<?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">ENG</journal-id><journal-title-group><journal-title>Engineering</journal-title></journal-title-group><issn pub-type="epub">1947-3931</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/eng.2013.55A009</article-id><article-id pub-id-type="publisher-id">ENG-31864</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Engineering</subject></subj-group></article-categories><title-group><article-title>
 
 
  Higher-Order WHEP Solutions of Quadratic Nonlinear Stochastic Oscillatory Equation
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>ohamed</surname><given-names>A. El-Beltagy</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>Amnah</surname><given-names>S. Al-Johani</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="aff1"><addr-line>Department of Engineering Mathematics &amp;amp; Physics, Engineering Faculty, Cairo University, Giza, Egypt</addr-line></aff><aff id="aff2"><addr-line>Department of Applied Mathematics, College of Science, Northern Borders University, Arar, KSA；College of Home Economics, Northern Borders University, Arar, KSA</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>zbeltagy@eng.cu.edu.eg(OAE)</email>;<email>xxwhitelinnetxx@hotmail.com(ASA)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>24</day><month>05</month><year>2013</year></pub-date><volume>05</volume><issue>05</issue><fpage>57</fpage><lpage>69</lpage><history><date date-type="received"><day>February</day>	<month>25,</month>	<year>2013</year></date><date date-type="rev-recd"><day>March</day>	<month>28,</month>	<year>2013</year>	</date><date date-type="accepted"><day>April</day>	<month>7,</month>	<year>2013</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>
 
 
  This paper introduces higher-order solutions of the quadratic nonlinear stochastic oscillatory equation. Solutions with different orders and different number of corrections are obtained with the WHEP technique which uses the Wiener
  Hermite expansion and perturbation technique. The equivalent deterministic equations are derived for each order and correction. The solution ensemble average and variance are estimated and compared for different orders, different number of corrections and different strengths of the nonlinearity. The solutions are simulated using symbolic computa
  tion software such as Mathematica. The comparisons between different orders and different number of corrections show the importance of higher-order and higher corrected WHEP solutions for the nonlinear stochastic differential equations.
  
 
</p></abstract><kwd-group><kwd>Oscillatory Equation; Nonlinear Differential Equations; Stochastic Differential Equation; Wiener-Hermite Expansion; Perturbation Technique</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Analysis of the response of linear and nonlinear systems subjected to random excitations is of considerable interest to the fields of mechanical and structural engineering [<xref ref-type="bibr" rid="scirp.31864-ref1">1</xref>]. Stochastic differential equations based on the white noise process provide a powerful tool for dynamically modeling complex and uncertain aspects. In many practical situations, it is appropriate to assume that the nonlinear term affecting the phenomena under study is small enough; then its intensity is controlled by means of a frank small parameter, say <img src="9-8101925\e7fb7f36-f36f-45af-ba94-4fb407f3ffd5.jpg" /> [<xref ref-type="bibr" rid="scirp.31864-ref2">2</xref>].</p><p>According to [<xref ref-type="bibr" rid="scirp.31864-ref3">3</xref>], the solution of stochastic partial differential equations (SPDEs) using Wiener-Hermite expansion (WHE) has the advantage of converting the problem to a system of deterministic equations that can be solved efficiently using the standard deterministic numerical methods. The main statistics, such as the mean, covariance, and higher order statistical moments, can be calculated by simple formulae involving only the deterministic Wiener-Hermite coefficients. In WHE approach, there is no randomness directly involved in the computations. One does not have to rely on pseudo random number generators, and there is no need to solve the stochastic PDEs repeatedly for many realizations. Instead, the deterministic system is solved only once.