<?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">NS</journal-id><journal-title-group><journal-title>Natural Science</journal-title></journal-title-group><issn pub-type="epub">2150-4091</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ns.2014.67046</article-id><article-id pub-id-type="publisher-id">NS-45340</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Biomedical&amp;Life Sciences</subject><subject> Chemistry&amp;Materials Science</subject><subject> Earth&amp;Environmental Sciences</subject><subject> Medicine&amp;Healthcare</subject><subject> Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Hyperbolic Approximation on System of Elasticity in Lagrangian Coordinates
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>ose</surname><given-names>Francisco Caicedo</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>C.</surname><given-names>Klingenberg</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Yunguang</surname><given-names>Lu</given-names></name><xref ref-type="aff" rid="aff3"><sup>3</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Leonardo</surname><given-names>Rendon</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Departamento de Matemáticas, Universidad Nacional de Colombia, Bogotá, Colombia</addr-line></aff><aff id="aff3"><addr-line>Department of Mathematics, Hangzhou Normal University, Hangzhou, China</addr-line></aff><aff id="aff2"><addr-line>Institute of Mathematics, University of Würzburg, Würzburg, Germany</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>ylu2005@ustc.edu.cn(YL)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>25</day><month>04</month><year>2014</year></pub-date><volume>06</volume><issue>07</issue><fpage>477</fpage><lpage>486</lpage><history><date date-type="received"><day>14</day>	<month>December</month>	<year>2013</year></date><date date-type="rev-recd"><day>14</day>	<month>January</month>	<year>2014</year>	</date><date date-type="accepted"><day>21</day>	<month>January</month>	<year>2014</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p><html>
 <head></head>
 
   In this paper, we construct a sequence of hyperbolic systems (13) to approximate the general system of one-dimensional nonlinear elasticity in Lagrangian coordinates (2). For each fixed approximation parameter <img src="Edit_5721d2be-0d36-4302-bfbb-14f57f386ea9.bmp" alt="" height="12" width="10" />, we establish the existence of entropy solutions for the Cauchy problem (13) with bounded initial data (23).  
    
 
</html></p></abstract><kwd-group><kwd>Entropy Solutions</kwd><kwd> Isentropic Gas Dynamics</kwd><kwd> Lax Entropy</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Three most classical, hyperbolic systems of two equations in one-dimension are the system of isentropic gas dynamics in Eulerian coordinates</p><disp-formula id="scirp.45340-formula86958"><label>(1)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\e90d0cee-331b-4e77-b94d-2e940227ef26.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\54013913-6080-468b-abdc-56cde1b791c9.png" xlink:type="simple"/></inline-formula> is the density of gas, <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\bc71ffdc-457b-444f-8e6e-7cf171fdfea3.png" xlink:type="simple"/></inline-formula>the velocity and <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\e0798f82-a7db-458a-b128-103a420bc28e.png" xlink:type="simple"/></inline-formula> the pressure; the nonlinear hyperbolic system of elasticity</p><disp-formula id="scirp.45340-formula86959"><label>(2)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\810c0611-e843-4d75-ba6f-b843820b5387.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\f0dcb64a-588b-4e9e-a7d1-436d98e31829.png" xlink:type="simple"/></inline-formula> denotes the strain, <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\220f7190-82da-4573-b36a-fabca3665e8e.png" xlink:type="simple"/></inline-formula>is the stress and <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\0c4ba8f5-bbaf-4d8c-9740-2fa983a5b833.png" xlink:type="simple"/></inline-formula> the velocity, which describes the balance of mass and linear momentum, and is equivalent to the nonlinear wave equation</p><disp-formula id="scirp.45340-formula86960"><label>(3)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\83ad2b74-08a7-42f0-8f4c-a85058265293.png"  xlink:type="simple"/></disp-formula><p>and the system of compressible fluid flow</p><disp-formula id="scirp.45340-formula86961"><label>(4)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\1e154d22-4537-4933-ac55-802b11ba1501.png"  xlink:type="simple"/></disp-formula><p>To obtain the global existence of weak solutions for nonstrictly hyperbolic systems (two eigenvalues are real, but coincide at some points or lines), the compensated compactness theory (cf. [<xref ref-type="bibr" rid="scirp.45340-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.45340-ref2">2</xref>] or the books [<xref ref-type="bibr" rid="scirp.45340-ref3">3</xref>] -[<xref ref-type="bibr" rid="scirp.45340-ref5">5</xref>] ) is still a powerful and unique method until now.</p><p>For the polytropic gas <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\52a40f9f-ff4a-419b-aff3-8efa79aa172c.png" xlink:type="simple"/></inline-formula> where <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\c32a0a92-4731-4022-a54b-b539e98364f4.