<?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">APM</journal-id><journal-title-group><journal-title>Advances in Pure Mathematics</journal-title></journal-title-group><issn pub-type="epub">2160-0368</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/apm.2013.31A023</article-id><article-id pub-id-type="publisher-id">APM-27535</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>
 
 
  Scattering of the Radial Focusing Mass-Supercritical and Energy-Subcritical Nonlinear Schr&#246;dinger Equation in 3D
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>ujahid</surname><given-names>Abd Elmjed M-Ali</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>Amadu</surname><given-names>Fullah Kamara</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>Department of Mathematics, Faculty of Pure and Applied Sciences, Fourah Bay College, University of Sierra Leone, Freetown, Sierra Leone</addr-line></aff><aff id="aff1"><addr-line>Department of Mathematics, Faculty of Education, Kassala University, Kassala, Sudan</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>mujahid@mail.ustc.edu.cn(UAEM)</email>;<email>amadu_fullah2005@yahoo.com(AFK)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>30</day><month>01</month><year>2013</year></pub-date><volume>03</volume><issue>01</issue><fpage>164</fpage><lpage>171</lpage><history><date date-type="received"><day>October</day>	<month>2,</month>	<year>2012</year></date><date date-type="rev-recd"><day>November</day>	<month>5,</month>	<year>2012</year>	</date><date date-type="accepted"><day>November</day>	<month>13,</month>	<year>2012</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 studies the global behavior to 3D focusing nonlinear Schrodinger equation (NLS), the scaling index here is (0＜s<sub>c</sub>＜1), which is the mass-supercritical and energy-subcritical, and we prove under some condition the solution u(t) is globally well-posed and scattered. We also show that the solution “blows-up in finite time” if the solution is not globally defined, as t→T we can provide a depiction of the behavior of the solution, where T is the “blow-up time”. 
 
</p></abstract><kwd-group><kwd>NLS; Blows-Up in Finite Time; Supremum; Precompactness</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Consider the Cauchy problem for the nonlinear Schr&#246;- dinger equation (NLS) in dimensions d = 3:</p><disp-formula id="scirp.27535-formula82073"><label>(1.1)</label><graphic position="anchor" xlink:href="3-5300329\c539c783-fcc8-4766-87e7-4db81ccf80fe.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="3-5300329\7fb292b8-8c5d-4925-afc7-3039398bf46e.jpg" />is a complex-valued function in <img src="3-5300329\dba94970-21d5-4f09-80b0-622eeebdb913.jpg" />. The initial-value problem <img src="3-5300329\a0115619-cf78-4bbf-b633-a26be57dd850.jpg" /> is locally well-posed in<img src="3-5300329\eb882385-7411-4894-ab21-972f0ea9a4d8.jpg" />.</p><p>In this paper we will study the focusing (NLS) problem, which is the mass-supercritical and energy-subcritical, where <img src="3-5300329\e1a89439-5d8e-41a5-944b-d7420a87fa72.jpg" /></p><p>The Equation (1.1) has mass <img src="3-5300329\5a8290b9-ca52-4a05-ad4a-eaedbae11c0b.jpg" /> where</p><p><img src="3-5300329\bea3d75b-8a4f-40db-957c-d09eef870581.jpg" /></p><p>Energy <img src="3-5300329\4530971f-cff7-4dee-975e-ddb3a908a900.jpg" /> where</p><p><img src="3-5300329\990d9df8-247b-4fe7-8f21-10c12aca5615.jpg" /></p><p>and Momentum <img src="3-5300329\571d7900-07a0-434c-b857-69236264e28e.jpg" /> where</p><p><img src="3-5300329\1a67f784-d204-4cd7-8aac-ddd5e6d5fe63.jpg" />.