"  xlink:type="simple"/></disp-formula><p>with</p><disp-formula id="scirp.57473-formula1834"><label>(34d)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x129.png"  xlink:type="simple"/></disp-formula><p>To appreciate the accuracy of the two approximate results in (33) and (34) we have plotted in <xref ref-type="fig" rid="fig4">Figure 4</xref> the corresponding period calculated as <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x130.png" xlink:type="simple"/></inline-formula> and the exact period</p><disp-formula id="scirp.57473-formula1835"><label>(35)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720314x131.png"  xlink:type="simple"/></disp-formula><p>as a function of A. It appears clearly from this figure that the result obtained from the method of cubication so diverges from the exact result for large oscillation amplitudes that it can simply be considered invalid. However a good match is observed between the result of our proposed approach and the exact result. <xref ref-type="fig" rid="fig5">Figure 5</xref> indicates that the maximum relative error on the period is achieved for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720314x132.png" xlink:type="simple"/></inline-formula> and is less than 1.6%.</p></sec></sec><sec id="s4"><title>4. Conclusion and Remarks</title><p>In this paper we have investigated the approximation of periodic solutions to autonomous single degree-of- freedom oscillators equations using the Jacobian elliptic function with the objective of improving the method of cubication. To this end we have shown that the properties of these functions can be exploited to put such ODEs</p><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Comparison of harmonic (magenta triangle), anharmonic (blue circle) and numerical (black star) period for the rational restoring force oscillator</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-1720314x133.png"/></fig><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> Relative percentage error on the period for the rational restoring force oscillator</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-1720314x134.png"/></fig><p>in a form for which the standard HB and like methods can be applied, while the result is however expressed in terms of Jacobian elliptic functions. Our investigation reveals that in the HBwL the harmonics to include in the correction to a given stage should be higher than or equal to the least harmonic of the residual terms of that stage. With the change of variable sustaining our approach, the analysis can be carried out to higher order, just as in the standard HBwL. For our examples, comparison to the standard harmonic balance indicates that our approach is generally the best, except for periodic orbits too close to a heteroclinic orbit. However, even in this case, the standard HBwL has to be carried to higher order than our approach to gain this advantage. Such a higher order analysis can be quite intricate for non polynomial restoring force. A further interesting property of the solution resulting from our approach is that it also approximates all the harmonics of the exact solution. While the method of rational harmonic balance and the method of cubication also offer solutions with this property, they do not include a mean to carrying the approximations to higher orders as in the present work. In fact our method encompasses the method of cubication which is equivalent to ist first order application.</p></sec><sec id="s5"><title>Cite this paper</title><p>Serge Bruno Yamgou&#233;,Bonaventure Nana,Olivier Tiokeng Lekeufack, (2015) Improvement of Harmonic Balance Using Jacobian Elliptic Functions. Journal of Applied Mathematics and Physics,03,680-690. doi: 10.4236/jamp.2015.36081</p></sec></body><back><ref-list><title>References</title><ref id="scirp.57473-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Wu, B.S. and Li, P.S. (2001) A Method for Obtaining Approximate Analytical Periods for a Class of Nonlinear Oscillators. 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