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\276f9da1-65c3-4f16-9dc2-ce0e6dc2d36c.png" xlink:type="simple"/></inline-formula> is an arbitrary positive constant, the Cauchy problem (1) with bounded initial data was completely resolved by many authors (cf. [<xref ref-type="bibr" rid="scirp.45340-ref6">6</xref>] -[<xref ref-type="bibr" rid="scirp.45340-ref11">11</xref>] ). When <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\35254b55-24f8-4527-a206-e7c2ae1a7573.png" xlink:type="simple"/></inline-formula> has the same principal singularity as the <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\798b997a-40f5-4b33-8e6c-9dada84d185c.png" xlink:type="simple"/></inline-formula>-law in the neighborhood of vacuum<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\efa76b63-9c06-418d-acba-d212d6f46466.png" xlink:type="simple"/></inline-formula>, a compact framework was first provided in [<xref ref-type="bibr" rid="scirp.45340-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.45340-ref13">13</xref>] and later, the necessary <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\9db8e0db-cc68-41bb-921f-64927b234288.png" xlink:type="simple"/></inline-formula> compactness of weak entropy-entropy flux pairs for general pressure function was completed in [<xref ref-type="bibr" rid="scirp.45340-ref14">14</xref>] .</p><p>Under the strictly hyperbolic condition <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\90028e5a-3252-4619-b049-345cd7d5b0eb.png" xlink:type="simple"/></inline-formula> and some linearly degenerate conditions <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\022179da-ee7b-4890-94f2-b40f7afef42c.png" xlink:type="simple"/></inline-formula> or <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\c0bd7c9b-73f3-4a19-a2c4-29418f1c5378.png" xlink:type="simple"/></inline-formula> as<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\614601e7-06be-45c3-8315-3b06cdb98404.png" xlink:type="simple"/></inline-formula>, the global existence of weak bounded solutions, or <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\70265142-7a13-460e-a48b-09fd0b0e24b9.png" xlink:type="simple"/></inline-formula> solutions, <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\aaf45ee4-5ea6-4918-9bbb-b47fc0d90da8.png" xlink:type="simple"/></inline-formula>was obtained by Diperna [<xref ref-type="bibr" rid="scirp.45340-ref15">15</xref>] and Lin [<xref ref-type="bibr" rid="scirp.45340-ref16">16</xref>] , Shearer [<xref ref-type="bibr" rid="scirp.45340-ref17">17</xref>] respectively.</p><p>Without the strictly hyperbolic restriction, a preliminary existence result of the nonlinear wave Equation (3) was proved in [<xref ref-type="bibr" rid="scirp.45340-ref18">18</xref>] for the special case <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\53140944-eb6c-4b97-855a-60771fb51441.png" xlink:type="simple"/></inline-formula> under the assumption <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\81578b6a-a20c-45bb-a5fc-287f4ab62ffd.png" xlink:type="simple"/></inline-formula> or<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\f7595dd7-fca2-4684-ad9a-d842290751a4.png" xlink:type="simple"/></inline-formula>.</p><p>Using the Glimm’s scheme method (cf. [<xref ref-type="bibr" rid="scirp.45340-ref19">19</xref>] ), Diperna [<xref ref-type="bibr" rid="scirp.45340-ref20">20</xref>] first studied the system (4) in a strictly hyperbolic region. Roughly speaking, for the polytropic case<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\abaf9828-09f6-4974-9386-e29306b204c2.png" xlink:type="simple"/></inline-formula>, Diperna’s results cover the case<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\e50afd84-287a-456e-9b71-b5905c3b2d76.png" xlink:type="simple"/></inline-formula>.</p><p>Since the solutions for the case of <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\ee215f87-5fb8-42a2-8f59-30f965fd5ffe.png" xlink:type="simple"/></inline-formula> always touch the vacuum, its existence was obtained in [<xref ref-type="bibr" rid="scirp.45340-ref21">21</xref>] by using the compensated compactness method coupled with some basic ideas of the kinetic formulations (cf. [<xref ref-type="bibr" rid="scirp.45340-ref10">10</xref>] [<xref ref-type="bibr" rid="scirp.45340-ref11">11</xref>] ). The existence of the Cauchy problem (7) for more general function <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\e38704e5-782f-4ed8-82ed-575627ed35b0.png" xlink:type="simple"/></inline-formula> was given in [<xref ref-type="bibr" rid="scirp.45340-ref22">22</xref>] under some conditions to ensure the <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\171d1a5a-b204-4f74-89d6-b04897a99618.png" xlink:type="simple"/></inline-formula> compactness for all smooth entropy-entropy flux pairs.</p><p>If all smooth entropy-entropy flux pairs satisfy the <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\dc0deb59-e401-4e8f-a886-2d66c3978f6f.png" xlink:type="simple"/></inline-formula> compactness, an ideal compactness framework to prove the global existence was provided by Diperna in [<xref ref-type="bibr" rid="scirp.45340-ref15">15</xref>] . For the above three systems (1)-(2) and (4), we can prove the <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\f472194c-342c-42ae-ba70-d1e6bf48525e.png" xlink:type="simple"/></inline-formula> compactness only for half of the entropies (weak or strong entropy).