</p><p>If<img src="3-5300329\74817458-2a22-4b73-a68c-5451b1d0c44b.jpg" />, then u satisﬁes</p><disp-formula id="scirp.27535-formula82074"><label>(1.2)</label><graphic position="anchor" xlink:href="3-5300329\03436b0d-329a-4776-a4fc-958a89121251.jpg"  xlink:type="simple"/></disp-formula><p>Equation (1.2) is said to be the Virial identity.</p><p>The Equation (1.1) has the scaling:</p><p><img src="3-5300329\bf61be78-d6df-4206-82d1-709c98ffbab7.jpg" /></p><p>and also this scaling is a solution if <img src="3-5300329\973cd20c-b20a-4fcd-b0b0-ccf1838fa080.jpg" /> is a solution.</p><p>Moreover, u<sub>0</sub> is a solution that is globally deﬁned by u, if it is globally deﬁned<img src="3-5300329\490a9632-e5dc-4d75-a90e-949fc480798b.jpg" />, and it does scatter (See [1,2]). We say the solution “blows-up in ﬁnite time”. If the solution is not globally deﬁned, as<img src="3-5300329\ed49273a-e066-4112-8e77-475310b4e5b3.jpg" />, we can provide a depiction of the behavior of the solution, where T is the “blow-up time”. It follows from the H<sup>1</sup> local theory optimized by scaling, that if blow-up in ﬁnite-time T &gt; 0 happens, (see [<xref ref-type="bibr" rid="scirp.27535-ref3">3</xref>] or [<xref ref-type="bibr" rid="scirp.27535-ref4">4</xref>]), then there is a lower-bound on the “blow-up rate”:</p><disp-formula id="scirp.27535-formula82075"><label>(1.3)</label><graphic position="anchor" xlink:href="3-5300329\8367a26e-e599-43a7-b874-5e549c0a82c6.jpg"  xlink:type="simple"/></disp-formula><p>for some constant c. Thus, to prove global presence, it suffices to prove a global axiomatic bound on<img src="3-5300329\eeb5f7ce-6ebf-4544-af4f-9c8a88c35bc4.jpg" />.</p><p>From the Strichartz estimates, there is a constant <img src="3-5300329\a92c2061-369f-46f1-8db7-d4f8f50d615a.jpg" /> such that if <img src="3-5300329\505736f5-06f8-4d90-ad50-cd7bb1318952.jpg" /> , then the solution <img src="3-5300329\4be66621-8910-4019-8122-6d7577f45695.jpg" /> is globally deﬁned and scattered.</p><p>Note that the quantities <img src="3-5300329\50fb22d9-eab9-4e14-a5be-fe4a4283d4e8.jpg" /> and</p><p><img src="3-5300329\d320703e-45d0-4fae-85fd-315c9934517c.jpg" />are also scale-invariant (See also [<xref ref-type="bibr" rid="scirp.27535-ref5">5</xref>]).</p><p>Let <img src="3-5300329\ca1f75af-ad8d-4647-906a-a1823caa5e10.jpg" /> then u solves (1.1) as long as</p><p><img src="3-5300329\5060b0c4-8d70-4488-a743-0ae7b030a2f3.jpg" />solves the nonlinear elliptic equation</p><disp-formula id="scirp.27535-formula82076"><label>(1.4)</label><graphic position="anchor" xlink:href="3-5300329\b60a6562-4f1f-4076-b2f0-509aec3429b4.jpg"  xlink:type="simple"/></disp-formula><p>Equation (1.4) has an inﬁnite number of solutions in<img src="3-5300329\5d8cd9b5-aeca-4325-99e6-0afe1134fd1e.jpg" />. The solution of minimal mass is denoted by <img src="3-5300329\51cf99cd-5d32-40d2-a1bf-9cbacaa617ce.jpg" /> and for the properties of <img src="3-5300329\b91dcb84-089c-4b8a-99e5-faa40ef7b9f1.jpg" /> see [3,5,6].</p><p>Under the condition<img src="3-5300329\cadf73b5-3b11-4c35-b465-0422321b0fcd.jpg" />, solutions to (1.1) globally exist if u<sub>0</sub> satisﬁes;</p><disp-formula id="scirp.27535-formula82077"><label>(1.5)</label><graphic position="anchor" xlink:href="3-5300329\34ee1993-7075-46ee-91e8-e424b97b9dd5.jpg"  xlink:type="simple"/></disp-formula><p>and there exist <img src="3-5300329\272819fa-2f1b-4d59-a5eb-7128e0fc6104.jpg" /> such that</p><p><img src="3-5300329\98d9ae01-20ff-4219-bc70-f7b283344721.jpg" />.