</p><p>The application of the WHE [4-10] aims at finding a truncated series solution to the solution process of a stochastic differential equation. The truncated series composes of two major parts; the first is the Gaussian part which consists of the first two terms, while the rest of the series constitute the non-Gaussian part. In non-linear cases, there exists always difficulties of solving the resultant set of deterministic integro-differential equations got from the applications of a set of comprehensive averages on the stochastic integro-differential equation obtained after the direct application of WHE. Many authors introduced different methods to face these obstacles. Among them, the WHEP technique [<xref ref-type="bibr" rid="scirp.31864-ref4">4</xref>] was introduced using the perturbation technique to solve perturbed nonlinear problems.</p><p>The WHE was originally started and developed by Norbert Wiener in 1938 and 1958 [<xref ref-type="bibr" rid="scirp.31864-ref11">11</xref>]. Wiener constructed an orthonormal random bases for expanding homogeneous chaos depending on white noise, and used it to study problems in statistical mechanics. Cameron and Martin [<xref ref-type="bibr" rid="scirp.31864-ref12">12</xref>] developed a more explicit and intuitive formulation for Wiener-Hermite expansion (now it is known as Wiener Chaos Expansion, WCE). Their development is based on an explicit discretization of the white noise process through its Fourier expansion, which was missed in Wiener’s original formalism. This approach is much easier to understand and more convenient to use, and hence replaced Wiener’s original formulation. Since Cameron and Martin’s work, WHE has become a useful tool in stochastic analysis involving white noise (Brownian motion) [<xref ref-type="bibr" rid="scirp.31864-ref3">3</xref>]. Also, another formulation was suggested and applied by Meecham and his co-workers [13, 14]. They have developed a theory of turbulence involving a truncated WHE of the velocity field. The randomness is taken up by a white-noise function associated, in the original version of the theory, with the initial state of the flow. The mechanical problem then reduces to a set of coupled integro-differential equations for deterministic kernels. In [<xref ref-type="bibr" rid="scirp.31864-ref1">1</xref>], the WHE (Imamura formulation, [<xref ref-type="bibr" rid="scirp.31864-ref13">13</xref>]) was used to compute the nonstationary random vibration of a Duffing oscillator which has cubic nonlinearity under white-noise excitation. Solutions up to second order are obtained by solving the equivalent deterministic system by an iterative scheme. M. El-Tawil and his coworkers [4-10] used the WHE together with the perturbation theory (WHEP technique) to solve a perturbed nonlinear stochastic diffusion equation.</p><p>As in [<xref ref-type="bibr" rid="scirp.31864-ref15">15</xref>], the analysis of nonlinear random vibration has been studied using several methods, such as, equivalent linearization method [<xref ref-type="bibr" rid="scirp.31864-ref16">16</xref>], stochastic averaging method [<xref ref-type="bibr" rid="scirp.31864-ref17">17</xref>], the WHE approach with nonstationary excitations [<xref ref-type="bibr" rid="scirp.31864-ref1">1</xref>], the WHE method combining with the small perturbation technique [<xref ref-type="bibr" rid="scirp.31864-ref18">18</xref>], eigenfunction expansions [<xref ref-type="bibr" rid="scirp.31864-ref19">19</xref>], and the method of detailed balance [<xref ref-type="bibr" rid="scirp.31864-ref20">20</xref>]. All the above methods are applied and used for nonlinear random oscillations of real systems subjected to random nonstationary (or stationary) excitations.</p><p>As in [5,6], quadrate oscillation arises through many applied models in applied sciences and engineering when studying oscillatory systems [<xref ref-type="bibr" rid="scirp.31864-ref21">21</xref>]. These systems can be exposed to a lot of uncertainties through the external forces, the damping coefficient, the frequency and/or the initial or boundary conditions. These input uncertainties cause the output solution process to be also uncertain. For most of the cases, getting the probability density function (p.d.f.) of the solution process may be impossible. So, developing approximate techniques (through which approximate statistical moments can be obtained) is an important and necessary work. There are many techniques which can be used to obtain statistical moments of such problems. The main goal of this paper is to compare some of these methods when applied to a quadrate nonlinearity problem.