</p></sec><sec id="s2"><title>2. Main New Ideas</title><p>In [<xref ref-type="bibr" rid="scirp.45340-ref14">14</xref>] (see also [<xref ref-type="bibr" rid="scirp.45340-ref23">23</xref>] for inhomogeneous system), the author constructed a sequence of regular hyperbolic systems</p><disp-formula id="scirp.45340-formula86962"><label>(5)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\2502cf70-8c6d-47b5-b01d-7f7c5fe03534.png"  xlink:type="simple"/></disp-formula><p>to approximate system (1), where <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\d73ac7ba-6396-455b-af77-43841d9f443d.png" xlink:type="simple"/></inline-formula> in (5) denotes a regular perturbation constant and the perturbation pressure</p><disp-formula id="scirp.45340-formula86963"><label>(6)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\038efc1d-3ae9-4de7-90bc-a9145a979030.png"  xlink:type="simple"/></disp-formula><p>The most interesting point of this kind approximation is that both systems (5) and (1) have the same entropies (or the same entropy equation). In [<xref ref-type="bibr" rid="scirp.45340-ref14">14</xref>] , the <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\b6a57651-72d7-4d51-810a-46e24677d06e.png" xlink:type="simple"/></inline-formula> compactness of weak entropy-entropy flux pairs was also proved for general pressure function<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\75d4bb44-0b70-49b7-98f7-9a27e3bdeff2.png" xlink:type="simple"/></inline-formula>.</p><p>Let the entropy-entropy flux pairs of systems (1) and (5) be <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\26cc027a-9d80-4a55-b140-a0b241daf2d1.png" xlink:type="simple"/></inline-formula> and</p><p><inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\f600fda9-703c-40ee-8c4d-4c0058c77062.png" xlink:type="simple"/></inline-formula>respectively. Then by using Murat-Tartar theorem, we have</p><disp-formula id="scirp.45340-formula86964"><label>(7)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\47451e0e-4c70-4a54-ba48-9b75e56e2c88.png"  xlink:type="simple"/></disp-formula><p>for any fixed<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\31f81454-a891-42c8-b262-d9bc94100782.png" xlink:type="simple"/></inline-formula>, where the weak-star limit is denoted by <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\3a2784ff-8ebf-4f52-b6ff-546d36e0b71f.png" xlink:type="simple"/></inline-formula> as <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\80a40eb5-d96d-44cd-bd61-1d8c2d8f9311.png" xlink:type="simple"/></inline-formula> goes to zero.</p><p>Paying attention to the approximation function (6), we know that</p><disp-formula id="scirp.45340-formula86965"><label>(8)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\b4c849e7-0048-4aaf-9c56-eb73430f138d.png"  xlink:type="simple"/></disp-formula><p>are the entropy-entropy flux pairs of system</p><disp-formula id="scirp.45340-formula86966"><label>(9)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\72f26140-e833-4b86-b8c2-55f33a202744.png"  xlink:type="simple"/></disp-formula><p>or system</p><disp-formula id="scirp.45340-formula86967"><label>(10)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\38057d98-6007-44c8-b8c7-35f1adc6875f.png"  xlink:type="simple"/></disp-formula><p>respectively.</p><p>If we could prove from the arbitrary of <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\479d1006-b2e9-4f2c-9cf5-ab82fb57ce6a.png" xlink:type="simple"/></inline-formula> in (7) that</p><disp-formula id="scirp.45340-formula86968"><label>(11)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\4a2eadd9-24d1-4f17-a6b5-4cfe40a86d53.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.45340-formula86969"><label>(12)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\35bc13c9-8814-438f-a24a-1f8fe5b0b383.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\6fce9e31-a4d1-4d33-8f13-edb3ac0eb934.png" xlink:type="simple"/></inline-formula> denotes the weak-star limit <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\b95faf8b-3316-493e-9566-4a3bba22f19e.png" xlink:type="simple"/></inline-formula> as <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\1be9531f-466c-457d-bbbd-42e79e1b3040.png" xlink:type="simple"/></inline-formula> tend to zero, then we would have more function Equations (12) to reduce the strong convergence of <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\0b6a7b3b-fa2f-49ec-9342-55bbc2e75dbe.png" xlink:type="simple"/></inline-formula> as <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\9acff7e2-cd75-4bd2-bfa9-94ef31f0ad31.png" xlink:type="simple"/></inline-formula> tend to zero.</p><p>Between systems (2) and (4), we have the following approximation</p><disp-formula id="scirp.45340-formula86970"><label>(13)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\09cc880f-1fd4-423d-9bbd-701f36ee0c01.png"  xlink:type="simple"/></disp-formula><p>which has also the same entropy equation like system (2). If we could prove (11) and (12) from (7), then similarly we could prove the equivalence of systems (2) and (4). Moreover, we have much more information from system (13) to prove the existence of solutions for system (2) or (4).</p><p>Systems (13) and (2) have many common basic behaviors, such as the nonstrict hyperbolicity, the same entropy equation, same Riemann invariants and so on.</p></sec><sec id="s3"><title>3. Main Results</title><p>By simple calculations, two eigenvalues of system (13) are</p><disp-formula id="scirp.45340-formula86971"><label>(14)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\3793d11e-4307-48e9-afd3-a8117ac9a9fe.png"  xlink:type="simple"/></disp-formula><p>with corresponding right eigenvectors</p><disp-formula id="scirp.45340-formula86972"><label>(15)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\ca1dd3be-fba4-4395-a543-6f9440802268.png"  xlink:type="simple"/></disp-formula><p>and Riemann invariants</p><disp-formula id="scirp.45340-formula86973"><label>(16)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\e1f66619-e640-4d01-b99c-64ba3aaef283.png"  xlink:type="simple"/></disp-formula><p>Moreover</p><disp-formula id="scirp.45340-formula86974"><label>(17)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\ecb2cf16-48e9-46e5-848b-a82106b38339.