<?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.2015.34054</article-id><article-id pub-id-type="publisher-id">JAMP-55822</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>
 
 
  Self-Consistent Sources and Conservation Laws for Super Tu Equation Hierarchy
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Sixing</surname><given-names>Tao</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>School of Mathematics and Information Science, Shangqiu Normal University, Shangqiu, China</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>taosixing@163.com</email></corresp></author-notes><pub-date pub-type="epub"><day>20</day><month>04</month><year>2015</year></pub-date><volume>03</volume><issue>04</issue><fpage>428</fpage><lpage>435</lpage><history><date date-type="received"><day>December</day>	<month>2014</month>	</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>
 
 
   Based upon the basis of Lie super algebra B(0,1), the super Tu equation hierarchy with self-con- sistent sources was presented. Furthermore, the infinite conservation laws of above hierarchy were given. 
 
</p></abstract><kwd-group><kwd>Super Tu Hierarchy</kwd><kwd> Self-Consistent Sources</kwd><kwd> Conservation Laws</kwd><kwd> Lie Super Algebra</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Soliton equations with self-consistent sources have been receiving growing attention in recent years. Physically, the sources may result in solitary waves with a non-constant velocity and therefore lead to a variety of dynamics of physical models. For applications, these kinds of systems can be used to describe interactions between different solitary waves. Ma and Strampp systematically applied explicit symmetry constraint and binary nonlinearization of Lax pairs for generating soliton equation with sources [<xref ref-type="bibr" rid="scirp.55822-ref1">1</xref>]. Then, Ma presented the soliton solutions of the Schr&#246; dinger equation with self-consistent sources [<xref ref-type="bibr" rid="scirp.55822-ref2">2</xref>]. The discrete case of using variational derivatives in generating sources was discussed in [<xref ref-type="bibr" rid="scirp.55822-ref3">3</xref>].</p><p>With the development of soliton theory, super integrable systems associated with fermi variables have been receiving growing attention. Various methods have been developed to search for new super integrable systems, Lax pairs, soliton solutions, symmetries and conservation laws, etc. [<xref ref-type="bibr" rid="scirp.55822-ref4">4</xref>]-[<xref ref-type="bibr" rid="scirp.55822-ref11">11</xref>]. In 1997, Hu proposed the super- trace identity and applied it to establish the super Hamiltonian structures of super-integrable systems [<xref ref-type="bibr" rid="scirp.55822-ref4">4</xref>]. Then Professor Ma gave a systematic proof of super trace identity and presented the super Hamiltonian structures of super AKNS hierarchy and super Dirac hierarchy for application [<xref ref-type="bibr" rid="scirp.55822-ref5">5</xref>]. The super Tu hierarchy and its super-Ha- miltonian structure was considered [<xref ref-type="bibr" rid="scirp.55822-ref6">6</xref>]. Recently, Yu et al. considered the binary nonlinearization of the super AKNS hierarchy under an implicit symmetry constraint [<xref ref-type="bibr" rid="scirp.55822-ref7">7</xref>] and the Bargmann symmetry constraint and binary nonlinearization of the super Dirac systems [<xref ref-type="bibr" rid="scirp.55822-ref8">8</xref>]. Meanwhile, various systematic methods have been developed to obtain exact solutions of the super integrable such as the inverse transformations, the B&#228; cklund and Darboux transformations, the bilinear transformation of Hirota and others [<xref ref-type="bibr" rid="scirp.55822-ref9">9</xref>]-[<xref ref-type="bibr" rid="scirp.55822-ref11">11</xref>].</p><p>This paper is organized as follows. In Section 2, the method for establishing super integrable soliton hierarchy with self-consistent sources by using Lie super algebra <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x3.png" xlink:type="simple"/></inline-formula> was presented. For application, the super Tu hierarchy with self-consistent sources was obtained in Section 3. In Section 4, conservation laws of super Tu hierarchy were given.</p></sec><sec id="s2"><title>2. A Kind of Super Integrable Soliton with Hierarchy Self-Consistent Sources</title><p>In the following. Consider a basis of Lie super algebra <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x4.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.55822-ref5">5</xref>]</p><disp-formula id="scirp.55822-formula186"><label>. (1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x5.png"  xlink:type="simple"/></disp-formula><p>We introduce the loop algebra <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x6.png" xlink:type="simple"/></inline-formula> as follows</p><disp-formula id="scirp.55822-formula187"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x7.png"  xlink:type="simple"/></disp-formula><p>where the loop algebra <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x8.png" xlink:type="simple"/></inline-formula> is defined by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x9.png" xlink:type="simple"/></inline-formula> .</p><p>Consider the auxiliary linear problem</p><disp-formula id="scirp.55822-formula188"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x10.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x11.png" xlink:type="simple"/></inline-formula> , <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x12.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x13.png" xlink:type="simple"/></inline-formula> <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x14.