</p><p>In [<xref ref-type="bibr" rid="scirp.31864-ref22">22</xref>], the WHEP technique is generalized to n<sup>th</sup> nonlinearity, general order of WHE and general number of corrections. Also, the extension to handle white noise in more than one variable and general nonlinearities are outlined. The generalized algorithm is implemented and linked to MathML [<xref ref-type="bibr" rid="scirp.31864-ref23">23</xref>] script language to print out the resulting equivalent deterministic system.</p><p>In the current work the generalized WHEP technique developed in [<xref ref-type="bibr" rid="scirp.31864-ref22">22</xref>] is used to derive higher-order with higher corrections system of equations for the quadratic nonlinear stochastic oscillatory equation and then solve them. Up to fourth order equations are derived with different number of corrections. The mean and variance of the response will be simulated up to third order using Mathematica.</p><p>This paper is organized as follows. The formulation of the quadratic nonlinear stochastic oscillatory equation is outlined in Section 2. The WHEP technique is reviewed in Section 3. The equivalent deterministic system is derived in Section 4. In Section 5, the mean and variance of the solution is simulated with different order, different number of corrections and different values of the nonlinearity strengths.</p></sec><sec id="s2"><title>2. Problem Formulation</title><p>In this paper, the nonlinear oscillatory equation:</p><disp-formula id="scirp.31864-formula154633"><label>(1)</label><graphic position="anchor" xlink:href="9-8101925\c50181fb-c860-46d8-ba02-7b2abe4028ef.jpg"  xlink:type="simple"/></disp-formula><p>is considered under stochastic excitation and with the proper set of initial conditions <img src="9-8101925\ad1afc12-6c31-40f7-a742-cc58f184ac26.jpg" /> which is assumed to be deterministic. The operator L is a general linear operator and in the case of the oscillatory equation it will be:</p><p><img src="9-8101925\f0ddb50e-dcc2-4ed7-920f-91dcdde3718a.jpg" /></p><p>where <img src="9-8101925\63d6ec60-03eb-4a0e-ab39-1421cc40eac4.jpg" /> is the undamped angular frequency of the oscillator and <img src="9-8101925\15af5e7c-09c2-4b41-8c66-c8897e96ed2f.jpg" /> is the damping ratio. The nonlinearity is introduced as losses of degree <img src="9-8101925\f4eaa1c9-f52c-401c-9a7b-871374610fa4.jpg" /> strengthened by a deterministic small parameter<img src="9-8101925\c4f9c943-fd02-4ba8-a175-1ebc926de3ef.jpg" />. The uncertainty is introduced through white noise scaled by a deterministic envelope function<img src="9-8101925\fbf6a53d-d43f-4533-9f61-8923a7546729.jpg" />. The white noise is considered here as a function of time but it can be generalized in time and space as it was declared in [<xref ref-type="bibr" rid="scirp.31864-ref22">22</xref>]. The function <img src="9-8101925\7751f093-ecba-46ea-9eae-3d7f040a05b7.jpg" /> is a deterministic forcing function. Theorem (1) will be used in the derivation of the WHEP technique.</p><p>Theorem (1): The solution of Equation (1), if exists, is a power series in<img src="9-8101925\628c11ae-7d99-40b7-829f-192173289398.jpg" />, i.e.</p><disp-formula id="scirp.31864-formula154634"><label>(2)</label><graphic position="anchor" xlink:href="9-8101925\f7f0df27-bc52-4a6c-99d1-5db8de1d2eec.jpg"  xlink:type="simple"/></disp-formula><p>The theorem can be proved using the mathematical induction with the Pickard iterative technique [<xref ref-type="bibr" rid="scirp.31864-ref22">22</xref>]. As a direct result of this theorem, it is expected that the average, the variance as well as the covariance are also power series of<img src="9-8101925\232cae3d-4f7e-4462-8915-770922a79d0f.jpg" />.</p><p>The WHEP technique will be used in this work to determine the equivalent deterministic set of equations. The deterministic equations are then solved to obtain the solution kernels and hence the mean and variance of the response.</p></sec><sec id="s3"><title>3. WHEP Technique</title><p>As a consequence of the completeness of the WienerHermite set [<xref ref-type="bibr" rid="scirp.31864-ref13">13</xref>], any arbitrary stochastic process can be expanded in terms of the Weiner-Hermite polynomial set and this expansion converges to the original stochastic process with probability one.