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.45340-formula86975"><label>(18)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\c533c18f-087e-4d60-8667-94831e94f940.png"  xlink:type="simple"/></disp-formula><p>Any entropy-entropy flux pair <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\516b31a1-add2-44ba-9391-f043d543c060.png" xlink:type="simple"/></inline-formula> of system (13) satisfies the additional system</p><disp-formula id="scirp.45340-formula86976"><label>(19)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\c4a28a15-1cbf-44f0-aad9-36af17ffb355.png"  xlink:type="simple"/></disp-formula><p>Eliminating the <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\c2b364cb-651a-4841-b9e2-1069e6b998fe.png" xlink:type="simple"/></inline-formula> from (19), we have</p><disp-formula id="scirp.45340-formula86977"><label>(20)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\832342cc-c701-4548-b808-5092da714416.png"  xlink:type="simple"/></disp-formula><p>Therefore systems (13) and (2) have the same entropies. From these calculations, we know that system (13) is strictly hyperbolic in the domain <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\9530ae48-6441-4f53-a018-aed53039b72e.png" xlink:type="simple"/></inline-formula> or<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\2beb7060-aac1-4a3a-b7b3-972728cfaae4.png" xlink:type="simple"/></inline-formula>, while it is nonstrictly hyperbolic on the domain <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\6af9cdc5-b50e-4ac5-972a-950cc1722d40.png" xlink:type="simple"/></inline-formula> since <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\d13781d5-1f8f-4783-bf64-59cba307c726.png" xlink:type="simple"/></inline-formula> when<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\44c567a9-41dd-459d-8ede-1114ae04121d.png" xlink:type="simple"/></inline-formula>.</p><p>However, from (17) and (18), for each fixed<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\980d809c-58ab-478a-b316-3344dbb0970d.png" xlink:type="simple"/></inline-formula>, both characteristic fields of system (13) are genuinely nonlinear in the domain <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\3a418bff-5169-4525-9496-995ac9bd4c00.png" xlink:type="simple"/></inline-formula> if <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\bc6695c6-79f2-4c3f-9d50-5b6dc9606ebc.png" xlink:type="simple"/></inline-formula> or in the domain <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\91b85010-bdd4-4101-b1b4-c28c7e299e58.png" xlink:type="simple"/></inline-formula> if</p><p><inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\caac1947-8e36-47a6-a405-3e3fa2b5bb72.png" xlink:type="simple"/></inline-formula>. In the first case<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\8230e3e2-4528-4cde-b14f-6d46e756f3bb.png" xlink:type="simple"/></inline-formula>, we have an a-priori <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\6032ef22-3312-404c-b9e7-6e8337a11d4c.png" xlink:type="simple"/></inline-formula> estimate for the solutions of system (13)</p><disp-formula id="scirp.45340-formula86978"><label>(21)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\93f40f48-c1cf-4397-a12b-c7a235d5b3d0.png"  xlink:type="simple"/></disp-formula><p>because the region</p><p><img src="htmlimages\3-8302234x\73ed8c9b-dd48-437e-b39d-db356aebd52f.png" /></p><p>is an invariant region, where <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\0b5577e5-e6b4-4c65-ba69-e618697af5b3.png" xlink:type="simple"/></inline-formula> (<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\99e571b4-5e5d-403e-a22f-f9080ace6317.png" xlink:type="simple"/></inline-formula>is given in Theorem 1), <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\05ce248a-860a-42a6-9c63-889d8ee1bcb4.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\1c5c0189-2d9a-4d45-9a53-dbe2171aa51a.png" xlink:type="simple"/></inline-formula> are positive constants depending on the initial date, but being independent of<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\581b6937-fd20-41eb-b5a2-06f8c1b031ac.png" xlink:type="simple"/></inline-formula>. In the second case<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\31ff37e0-24f5-4415-bdcc-4bcc4658bc8c.png" xlink:type="simple"/></inline-formula>, we have the <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\b9f3d516-22fe-4af8-bedc-4216577c119e.png" xlink:type="simple"/></inline-formula> estimate</p><disp-formula id="scirp.45340-formula86979"><label>(22)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\6ecec0cf-422c-47e1-a916-4e1c901ac790.png"  xlink:type="simple"/></disp-formula><p>because the region</p><p><img src="htmlimages\3-8302234x\b3992755-e6cd-4c13-84a5-ad955987b30f.png" /></p><p>is an invariant region.</p><p>In this paper, for fixed<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\9c36239b-a2bd-4f99-bacf-e9602f80c01a.png" xlink:type="simple"/></inline-formula>, we first establish the existence of entropy solutions for the Cauchy problem (13) with bounded measurable initial data</p><disp-formula id="scirp.45340-formula86980"><label>(23)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\b90df001-a7a0-4b3c-9e23-7057f8000c23.png"  xlink:type="simple"/></disp-formula><p>In a further coming paper, we will study the relation between the functions equations (11) and (12), and the convergence of approximated solutions of system (13) as <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\9356ec17-d001-43e8-b193-905d83b00cf3.png" xlink:type="simple"/></inline-formula> goes to zero.