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x15.png" xlink:type="simple"/></inline-formula> are field va-</p><p>riables defining on<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x16.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x17.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x18.png" xlink:type="simple"/></inline-formula>.</p><p>From the spectral problem (3), the compatibility condition gives rise to the well-known zero curvature equation</p><disp-formula id="scirp.55822-formula189"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x19.png"  xlink:type="simple"/></disp-formula><p>The general scheme of searching for the consistent <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x20.png" xlink:type="simple"/></inline-formula> and generating a hierarchy of nonlinear equations was proposed as follows [<xref ref-type="bibr" rid="scirp.55822-ref5">5</xref>]. We solve the equation</p><disp-formula id="scirp.55822-formula190"><label>, (5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x21.png"  xlink:type="simple"/></disp-formula><p>And search for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x22.png" xlink:type="simple"/></inline-formula>, such that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x22.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x23.png" xlink:type="simple"/></inline-formula> can be constructed by</p><disp-formula id="scirp.55822-formula191"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x24.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x25.png" xlink:type="simple"/></inline-formula> are linear functions of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x25.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x26.png" xlink:type="simple"/></inline-formula> .</p><p>We consider the super trace identity of super integrable systems [<xref ref-type="bibr" rid="scirp.55822-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.55822-ref5">5</xref>]</p><disp-formula id="scirp.55822-formula192"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x27.png"  xlink:type="simple"/></disp-formula><p>where Str means the super trace. Defining a scalar <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x28.png" xlink:type="simple"/></inline-formula> by the equation</p><disp-formula id="scirp.55822-formula193"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x29.png"  xlink:type="simple"/></disp-formula><p>The sets <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x30.png" xlink:type="simple"/></inline-formula> proves the conserved densities of (4). The Hmailtonian form with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x31.png" xlink:type="simple"/></inline-formula> can be written as</p><disp-formula id="scirp.55822-formula194"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x32.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x33.png" xlink:type="simple"/></inline-formula> is a recursion operator and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x33.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x34.png" xlink:type="simple"/></inline-formula> is a symplectic operator, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x33.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x34.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x35.png" xlink:type="simple"/></inline-formula> .</p><p>According to (3) and (5), we consider the auxiliary linear problem. For <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x36.png" xlink:type="simple"/></inline-formula> distinct<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x37.png" xlink:type="simple"/></inline-formula>, the following systems result from (1)</p><disp-formula id="scirp.55822-formula195"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x38.png"  xlink:type="simple"/></disp-formula><p>Based on the results [<xref ref-type="bibr" rid="scirp.55822-ref11">11</xref>], we show that the following equations</p><disp-formula id="scirp.55822-formula196"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x39.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x40.png" xlink:type="simple"/></inline-formula> are constants. Equation (11) determines a finite dimensional invariant set for the flows (9).</p><p>For (10), it is known that</p><disp-formula id="scirp.55822-formula197"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x41.png"  xlink:type="simple"/></disp-formula><p>where Str denotes the super trace of a matrix and</p><disp-formula id="scirp.55822-formula198"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x42.png"  xlink:type="simple"/></disp-formula><p>According to (11), for a specific <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x43.png" xlink:type="simple"/></inline-formula> , we demand that</p><disp-formula id="scirp.55822-formula199"><label>(14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x44.png"  xlink:type="simple"/></disp-formula><p>From (9) and (11), a kind of super integrable hierarchy with self-consistent sources can be present as follows</p><disp-formula id="scirp.55822-formula200"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x45.png"  xlink:type="simple"/></disp-formula></sec><sec id="s3"><title>3. The Super Tu Hierarchy with Self-Consistent Sources</title><p>The super Tu spectral problem associated with Lie super algebra <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x46.png" xlink:type="simple"/></inline-formula>is given by [<xref ref-type="bibr" rid="scirp.55822-ref6">6</xref>]</p><disp-formula id="scirp.55822-formula201"><label>(16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x47.