</p><p>The solution function <img src="9-8101925\15fb440e-96fd-4ac3-92ed-ef7c0eb0a20d.jpg" /> can be expanded in terms of Wiener-Hermite functionals as [<xref ref-type="bibr" rid="scirp.31864-ref4">4</xref>]:</p><p><img src="9-8101925\9a2f95a2-b4bf-4993-99e4-5c84d4cb5c00.jpg" /></p><p>Or after eliminating the parameters, for the sake of brevity, we get:</p><disp-formula id="scirp.31864-formula154635"><label>(3)</label><graphic position="anchor" xlink:href="9-8101925\ffa05c15-f5c9-4328-8f8f-a602f1b16429.jpg"  xlink:type="simple"/></disp-formula><p>where &#160;<img src="9-8101925\c458f3c5-95bd-4f18-ba71-2e17c96f2130.jpg" />&#160;and <img src="9-8101925\52000eeb-c565-4285-8e17-add577757206.jpg" />is a k-dimensional integral over the variables<img src="9-8101925\c8f44ca5-79fb-4b7b-b463-655f88ab23c7.jpg" />. The first term in the expansion (3) is the non-random part or ensemble mean of the function. The first two terms represent the normally distributed (Gaussian) part of the solution. Higher terms in the expansion depart more and more from the Gaussian form. The Gaussian approximation is usually a bad approximation for nonlinear problems, especially when high order statistics are concerned [<xref ref-type="bibr" rid="scirp.31864-ref3">3</xref>].</p><p>The components <img src="9-8101925\d44dcd8c-e1af-4757-ae14-1d88ab948acb.jpg" /> are called the (deterministic) kernels of the WHE for<img src="9-8101925\6cf95dc0-c50a-4e0a-bb44-8e1b2ba48f1e.jpg" />. The variable w is a random output of a triple probability space<img src="9-8101925\2143fe80-3f69-4c90-a520-6f32fa7c94f2.jpg" />, where <img src="9-8101925\ea559e93-ef07-4928-bd9c-49a6e66fb2fc.jpg" /> is a sample space, <img src="9-8101925\b01d278d-f65d-4b86-8fa6-87b758867524.jpg" />is a <img src="9-8101925\7831eadd-790b-43c5-bfb8-98d647bc2b3d.jpg" />- algebra associated with <img src="9-8101925\2c03654f-0bb3-47ed-92c9-a45524028643.jpg" /> and P is a probability measure. For simplicity, <img src="9-8101925\db1335ba-1fe7-4f6e-9cc6-cafa113b1291.jpg" />will be dropped later on.</p><p>The functional <img src="9-8101925\7c1b98b9-6c1c-4b88-81ea-8540b747e56f.jpg" /> is the <img src="9-8101925\ba4f7b90-f67f-4609-b2a0-1e8c29a6f44d.jpg" /> order Wiener-Hermite time-independent functional. The Wiener-H functionals form a complete set with <img src="9-8101925\07aef298-1cd0-43c4-b4cf-622887f5591a.jpg" /> and<img src="9-8101925\451b5507-17d1-48a3-954a-ecdc8a527fab.jpg" />: the white noise. By construction, the Wiener-Hermite functions are symmetric in their arguments and are statistically orthonormal, i.e.</p><p><img src="9-8101925\213a46c4-b529-4af3-bf3a-969d172d1eed.jpg" /></p><p>The average of almost all Wiener-Hermite functionals vanishes, particularly,</p><p><img src="9-8101925\f4c5fcf8-8c6b-479f-8307-7a4e52d56e09.jpg" /></p><p>The expectation and variance of the solution will be:</p><disp-formula id="scirp.31864-formula154636"><label>(4)</label><graphic position="anchor" xlink:href="9-8101925\651b16e7-87a0-40ee-9524-cd52922931d9.jpg"  xlink:type="simple"/></disp-formula><p>The WHE method can be elementary used in solving stochastic differential equations by expanding the solution as well as the stochastic input processes via the WHE. The resultant equation is more complex than the original one due to being a stochastic integro-differential equation [<xref ref-type="bibr" rid="scirp.31864-ref4">4</xref>]. Taking a set of ensemble averages together with using the statistical properties of the WHE functionals, a set of deterministic integro-differential equations are obtained in the deterministic kernels <img src="9-8101925\fcd4e927-fbcf-4ab8-8e3f-a8e5e6786212.jpg" /> To obtain approximate solutions of these deterministic kernels, one can use perturbation theory in the case of having a perturbed system depending on a small parameter<img src="9-8101925\d35ada72-df6f-48b5-9ea8-53b6632c33e0.jpg" />. Expanding the kernels as a power series of<img src="9-8101925\a176890d-9ad4-4059-be17-cabd2dc83491.jpg" />, another set of simpler iterative equations in the kernel series components are obtained. This is the main idea of the WHEP algorithm.