</p><p>Theorem 1 Suppose the initial data <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\c266db19-d345-404c-b960-d935f6e6a165.png" xlink:type="simple"/></inline-formula> be bounded measurable. Let (I):</p><p><img src="htmlimages\3-8302234x\65ccf6cb-e9bd-47c3-afcc-d6be32a75c47.png" /></p><p>where <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\6fc362dc-9e45-49ef-bf9a-2fab269dc5e5.png" xlink:type="simple"/></inline-formula> is a positive constant, or (II):<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\68075803-358b-4e52-917e-fc62ff765ec4.png" xlink:type="simple"/></inline-formula>. Then the Cauchy problem (13)</p><p>with the bounded measurable initial data (23) has a global bounded entropy solution.</p><p>Note 1. The idea to use the flux perturbation coupled with the vanishing viscosity was well applied by the author in [<xref ref-type="bibr" rid="scirp.45340-ref24">24</xref>] to control the super-line, source terms and to obtain the <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\22ec43f1-942b-4d36-b1e1-8dfe978bfea4.png" xlink:type="simple"/></inline-formula> estimate for the nonhomogeneous system of isentropic gas dynamics.</p><p>Note 2. It is well known that system (2) is equivalent to system (1), but (1) is different from system (4) although the latter can be derived by substituting the first equation in (1) into the second. However, (4) can be considered as the approximation of (2). In fact, let <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\2ea0e89f-6e16-4844-a6c2-f96d00736b4d.png" xlink:type="simple"/></inline-formula> in (13). Then (13) is rewritten to the form</p><disp-formula id="scirp.45340-formula86981"><label>(24)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\0f965482-7960-4ca0-85f3-03c9c2201743.png"  xlink:type="simple"/></disp-formula><p>for some nonlinear function<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\2f9661f9-1d45-47a4-8328-b9c17efc9e9c.png" xlink:type="simple"/></inline-formula>.</p><p>Note 3. For any fixed<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\47d9dccc-bddf-4fbc-84d4-7c7cd5ceda23.png" xlink:type="simple"/></inline-formula>, the invariant region <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\93b3ba48-cba5-4b45-bf03-84191190bc3f.png" xlink:type="simple"/></inline-formula> above is bounded, so the vacuum is avoided. However, the limit of<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\5c04ee1d-4b4c-49b1-bea4-611723589fe2.png" xlink:type="simple"/></inline-formula>, as <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\4d09443d-d0e1-4d01-a81e-090dc619dea3.png" xlink:type="simple"/></inline-formula> goes to zero, is the original invariant region of system (2) because <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\91f20832-9c26-43a7-ae5f-013b91a3b96b.png" xlink:type="simple"/></inline-formula> could be infinity from the estimates in (21).</p><p>In the next section, we will use the compensated compactness method coupled with the construction of Lax entropies [<xref ref-type="bibr" rid="scirp.45340-ref25">25</xref>] to prove Theorem 1.</p></sec><sec id="s4"><title>4. Proof of Theorem 1</title><p>In this section, we prove Theorem 1.</p><p>Consider the Cauchy problem for the related parabolic system</p><disp-formula id="scirp.45340-formula86982"><label>(25)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\64d45675-e6e0-4eea-992d-ae6acfecdb5e.png"  xlink:type="simple"/></disp-formula><p>with the initial data (23).</p><p>We multiply (25) by <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\076f1f7a-672f-47e3-9f5e-28a02846c323.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\4b87af5b-103f-47da-be02-e8a76d3c8230.png" xlink:type="simple"/></inline-formula>, respectively, to obtain</p><disp-formula id="scirp.45340-formula86983"><label>(26)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\41fcdf9c-1207-4d91-a86e-c74bd34911a4.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.45340-formula86984"><label>(27)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\e1333d29-047b-4f94-966a-cf7797010833.png"  xlink:type="simple"/></disp-formula><p>Then the assumptions on <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\e67551dc-cf70-4bf4-ab3f-1a7b179777ea.png" xlink:type="simple"/></inline-formula> yield</p><disp-formula id="scirp.45340-formula86985"><label>(28)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\ebabebe9-7046-416b-890f-05fe6d807361.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.45340-formula86986"><label>(29)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\c1d25fa7-62d1-4617-8954-881da754373f.png"  xlink:type="simple"/></disp-formula><p>if<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\4881c688-5f74-4eed-852d-40387fee2b61.png" xlink:type="simple"/></inline-formula>; or</p><disp-formula id="scirp.45340-formula86987"><label>(30)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\c2a0be9f-07db-48bc-ac74-c4e258d22ca8.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.45340-formula86988"><label>(31)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\fb58c4fa-9ed9-4208-a98c-22ec019ca222.png"  xlink:type="simple"/></disp-formula><p>if <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\fe92e703-0093-46a8-80c8-dc543354a4f7.png" xlink:type="simple"/></inline-formula></p><p>If we consider (28) and (29) (or (30) and (31)) as inequalities about the variables <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\1cff7e00-de74-45c9-a923-feea148e6c97.