</p><p>Theorem 1.1. Let<img src="3-5300329\f8fd155e-2b87-492a-9b15-3d8918928d45.jpg" />, and let <img src="3-5300329\6c0ba000-bc90-46a3-930d-3f2ec3f8c896.jpg" /> be the corresponding solution to (1.1) in H<sup>1</sup>. Suppose</p><disp-formula id="scirp.27535-formula82078"><label>(1.6)</label><graphic position="anchor" xlink:href="3-5300329\cc250512-97a7-4392-b306-5e9de5bccb5d.jpg"  xlink:type="simple"/></disp-formula><p>If <img src="3-5300329\31129672-83bd-45ca-b17c-0486da540028.jpg" /> then u scatters in H<sup>1</sup>.</p><p>The argument of [<xref ref-type="bibr" rid="scirp.27535-ref6">6</xref>] in the radial case followed a strategy introduced by [<xref ref-type="bibr" rid="scirp.27535-ref7">7</xref>] for proving global well-posedness and scattering for the focusing energy-critical NLS. The beginning used a contradiction to the argument: suppose the sill for scattering is strictly below that claimed. This uniform localization enabled the use of a local Virial identity to be established, with the support of the sharp Gagliardo-Nirenberg inequality, an accurately positive lower bound on the convexity (in time) of the local mass of u<sub>c</sub> Mass conservation is then violated at enough large time.</p><p>We show in this paper, that the above program carries over to the non-radial setting with the extension of two key components.</p><p>Theorem 1.2. Suppose the radial H<sup>1</sup> solution u to (1.1) blows-up at time <img src="3-5300329\40cfab73-130d-4a36-9f4b-357440d29681.jpg" />Then either there is a non-absolute <img src="3-5300329\ed699f61-0744-4f05-8c0b-bf7ce8755007.jpg" /> constant such that, as <img src="3-5300329\3fe4e52e-dc06-462a-92a4-aa4a784c46d1.jpg" /></p><disp-formula id="scirp.27535-formula82079"><label>(1.7)</label><graphic position="anchor" xlink:href="3-5300329\3a4472dd-4620-4114-a97c-e06d27014e83.jpg"  xlink:type="simple"/></disp-formula><p>or there exists a sequence of times <img src="3-5300329\b822e1a3-9f76-4fca-bd96-7cf97c15f773.jpg" /> such that for an absolute constant <img src="3-5300329\98bed724-2034-4724-8370-eeb285176715.jpg" /></p><disp-formula id="scirp.27535-formula82080"><label>(1.8)</label><graphic position="anchor" xlink:href="3-5300329\f4f250c3-8898-40f2-9c9f-8ae113621ccf.jpg"  xlink:type="simple"/></disp-formula><p>From (1.3), we have that the concentration in (1.7) satisﬁes<img src="3-5300329\c90270bc-7257-4900-b458-c228054fe44d.jpg" />, and the concentration in (1.8) satisﬁes <img src="3-5300329\63a49cdf-ac63-45f8-82ed-6162201659fc.jpg" /> (For more additional information see [8-10]).</p>Notation<p>Let <img src="3-5300329\f3005d53-0d56-4d03-851d-b210a60440fd.jpg" /> be the free Schr&#246;dinger propagator, and let<img src="3-5300329\d6999a18-d1a8-465d-9e27-ff902f657aea.jpg" />, with <img src="3-5300329\57c24cb2-722a-4d2c-b6fb-6257db79a161.jpg" /> be linear equation, a solution in physical space, is given by:</p><p><img src="3-5300329\de80e65f-e384-44b3-847c-1384b3a9225e.jpg" />and in frequency space</p><p><img src="3-5300329\15aa080b-a6ac-425e-af26-1d0caf60fb5a.jpg" /></p><p>In particular, they save the Farewell homogeneous Sobolev norms and obey the dispersive inequality</p><disp-formula id="scirp.27535-formula82081"><label>(1.9)</label><graphic position="anchor" xlink:href="3-5300329\0d4bff62-d4c6-4456-b095-0345e6d517cf.jpg"  xlink:type="simple"/></disp-formula><p>For all times<img src="3-5300329\cf79657f-d4ff-47b9-8f73-8c62b0c2a2f2.jpg" />.