</p><p>The WHEP technique for general nonlinear exponent<img src="9-8101925\f6c528e6-e406-4ca4-a4ac-97503c5df364.jpg" />, general order <img src="9-8101925\67fd190f-49eb-4591-b1ce-253c3f4aa579.jpg" /> and general number of corrections <img src="9-8101925\3007baac-da1c-4549-9234-cd61dc94bc22.jpg" /> follow the steps [<xref ref-type="bibr" rid="scirp.31864-ref22">22</xref>]:</p><p>1. Truncate the expansion (3) to contain only</p><p><img src="9-8101925\fae6d573-b9b5-48d7-9816-7876cfc77f36.jpg" />kernels<img src="9-8101925\583ffd9f-0921-4264-a61e-49756a0e495b.jpg" />, i.e.</p><p><img src="9-8101925\a9a7ac2d-0b05-452e-b137-e4e4280e588a.jpg" />and then 2. Substitute into the stochastic partial differential Equation (1);</p><p>3. Use the multinomial theorem to expand the nonlinear term <img src="9-8101925\a356eb16-36c8-42b7-8b58-ca8ab7373672.jpg" /> in (1);</p><p>4. Multiply by <img src="9-8101925\ebf35a27-0300-4317-aebf-ad7a415c0ed2.jpg" /> and then apply the ensemble average. This will lead to <img src="9-8101925\86b95424-e38d-4c6d-97b5-db25fa3db08d.jpg" /> equations in the kernels<img src="9-8101925\0414b809-4107-4141-9302-99fe826a0957.jpg" />;</p><p>5. For each kernel<img src="9-8101925\219b2830-8f3a-4d09-8582-a373e5bee3bc.jpg" />, apply the perturbation technique up to <img src="9-8101925\3da7359b-09a3-4f5b-a9b0-23bd1e32d1cf.jpg" /> corrections, i.e.</p><p><img src="9-8101925\aa3dd497-704f-4966-a907-e9d7aa928490.jpg" />;</p><p>6. Equating the coefficients of <img src="9-8101925\6501eb28-ca45-47c6-b4eb-8b589fbeeecf.jpg" /> in both sides to get <img src="9-8101925\843959c4-f26a-42a6-9ec9-7bd142a30a08.jpg" /> equations for each kernel <img src="9-8101925\084671ca-c682-433d-8cb7-a84463107d38.jpg" />.</p><p>This will lead to the following <img src="9-8101925\7beaee3e-3847-4e2c-ab72-3feb36557523.jpg" /> equations [<xref ref-type="bibr" rid="scirp.31864-ref22">22</xref>]:</p><disp-formula id="scirp.31864-formula154637"><label>(5)</label><graphic position="anchor" xlink:href="9-8101925\d221f5d9-fc45-4eb8-9c47-18ba9893806d.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.31864-formula154638"><label>(6)</label><graphic position="anchor" xlink:href="9-8101925\cc988f2e-c389-44c1-80e5-1ec23835673a.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.31864-formula154639"><label>(7)</label><graphic position="anchor" xlink:href="9-8101925\d7b7532b-e95d-4b14-ba62-1e85a5373892.jpg"  xlink:type="simple"/></disp-formula><p>And the expectations <img src="9-8101925\bd7289fc-6188-4693-b2bb-49a331e6495e.jpg" /> are computed as:</p><disp-formula id="scirp.31864-formula154640"><label>(8)</label><graphic position="anchor" xlink:href="9-8101925\c2bd9503-e7e8-454a-b8f8-a469981b3acc.jpg"  xlink:type="simple"/></disp-formula><p>It was explained in [<xref ref-type="bibr" rid="scirp.31864-ref22">22</xref>] how to get <img src="9-8101925\cbe68e33-ca26-4c73-8986-3a20e9bb3d48.jpg" /> in terms of the Dirac delta functions and then use them to reduce the integrals appear in<img src="9-8101925\ca39e055-2ccc-4b1b-9934-93c927a49958.jpg" />. The summation <img src="9-8101925\f595eae3-617c-43e9-b27d-16d37d42da10.jpg" />means that all variations <img src="9-8101925\a618ae34-7e91-4954-9acc-5a71103b59ed.jpg" /> that satisfy the equality <img src="9-8101925\4158d58a-3863-4d5e-98b4-bf52917f466f.jpg" /> are selected. This can be done be a searching technique. For these variations, the factors <img src="9-8101925\701fe097-36db-42c4-9fb7-aaf04fe8d8a6.jpg" /> will be multiplied by each other to get <img src="9-8101925\573cc63e-e903-404e-8f4d-026a4e6e19ff.jpg" /> i.e.<img src="9-8101925\e022c84e-a121-48c3-b7e8-cd5011c72126.jpg" />. The term <img src="9-8101925\2a9388fe-94d7-48f6-be0e-d6b4661f8460.jpg" /> is the Kronecker delta function that equals one when <img src="9-8101925\6065fb43-8678-40e2-aad3-1a81f55052f9.jpg" />and zero otherwise. Similarly, the term <img src="9-8101925\95c666ed-17fe-4347-ab5a-eac1293ed119.jpg" /> is the Kronecker delta function that equals one when <img src="9-8101925\84e4b43a-1d72-40bb-9c22-31489a20a160.jpg" />and zero otherwise. The counter<img src="9-8101925\b4f11ed0-0605-4b06-af8d-e497fbede776.jpg" />, in the summation in the right hand side of (6), runs over all the <img src="9-8101925\96721904-457a-48fd-a035-7e48843fb643.jpg" /> combinations of the positive integers <img src="9-8101925\4397ae1c-9268-4f00-b2ec-159d45dbf4fd.jpg" /> such that<img src="9-8101925\5fb763df-6069-45a7-aa2b-0d6f98433600.jpg" />.