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\1ffedbc4-f0b2-415b-aed6-5fc4978c264a.png" xlink:type="simple"/></inline-formula>, then we can get the estimates <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\065615d4-c26a-4fc5-83e8-f66ce549f00e.png" xlink:type="simple"/></inline-formula> by applying the maximum principle to (28) and (29) (or</p><p><inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\95b1539b-21f7-4957-870d-3d56abd7483f.png" xlink:type="simple"/></inline-formula>by applying the maximum principle to (30) and (31)). Then, using the first equation in (25), we get <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\7b3d6829-4d7f-4504-9113-c9852eeba2ca.png" xlink:type="simple"/></inline-formula> or <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\53ce11c1-1e68-4d68-94d2-ed373543cc07.png" xlink:type="simple"/></inline-formula> depending on the conditions on<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\c640115c-1400-4f3b-9198-06e403e0c9d6.png" xlink:type="simple"/></inline-formula>. Therefore, the region</p><p><img src="htmlimages\3-8302234x\9bef05c4-5f73-4f5d-9acc-36e38772b759.png" /></p><p>or</p><p><img src="htmlimages\3-8302234x\f5397cd0-c98d-4483-bc0d-280acdb94c15.png" /></p><p>is respectively an invariant region. Thus we obtain the estimates given in (21) or (22) respectively.</p><p>It is easy to check that system (13) has a strictly convex entropy when <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\b4420b41-d60c-4fff-953c-933696247bbf.png" xlink:type="simple"/></inline-formula> or <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\4cf7fe56-7eff-4eb2-ae49-1043b6526043.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.45340-formula86989"><label>(32)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\0cec5b85-2110-45e1-b7df-fd578fae6203.png"  xlink:type="simple"/></disp-formula><p>We multiply (4.1) by <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\1ad6d163-0907-4aef-a860-6167837b5c9d.png" xlink:type="simple"/></inline-formula> to obtain the boundedness of</p><disp-formula id="scirp.45340-formula86990"><label>(33)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\41b09f7a-8835-41c9-8803-7942bd6a3c33.png"  xlink:type="simple"/></disp-formula><p>in<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\f3dbe153-7cb1-494c-aa1b-90a07c615261.png" xlink:type="simple"/></inline-formula>. Then it follows that</p><disp-formula id="scirp.45340-formula86991"><label>(34)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\683a645e-f0d8-4370-b7de-c65bf2c33e91.png"  xlink:type="simple"/></disp-formula><p>is bounded in<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\f58d957a-f951-436b-9746-a4dc2d38ffb1.png" xlink:type="simple"/></inline-formula>. Since <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\7259dc22-da94-4cb7-b2ea-8b3fd01a856b.png" xlink:type="simple"/></inline-formula> for some bounded constants <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\79bc504d-9c2a-4fdc-9ce9-a9e99502c023.png" xlink:type="simple"/></inline-formula></p><p>when <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\96c991e6-d652-4d0f-8a55-f2bcdae5b964.png" xlink:type="simple"/></inline-formula> or<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\55c892d2-faaa-466c-b933-8d01885c986e.png" xlink:type="simple"/></inline-formula>, we get the boundedness of</p><disp-formula id="scirp.45340-formula86992"><label>(35)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\d8c1d527-6fa4-4940-ab7d-964d96d0bc10.png"  xlink:type="simple"/></disp-formula><p>for any fixed<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\73c5d29f-ed3a-4c22-8880-37de26bd381a.png" xlink:type="simple"/></inline-formula>.</p><p>Now we multiply (4.1) by<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\d71e897a-a268-4284-8f66-d3ff1f4a470e.png" xlink:type="simple"/></inline-formula>, where <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\278247d1-9aca-4122-adbc-315902573f8d.png" xlink:type="simple"/></inline-formula> is any smooth entropy of system (13), to obtain</p><disp-formula id="scirp.45340-formula86993"><label>(36)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\4f02204b-81c6-4818-b272-1114ee91a341.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\7c359e84-e298-4c3f-8960-0ace5d66cefd.png" xlink:type="simple"/></inline-formula> is the entropy-flux corresponding to<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\eed8cdaf-e7ee-4e8f-8615-debc12ba3777.png" xlink:type="simple"/></inline-formula>. Then using the estimate given in (35), we know that the first term in the right-hand side of (36) is compact in<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\4f8f82a9-e4d7-41b4-82bf-6107048f0ecc.png" xlink:type="simple"/></inline-formula>, and the second is bounded in</p><p><inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\67b6b16f-7b6e-477a-8072-df36417126a1.png" xlink:type="simple"/></inline-formula>. Thus the term in the left-hand side of (36) is compact in<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\a1c93a35-2fa6-4acf-9b1f-096608c55ee5.png" xlink:type="simple"/></inline-formula>.</p><p>Then for smooth entropy-entropy flux pairs <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\08a8e453-6710-4ff4-a1ca-1b0a3484de99.png" xlink:type="simple"/></inline-formula> of system (13), the following measure equations or the communicate relations are satisfied</p><disp-formula id="scirp.45340-formula86994"><label>(37)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\5bfbcac4-479c-4c8a-9e29-b5c525be8af6.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\74398fad-0407-4c91-bf0a-fcfd5bb23dfe.png" xlink:type="simple"/></inline-formula> is the family of positive probability measures with respect to the viscosity solutions <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\a55799e2-ce8f-4192-8ea4-34f678f137bf.png" xlink:type="simple"/></inline-formula> of the Cauchy problem (25) and (23).