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x48.png" xlink:type="simple"/></inline-formula> is a spectral parameter, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x49.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x50.png" xlink:type="simple"/></inline-formula> are even variables, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x51.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x52.png" xlink:type="simple"/></inline-formula> are odd variables [<xref ref-type="bibr" rid="scirp.55822-ref6">6</xref>].</p><p>Taking</p><disp-formula id="scirp.55822-formula202"><graphic  xlink:href="http://html.scirp.org/file/55822x53.png"  xlink:type="simple"/></disp-formula><p>The co-adjoint equation associated with (16) <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x54.png" xlink:type="simple"/></inline-formula>gives</p><disp-formula id="scirp.55822-formula203"><label>(17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x55.png"  xlink:type="simple"/></disp-formula><p>If we set</p><disp-formula id="scirp.55822-formula204"><label>(18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x56.png"  xlink:type="simple"/></disp-formula><p>Then (17) is equivalent to</p><disp-formula id="scirp.55822-formula205"><label>(19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x57.png"  xlink:type="simple"/></disp-formula><p>Which results in the recurrence relations</p><disp-formula id="scirp.55822-formula206"><label>(20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x58.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.55822-formula207"><label>(21)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x59.png"  xlink:type="simple"/></disp-formula><p>Upon choosing the initial conditions</p><disp-formula id="scirp.55822-formula208"><graphic  xlink:href="http://html.scirp.org/file/55822x60.png"  xlink:type="simple"/></disp-formula><p>All other <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x61.png" xlink:type="simple"/></inline-formula> can be worked out by the recurrence relations (20). The first few sets are as follows:</p><disp-formula id="scirp.55822-formula209"><graphic  xlink:href="http://html.scirp.org/file/55822x62.png"  xlink:type="simple"/></disp-formula><p>Let us associate the problem (16) with the following auxiliary problem</p><disp-formula id="scirp.55822-formula210"><label>(22)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x63.png"  xlink:type="simple"/></disp-formula><p>The compatible conditions of the spectral problem (16) and the auxiliary problem (22) are</p><disp-formula id="scirp.55822-formula211"><label>(23)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x64.png"  xlink:type="simple"/></disp-formula><p>Which refer the super Tu equation hierarchy</p><disp-formula id="scirp.55822-formula212"><label>. (24)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x65.png"  xlink:type="simple"/></disp-formula><p>Here <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x66.png" xlink:type="simple"/></inline-formula> in (24) is called the n-th Tu flow of this hierarchy.</p><p>Using the super trace identity (7), we have</p><disp-formula id="scirp.55822-formula213"><label>(25)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x67.png"  xlink:type="simple"/></disp-formula><p>Therefore, the super Tu soliton hierarchy Equation (24) can be written as the following super Hamiltonian form:</p><disp-formula id="scirp.55822-formula214"><label>(26)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x68.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.55822-formula215"><graphic  xlink:href="http://html.scirp.org/file/55822x69.png"  xlink:type="simple"/></disp-formula><p>Is a super symplectic operator, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x70.png" xlink:type="simple"/></inline-formula> is given by (25).</p><p>The first non-trivial nonlinear of super Tu hierarchy is given by its second flow</p><disp-formula id="scirp.55822-formula216"><label>(27)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x71.png"  xlink:type="simple"/></disp-formula><p>Which possesses a Lax pair of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x72.png" xlink:type="simple"/></inline-formula> defined in (16) and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x73.png" xlink:type="simple"/></inline-formula> defined by</p><disp-formula id="scirp.55822-formula217"><graphic  xlink:href="http://html.scirp.org/file/55822x74.png"  xlink:type="simple"/></disp-formula><p>Next we will establish the super Tu hierarchy with self-consistent sources. Consider the linear system</p><disp-formula id="scirp.55822-formula218"><label>(28)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x75.png"  xlink:type="simple"/></disp-formula><p>For the system (28), we consider the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x76.png" xlink:type="simple"/></inline-formula> in the Lie super algebra <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x77.png" xlink:type="simple"/></inline-formula> and obtain</p><disp-formula id="scirp.55822-formula219"><label>(29)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x78.png"  xlink:type="simple"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x79.png" xlink:type="simple"/></inline-formula>.</p><p>According to the results in (15), the super Tu hierarchy with self-consistent sources is presented as</p><disp-formula id="scirp.55822-formula220"><label>(30)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x80.png"  xlink:type="simple"/></disp-formula><p>The first nontrivial integrable super Tu hierarchy with self-consistent sources is its second flow</p><disp-formula id="scirp.55822-formula221"><label>(31)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x81.png"  xlink:type="simple"/></disp-formula><p>When<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x82.png" xlink:type="simple"/></inline-formula>, it is the well known nonlinear Tu equation with self-consistent sources. So system (30) is a novel super integrable equation hierarchy.