</p><p>Equations (5) and (6) can always be solved using the proper sequence. The first <img src="9-8101925\4fd72038-fcd5-40db-9833-7eb62214948d.jpg" /> Equations (5) are solved independently to get <img src="9-8101925\c3273f70-c508-4727-86c7-f1a742392425.jpg" /> then they are used to compute the other components in (6). For<img src="9-8101925\7b319fd3-202a-4e71-88d9-1279b82708d7.jpg" />, the component <img src="9-8101925\ea180992-b1a2-40c3-aca9-fb10f50d1efb.jpg" /> is obtained by solving</p><p><img src="9-8101925\35f0126c-0282-4a16-befe-be8fa5beced0.jpg" />with the original initial conditions which are assumed deterministic. For<img src="9-8101925\1d35c81b-074a-4d75-83a3-8f9b58a50d04.jpg" />, the component</p><p><img src="9-8101925\52cce18d-2efa-419d-a4d6-9fac5e5be709.jpg" />is obtained by solving <img src="9-8101925\8a569562-1c5b-4976-8ead-c9ab7b73fc9a.jpg" /> with zero initial conditions. The other components <img src="9-8101925\c5557f3a-a002-4cbb-a2bf-b210fc9ebf81.jpg" /> will be zeros due to zero right hand side and zero initial conditions. Equations (6) specify the solution sequence to be followed. The component <img src="9-8101925\7bd66c06-2791-49da-9780-96f91a4a37f7.jpg" /> is evaluated in terms of the previously computed components</p><p><img src="9-8101925\92b64c10-caf0-433d-8588-1cb5c2bf036e.jpg" />. This means that the 1<sup>st</sup> corrections for all kernels, <img src="9-8101925\6cb549a8-4837-4116-acea-bd7fb99cc2f2.jpg" />are solved firstly then solving the 2<sup>nd</sup> corrections for all kernels, <img src="9-8101925\48d9f069-efe4-4bd1-a129-b5068cf8e669.jpg" />,</p><p><img src="9-8101925\f91448c5-72d6-4ecd-b2ea-db8dce040de6.jpg" />up to the <img src="9-8101925\0f6a9047-dc7d-4671-b06c-c8b3a832a34c.jpg" /> corrections for all kernels</p><p><img src="9-8101925\f408e9e0-c6cc-4308-a7b3-9a799d5c8a86.jpg" />.</p><p>These results are consistent with the known results obtained using WHE. In WHE, higher order kernels are driven by lower order kernels, and at the bottom, the Gaussian kernels are driven by the random forcing directly. So, the lower order kernels are usually dominant in magnitude [<xref ref-type="bibr" rid="scirp.31864-ref3">3</xref>].</p><p>The statistical properties of the solution will now be calculated as:</p><disp-formula id="scirp.31864-formula154641"><label>(9)</label><graphic position="anchor" xlink:href="9-8101925\3b3c9fee-789d-4dbe-893e-40a86157d4b7.jpg"  xlink:type="simple"/></disp-formula><p>If<img src="9-8101925\dd7ba31e-4b9c-4340-af62-35f288d987dd.jpg" />, then it will be convergent if [<xref ref-type="bibr" rid="scirp.31864-ref22">22</xref>]:</p><p><img src="9-8101925\e8fb3f4a-6b88-45e0-ba81-461caf688333.jpg" /></p><p>for<img src="9-8101925\0e4efa8d-5113-4d0c-b5fb-e3ab45b532b2.jpg" />. This means that <img src="9-8101925\1fab302f-80f9-4a68-b407-eb8db0e09ead.jpg" /> should obey an upper bound condition after which divergence is obtained.</p><p>The formulation given in Equations (5) and (6) are quite general and could be used for analysis of the response of an any linear operator <img src="9-8101925\5407b372-7509-4f50-bd1a-a4034abea7cc.jpg" />with <img src="9-8101925\331c4442-f959-45b3-863f-0b6d66ee75c1.jpg" />degree nonlinearity and subjected to an arbitrary, stationary, or nonstationary Gaussian or non-Gaussian random excitation.</p><p>Consider the quadratic <img src="9-8101925\050f50c5-7146-4c0f-8156-e5db61552176.jpg" /> nonlinear oscillatory equation with excitation function:</p><disp-formula id="scirp.31864-formula154642"><label>(10)</label><graphic position="anchor" xlink:href="9-8101925\278183d2-403d-4a68-9e1e-ba886e612bf5.jpg"  xlink:type="simple"/></disp-formula><p>With the initial conditions</p><p><img src="9-8101925\19dd5f67-fae4-4627-8fcd-8d47cb956b41.jpg" /></p><p>In case of zero initial conditions, the exact solution can be obtained using different methods such as the theory of linear differential equations or the Laplace transform, and it will be the convolution:</p><disp-formula id="scirp.31864-formula154643"><label>(11)</label><graphic position="anchor" xlink:href="9-8101925\a2ea41fb-ab90-4b19-9907-a52530f6a0a2.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="9-8101925\ac18e572-ebd4-45ec-9a0b-fcdbcd67de86.jpg" /> with<img src="9-8101925\66d6bd2a-4816-4d23-b097-0dbe86d45808.jpg" />which is the angular frequency of the underdamped <img src="9-8101925\885d6c5f-1328-49fc-9179-6afabce055f6.jpg" /> harmonic oscillator.</p><p>For<img src="9-8101925\009149ad-9364-4d61-a1b4-1c68dcc3a787.jpg" />, the solution will results in:</p><p><img src="9-8101925\996bc8e8-9e6b-46e3-b2a9-32f5828fb4cb.jpg" /></p><p>The solution (11) of the model Equation (10) can be used as a model solution that is used in all kernels after considering the proper right hand side for the kernel equation.