</p><p>To finish the proof of Theorem 1, it is enough to prove that Young measures given in (37) are Dirac measures.</p><p>For applying for the framework given by DiPerna in [<xref ref-type="bibr" rid="scirp.45340-ref5">5</xref>] to prove that Young measures are Dirac ones, we construct four families of entropy-entropy flux pairs of Lax’s type in the following special form:</p><disp-formula id="scirp.45340-formula86995"><label>(38)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\0f248d5d-9bc6-411c-8f5d-29b3939916d4.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.45340-formula86996"><label>(39)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\a4ffe9dc-e25a-4182-90ed-fdf72f5216b0.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.45340-formula86997"><label>(40)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\27963909-74d6-4d62-bba6-9a37892ec481.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.45340-formula86998"><label>(41)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\1ef635a8-d683-414b-b42e-67911f96cb92.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\f257f92c-1808-4da4-9a72-39718c626ced.png" xlink:type="simple"/></inline-formula> are the Riemann invariants of system (13) given by (16). Notice that all the unknown functions <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\26e9c6ee-a73c-4f9c-8b05-1d03c594ca68.png" xlink:type="simple"/></inline-formula> are only of a single variable<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\cb01b59f-e6cb-4806-afc2-ac0d0a1afb0c.png" xlink:type="simple"/></inline-formula>. This special simple construction yields an ordinary differential equation of second order with a singular coefficient <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\dd96f309-281b-4e98-bdf7-9d5d58339c95.png" xlink:type="simple"/></inline-formula> before the term of the second order derivative. Then the following necessary estimates for functions <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\17cbae35-aec5-41bf-b7e8-eca6b0d3d589.png" xlink:type="simple"/></inline-formula> are obtained by the use of the singular perturbation theory of ordinary differential equations:</p><disp-formula id="scirp.45340-formula86999"><label>(42)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\3b179bea-3692-427f-a240-dda4803f5add.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.45340-formula87000"><label>(43)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\22689675-5c30-4863-957c-013485de03e8.png"  xlink:type="simple"/></disp-formula><p>uniformly for <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\426e5bf2-cfc5-4e83-a183-a6532e81768b.png" xlink:type="simple"/></inline-formula> or<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\c0904f12-4d2b-47d0-904e-547a2ea0abd9.png" xlink:type="simple"/></inline-formula>, where <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\9132b220-156e-4a14-886a-40fab469175e.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\b3ad1e78-3c05-4093-bcff-da27f5a9db98.png" xlink:type="simple"/></inline-formula> is a positive constant independent of<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\2d00ff4e-305b-45ab-8e2b-053ebdc120f3.png" xlink:type="simple"/></inline-formula>.</p><p>In fact, substituting entropies <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\4e3076ce-b516-4e9d-999b-35a8477579a9.png" xlink:type="simple"/></inline-formula> into (20), we obtain that</p><disp-formula id="scirp.45340-formula87001"><label>(44)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\9518cb22-c06f-4470-89f5-19d6b7de8c74.png"  xlink:type="simple"/></disp-formula><p>Let</p><disp-formula id="scirp.45340-formula87002"><label>(45)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\6316074d-f535-4cc2-bdd0-6a59c667a81e.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.45340-formula87003"><label>(46)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\3ebfba6f-f5bc-4612-8a8f-731cbf00973e.png"  xlink:type="simple"/></disp-formula><p>Then</p><disp-formula id="scirp.45340-formula87004"><label>(47)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\00de96b1-b13a-4365-812a-c1885aaef3b5.png"  xlink:type="simple"/></disp-formula><p>The existence of <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\c8b5d3f1-6fcc-4cc6-b5c2-67e18f452d40.png" xlink:type="simple"/></inline-formula> and its uniform bound <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\48b2cb97-d1a4-419a-97b2-c8dc7b8cac6f.png" xlink:type="simple"/></inline-formula> on <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\d23a14c4-d499-4f0a-b4bd-a91b57f33f61.png" xlink:type="simple"/></inline-formula> or <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\d62c1a99-6d8c-4cce-bca3-05d4d53a4e85.png" xlink:type="simple"/></inline-formula> with respect to <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\b254b1af-eadd-4995-b815-d2b2cb3fca1f.png" xlink:type="simple"/></inline-formula> can be obtained by the following lemma (cf. [<xref ref-type="bibr" rid="scirp.45340-ref26">26</xref>] ) (also see Lemma 10.2.1 in [<xref ref-type="bibr" rid="scirp.45340-ref15">15</xref>] ):</p><p>Lemma 2 Let <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\2db025d7-3cab-4898-8f62-49c790003e61.png" xlink:type="simple"/></inline-formula> be the solution of the equation</p><p><img src="htmlimages\3-8302234x\66ba7631-1ed3-4ff2-954c-49f44b90c131.png" /></p><p>and functions <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\5fa7d23d-90c0-4142-9963-164bc14499b9.png" xlink:type="simple"/></inline-formula> be continuous on the regions</p><p><img src="htmlimages\3-8302234x\7706cc73-715f-4e59-b69d-481b6d27ec19.png" /></p><p>for some positive functions <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\fb996f0f-1373-4fac-befb-6c025bdc1390.