</p></sec><sec id="s4"><title>4. Conservation Laws for the Super Tu Hierarchy</title><p>In what follows, we will construct conservation laws of the super coupled Burgers equation. Introduce the variables:</p><disp-formula id="scirp.55822-formula222"><label>, (32)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x83.png"  xlink:type="simple"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x84.png" xlink:type="simple"/></inline-formula>. From (10), we have</p><disp-formula id="scirp.55822-formula223"><label>(33)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x85.png"  xlink:type="simple"/></disp-formula><p>We expand <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x86.png" xlink:type="simple"/></inline-formula> in powers of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x86.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x87.png" xlink:type="simple"/></inline-formula> as follows</p><disp-formula id="scirp.55822-formula224"><label>, (34)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x88.png"  xlink:type="simple"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x89.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x90.png" xlink:type="simple"/></inline-formula>. Substituting (34) into (33) and comparing the coefficients of the same powers of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x90.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x91.png" xlink:type="simple"/></inline-formula>, we obtain</p><disp-formula id="scirp.55822-formula225"><label>(35)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x92.png"  xlink:type="simple"/></disp-formula><p>And a recursion formula for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x93.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x93.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x94.png" xlink:type="simple"/></inline-formula>,</p><disp-formula id="scirp.55822-formula226"><label>(36)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x95.png"  xlink:type="simple"/></disp-formula><p>Because of</p><disp-formula id="scirp.55822-formula227"><label>(37)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x96.png"  xlink:type="simple"/></disp-formula><p>we derive the conservation laws of (27)</p><disp-formula id="scirp.55822-formula228"><label>(38)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x97.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.55822-formula229"><graphic  xlink:href="http://html.scirp.org/file/55822x98.png"  xlink:type="simple"/></disp-formula><p>Assume that<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x99.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x100.png" xlink:type="simple"/></inline-formula>, then (38) can be written as<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x101.png" xlink:type="simple"/></inline-formula>, which is the right form of conservation laws. We expand <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x102.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x103.png" xlink:type="simple"/></inline-formula> as series in powers of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x103.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x104.png" xlink:type="simple"/></inline-formula> according with the coefficients, which are called conserved densities and currents respectively</p><disp-formula id="scirp.55822-formula230"><label>, (39)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x105.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x106.png" xlink:type="simple"/></inline-formula> are constants of integration. Then the first two conserved densities and currents are</p><disp-formula id="scirp.55822-formula231"><graphic  xlink:href="http://html.scirp.org/file/55822x107.png"  xlink:type="simple"/></disp-formula><p>The recursion relations for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x108.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x108.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x109.png" xlink:type="simple"/></inline-formula> are</p><disp-formula id="scirp.55822-formula232"><label>(40)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55822x110.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x111.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x111.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55822x112.png" xlink:type="simple"/></inline-formula> can be calculated from (36). The infinitely conservations laws of (36) can be easily obtained in (32)-(40) respectively.</p></sec><sec id="s5"><title>Acknowledgements</title><p>This work was supported by the Natural Science Foundation of Henan Province (No. 132300410202), the Sci- ence and Technology Key Research Foundation of the Education Department of Henan Province (No. 12A- 110017, 14A110010), the Youth Backbone Teacher Foundation of Shangqiu Normal University (No. 2013- GGJS02).</p></sec><sec id="s6"><title>Cite this paper</title><p>Sixing Tao, (2015) Self-Consistent Sources and Conservation Laws for Super Tu Equation Hierarchy. Journal of Applied Mathematics and Physics,03,428-435. doi: 10.4236/jamp.2015.34054</p></sec></body><back><ref-list><title>References</title><ref id="scirp.55822-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Ma, W.X. and Strampp, W. (1994) An Explicit Symmetry Constraint for the Lax Pairs of AKNS Systems. 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