</p></sec><sec id="s4"><title>4. The Equivalent Deterministic System</title><p>Applying the above mentioned WHEP algorithm to get the following systems of equations of the quadratic (n = 2) nonlinear oscillatory equation and first order (m = 1) Gaussian approximation and different number of corrections<img src="9-8101925\b1035a08-cee0-4d11-8cca-406e8bd5acf6.jpg" />. The initial conditions are assumed deterministic and hence only the zero-order and zerocorrection kernel equation <img src="9-8101925\8d6ff870-8e9d-4c59-bed0-91f6eebd043e.jpg" /> will has the initial conditions<img src="9-8101925\6b1d768d-9cd6-4d11-be36-8411ac4d8563.jpg" />. Other kernels equations will have zero initial conditions.</p><p><img src="9-8101925\3b1a00aa-e7de-4551-9e2f-f4776b49abcf.jpg" />:</p><p><img src="9-8101925\92a404b8-8eff-445a-b132-2aefb2290a6f.jpg" /></p><p><img src="9-8101925\806a57c8-dde5-4e55-8218-828bb77713cc.jpg" />: The above equations in addition to:</p><p><img src="9-8101925\7bbcd0dd-1ae0-4f0a-98f5-85a3b5c49e84.jpg" /></p><p><img src="9-8101925\daf18562-5e4e-42ef-8220-1abb767ec0bd.jpg" />: The above equations in addition to:</p><p><img src="9-8101925\2b19bcb9-720a-40b6-9c05-364548c4f7c6.jpg" /></p><p><img src="9-8101925\6ebd077e-4bb1-4fc4-9f25-007a356fc8bb.jpg" />: The above equations in addition to:</p><p><img src="9-8101925\b213f24b-0948-48c8-8a96-c4c67f4b44b0.jpg" /></p><p><img src="9-8101925\a9b8012e-0bcf-4c5e-a6a9-589d8d1bdb0b.jpg" />: The above equations in addition to:</p><p><img src="9-8101925\f4399dfc-e201-46bd-8ac5-40aa895dc907.jpg" /></p><p>In case of zero initial conditions and zero deterministic excitation [i.e.<img src="9-8101925\5bdaca31-3159-4753-8c93-51a64c72f775.jpg" />], we shall have:</p><p><img src="9-8101925\58598101-bbc7-44ed-8019-773ebedb42a3.jpg" /></p><p>Which means the all of <img src="9-8101925\1eb7320f-e64f-4163-85b4-152cf8fd7ca3.jpg" /> and <img src="9-8101925\d87580b4-eb1b-4d7f-8fc8-12c2e2ab456a.jpg" /> are become zeros.</p><p>The second order <img src="9-8101925\e0d8ba3f-a59d-468f-aa4e-5df4b5d2f40d.jpg" /> equations will be:</p><p><img src="9-8101925\7df05404-fdfa-424d-9f7b-d0fdb5206877.jpg" />:</p><p><img src="9-8101925\837324a0-7927-4826-a00b-ee99f24e2009.jpg" /></p><p><img src="9-8101925\d7b5d050-0043-4946-9ab0-fa2565e30eb4.jpg" />: The above equations in addition to:</p><p><img src="9-8101925\1960b8b0-6418-4ded-a3a0-9c7c8557b73a.jpg" /></p><p><img src="9-8101925\d1933f09-7ba6-4a49-88b5-5cd88cf4a5f1.jpg" />: The above equations in addition to:</p><p><img src="9-8101925\4a97856f-55ae-458b-b2c9-8e6cf82741e8.jpg" /></p><p><img src="9-8101925\17469b49-74cc-4803-a61e-69bd9ca10749.jpg" />: The above equations in addition to:</p><p><img src="9-8101925\83f48913-872e-4adb-8174-2f44801f5158.jpg" /></p><p>The third order <img src="9-8101925\ab04ac75-eb5e-477a-a5ed-22e1e27856e1.jpg" /> equations are:</p><p><img src="9-8101925\5f39c0a0-2f65-4192-9e08-d550f89390ce.jpg" />:</p><p><img src="9-8101925\d348a244-2791-404d-bd3a-0ca21b3b892a.jpg" /></p><p><img src="9-8101925\f5507807-a13e-4bab-b81c-de9bef6d9bde.jpg" />: The above equations in addition to:</p><p><img src="9-8101925\6134f42a-a4e3-4984-a63a-80489c222d9b.jpg" /></p><p><img src="9-8101925\572ee8ca-6494-4502-8b1a-cc6a2ca68c53.jpg" />: The above equations in addition to:</p><p><img src="9-8101925\f929a743-9c8e-47c4-9a06-d0fb5d637af0.jpg" /></p><p><img src="9-8101925\0ce1e746-4156-43c6-bd5c-826eee913b04.jpg" />: The above equations in addition to:</p><p><img src="9-8101925\7d066507-1b7d-4cdc-ab78-b9a2d1aeb9b6.jpg" /></p><p><img src="9-8101925\eb9161ab-dcc1-4f9c-97ff-0234b9aeca19.jpg" /></p><p><img src="9-8101925\3d55eda2-8fc4-43d2-8513-6709d3b4f40a.jpg" /></p><p><img src="9-8101925\8c258a5c-aa72-4a31-bb71-c0cd0b563436.jpg" /></p><p>The fourth order <img src="9-8101925\c14e0b11-2f4e-4522-b3e8-823a6332fc75.jpg" /> equations are:</p><p><img src="9-8101925\b318fb5b-fa26-42bc-a9f9-be8114ec99b8.jpg" />:</p><p><img src="9-8101925\b0be9b5b-6182-4d79-aa8d-ce765234dc2f.jpg" /></p><p><img src="9-8101925\7cf244b6-95ff-4e30-8e69-13b23a2314c5.jpg" />: The above equations in addition to:</p><p><img src="9-8101925\0ef4793d-d501-40dc-acff-560220ea24bb.jpg" /></p></sec><sec id="s5"><title>5. Results</title><p>The following output is simulated using Mathematica. The