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\05d1c4e2-170c-4558-b473-dfde975302fd.png" xlink:type="simple"/></inline-formula>. In addition,</p><p><img src="htmlimages\3-8302234x\d4c8ee5b-f0d7-4031-9283-95de902aa04e.png" /></p><p><img src="htmlimages\3-8302234x\f823eb48-64db-4a4a-a8b5-b029421658b7.png" /></p><p><img src="htmlimages\3-8302234x\f63c718f-b033-4c66-9d2a-4c0b7f928397.png" /></p><p>for some positive constants <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\6b8f25c2-f942-49a6-86a4-93fefc045707.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\458a684a-9339-43c5-a164-98f3c168b669.png" xlink:type="simple"/></inline-formula>.</p><p>If <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\ddafcd3f-6b06-40c9-91a4-e71dfa88e589.png" xlink:type="simple"/></inline-formula> is a solution of the following ordinary differential equation of second order:</p><p><img src="htmlimages\3-8302234x\156d1413-cb3e-49d6-9eae-f924fd665d06.png" /></p><p>with <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\6fe51ef6-ba86-46ec-a6dd-d3e786e311c6.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\e8d5ecd4-2bfb-4a3f-851f-379dbe8fca6f.png" xlink:type="simple"/></inline-formula> being arbitrary, then for sufficiently small <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\de13a889-0163-477b-98f7-a58b1e6f0b3f.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\72fca885-b1a1-4f4f-9d9c-ddda2b9fc540.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\09cce477-6581-4ee0-b92e-1b9cb85919db.png" xlink:type="simple"/></inline-formula>exists for all <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\d2865dc3-afae-4ed6-8c78-db75f641c525.png" xlink:type="simple"/></inline-formula> and satisfies</p><p><img src="htmlimages\3-8302234x\89b1c7f5-a2aa-439e-a774-f97a97d85b67.png" /></p><p>where <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\70b4b4ea-73e9-4b74-9824-d387f72055a2.png" xlink:type="simple"/></inline-formula></p><p>Furthermore, we can use Lemma 2 again to obtain the bound of <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\a037897b-39d6-424e-b6aa-680b878eec4e.png" xlink:type="simple"/></inline-formula> with respect to <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\c21873b2-2822-4857-bb73-116a5336e27f.png" xlink:type="simple"/></inline-formula> if we differentiate Equation (46) with respect to<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\b872afd0-0df1-42c1-9b78-4e210f438089.png" xlink:type="simple"/></inline-formula>.</p><p>By the second equation in (19), an entropy flux <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\928af25a-c719-4861-b2ec-a6ae07bb650e.png" xlink:type="simple"/></inline-formula> corresponding to <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\d28fa669-b514-498f-a6cd-e9bf84834575.png" xlink:type="simple"/></inline-formula> is provided by</p><disp-formula id="scirp.45340-formula87005"><label>(48)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\d1403b95-e3d0-4cdd-868e-4f44e8c51f6b.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.45340-formula87006"><label>(49)</label><graphic position="anchor" xlink:href="htmlimages\3-8302234x\2f3a309c-9633-45be-acab-0e1e442aa799.png"  xlink:type="simple"/></disp-formula><p>if <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\d09a73f9-0d3c-46a8-abb6-cacc6ba290cd.png" xlink:type="simple"/></inline-formula> or<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\4ee5b1f2-d580-48f9-b684-95b5ffa512e5.png" xlink:type="simple"/></inline-formula>, and <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\f6b249f9-0212-425f-b569-ea82023b3896.png" xlink:type="simple"/></inline-formula> both are bounded uniformly on <inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\f5e182a8-28ec-4b61-b35e-e18b8289857c.png" xlink:type="simple"/></inline-formula> or<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\e713c22b-019c-4583-98ec-19beb1356193.png" xlink:type="simple"/></inline-formula>.</p><p>In a similar way, we can obtain estimates on another three pairs of entropy-entropy flux of Lax type. Hence, Theorem 1 is proved when we use these entropy-entropy flux pairs in (38)-(41) together with the theory of compensated compactness coupled with DiPerna’s framework [<xref ref-type="bibr" rid="scirp.45340-ref15">15</xref>] .</p></sec><sec id="s5"><title>5. Conclusions</title><p>In this paper we have looked at the general system of one-dimensional nonlinear elasticity in Lagrangian coordinates (2).</p><p>We construct a hyperbolic approximations to this which are parameterized by<inline-formula><inline-graphic xlink:href="tmlimages\3-8302234x\bb5577c4-08a3-4d3f-bad4-8e9b6a44da34.png" xlink:type="simple"/></inline-formula>. They all have the same entropies as the original system. Under suitable assumptions we are able to establish uniform compactness estimates, and then obtain the existence of entropy solutions for the Cauchy problem.</p></sec><sec id="s6"><title>Acknowledgements</title><p>This work was partially supported by the Natural Science Foundation of Zhejiang Province of China (Grant No. LY12A01030 and Grant No. LZ13A010002) and the National Natural Science Foundation of China (Grant No. 11271105).</p></sec><sec id="s7"><title>NOTES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.45340-ref1"><label>1</label><mixed-citation publication-type="journal" xlink:type="simple"><name name-style="western"><surname>Murat</surname><given-names> F. </given-names></name>,<etal>et al</etal>. 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