solution (11) of the model Equation (10) is used to get all kernels with the proper right hand side. The mean response and the response variance are then calculated from the kernels using Equation (9):</p><p>Figures 1 and 2 show the response mean and variance, respectively, for the case of zero initial conditions, zero deterministic exciatation and unit envelope function multiplied by the white noise. The angular frequency <img src="9-8101925\7cfe0fd2-68e4-4f99-89d4-126591f123a4.jpg" /> and the damping ratio<img src="9-8101925\2fe366da-54c6-4e21-9e4a-44dc0cb1bffb.jpg" />. The nonlinearity strength is changed to study its effect on the response mean and variance. As it is shown in the figures, the nonlinearity strength greatly affect the amplitudes of the mean and variance. It should not be increased after a certain value to obtain convergent solution. This value depends on the different parameters of the problem.</p><p>Also, we can notice that higher correction solutions are required with longer time intervals.</p><p>In Figures 3 and 4, the envelope function <img src="9-8101925\933140bd-9e68-40ce-955c-cd447c08770f.jpg" /> is taken as<img src="9-8101925\9e5dc7d7-7999-45b1-9b50-154d95c7d65f.jpg" />. This will attenuate the effect of the white noise as the time increases. We can notice the attenuation effect on the response variance as the time increases. In this case, the variance vanishes with time and the solution becomes nearly deterministic.</p><p>In Figures 5 and 6, non-zero initial condition is considered; <img src="9-8101925\94c7d225-6d5b-49a2-bd40-58c2eddc10ae.jpg" />and<img src="9-8101925\600c023e-4f95-4f60-8b1f-fe5de718129a.jpg" />. The third correction mean and variance differs from the first and second corrections noticeably. This ensures the need for higher corrected WHEP solutions especially with larger values for the nonlinearity strength<img src="9-8101925\186de166-0d7a-4bac-82a4-30f1847d5183.jpg" />.</p><p>In Figures 7 and 8, the second order solution is simulated for different nonlinearity strengths with the first and second corrections. Higher corrected solutions will be time consuming even with multi-core machines. Mathematica automatically runs in parallel when multiple cores are available. The estimation of the response variance is more difficult than the response mean for higher corrections.</p><p>In Figures 9 and 10, the third order solution is simulated. Also, higher corrected solutions will be time con-</p><p>suming especially when estimating the response variance.</p><p>The fourth order first correction solution is also obtained but it is the same as the third and the second order with first corrections. Higher corrections will be more and more expensive. There is a need for an alternative method such as the numerical estimations to overcome the difficulties in using symbolic packages.</p></sec><sec id="s6"><title>6. Conclusion</title><p>In the present paper, we investigate the mean response of the quadratic nonlinear oscillatory system subjected to nonstationary random excitation using WHEP technique. The equivalent deterministic equations have been derived up to fourth order. The corrections are considered up to the fifth correction for lower orders and second corrections for higher orders. The mean and variance are simulated using Mathematica. It is observed that the WEHP technique can be applied to study the non-Gaussian response of any random systems. Moreover, the higherorder terms of the WHE should be adopted to obtain the responses of nonlinear random systems, and the integrodifferential equations for the kernels should be calculated. There is a need for numerical estimations when higher order and higher corrections are required.</p></sec><sec id="s7"><title>7. Acknowledgements</title><p>We should thank Prof. Magdy El-Tawil (has passed away) for motivating us to cooperate and do this work.</p></sec><sec id="s8"><title>REFERENCES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.31864-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">A. Jahedi and G. Ahmadi, “Application of Wiener-Hermite Expnasion to Nonstationary Random Vibration of a Duffing Oscillator,” Transactions of the ASME, Vol. 50, 1983, pp. 436-442.</mixed-citation></ref><ref id="scirp.31864-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">J. C. Cortes, J. V. Romero, M. D. Rosello and R. J. 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