</p><p>Let <img src="3-5300329\e6731419-b4e9-4c34-b10a-95d81b0127b8.jpg" /> be a radial function, so that, <img src="3-5300329\e5a39edb-e5fa-41ba-9fd0-8538f91be70b.jpg" /> for <img src="3-5300329\86b1a28b-72ad-43aa-9ca0-afd507badcad.jpg" /> and <img src="3-5300329\9415965b-0e42-4eca-af12-2ca6af9e885f.jpg" /> for<img src="3-5300329\ffe4ffbd-1226-49ad-8e5a-c426f300c8e1.jpg" />, Deﬁne the inner and outer spatial localizations of <img src="3-5300329\75c4c36f-b152-4cef-83f0-17fa5388c2fc.jpg" /> at radius <img src="3-5300329\31e88f77-10f5-41d7-be1b-fa58e323b7a1.jpg" /> as</p><p><img src="3-5300329\e994742c-f35b-4032-8914-c302e2d32dec.jpg" /></p><p><img src="3-5300329\2106ae1e-4d25-4038-914c-496f510723a7.jpg" /></p><p>Let <img src="3-5300329\aaeab8e5-4c29-48d7-a26b-8f8c3a5f8a28.jpg" /> be a radial function so that,</p><p><img src="3-5300329\040b9fd9-d1f4-4d55-ad77-d93e42efcc92.jpg" />for <img src="3-5300329\2ebf7ad0-20ea-41fc-b9a2-5896dedc7356.jpg" /> and <img src="3-5300329\c6507dfa-604e-48d4-8ba7-e9c113bf99f1.jpg" /> for <img src="3-5300329\4b6b9531-5152-438c-9e0c-0e6f5b82c974.jpg" /> then</p><p><img src="3-5300329\5ac356d7-3293-471b-8f2f-2320fb4b30d3.jpg" />, and deﬁne the inner and outer indecision localizations at radius <img src="3-5300329\d0684e9d-832c-4c64-94bc-609b542ea61a.jpg" /> of u<sub>1</sub> as</p><p><img src="3-5300329\e72609cf-08cc-4f0e-8c67-f9efa3b4d1e0.jpg" />and</p><p><img src="3-5300329\ac5dd4c0-6c69-4863-a67d-b52e7abe5d57.jpg" />(the <img src="3-5300329\322589f7-ded0-4557-9c3e-628f154ff27d.jpg" /> and <img src="3-5300329\a37e56b5-1fbe-4b5e-bc18-f550b909d0e5.jpg" /> radii are chosen to be consistent with the assumption<img src="3-5300329\deedb6eb-beb4-48e3-943e-a36e622eea34.jpg" />, since<img src="3-5300329\a25a3b22-819f-4fe7-8581-791a94709d31.jpg" />. In reality, this is for suitability only; the argument is easily proper to the case where <img src="3-5300329\c73ba3fd-f3a3-46be-b755-573efc786a30.jpg" /> is any number<img src="3-5300329\a7ad495a-6858-41aa-8088-d604337103a5.jpg" />). We note that the indecision localization of <img src="3-5300329\0dba6440-3797-40c1-b3fa-223678282d40.jpg" /> is inaccurate, though decisively we have;</p><disp-formula id="scirp.27535-formula82082"><label>(1.10)</label><graphic position="anchor" xlink:href="3-5300329\4de5e1dd-45d7-49ae-b8ad-5602bc3558d4.jpg"  xlink:type="simple"/></disp-formula></sec><sec id="s2"><title>2. Proof of Theorem 1.2</title><p>In this section we discuss a proof of Theorem (1.2).</p><p>Proposition 2.1. Let u be an H<sup>1</sup> radial solution to (1.1) that blows-up in ﬁnite<img src="3-5300329\d3f062a5-2b29-4a81-9576-62ff40784f6c.jpg" />. Let</p><p><img src="3-5300329\061fbee1-c28b-4a35-80a4-89d107f55ae0.jpg" /></p><p>and<img src="3-5300329\bbbd47f9-47fa-441e-809a-c4f8a1535090.jpg" />, (Where c<sub>1</sub> and c<sub>2</sub> are absolute constants), and <img src="3-5300329\ec93e9e2-8532-4871-afa4-d55f6cab89b9.jpg" /> as characterized in the paragraph above.</p><p>1) There exists an absolute constant <img src="3-5300329\9fc4177d-c09f-468c-8aec-009c7318bf5f.jpg" /> such that</p><disp-formula id="scirp.27535-formula82083"><label>(2.1)</label><graphic position="anchor" xlink:href="3-5300329\6b717b6d-8586-4e01-bc00-97395735f8c8.jpg"  xlink:type="simple"/></disp-formula><p>2) Let us assume that there exists a constant <img src="3-5300329\1f06ddbf-4722-4c67-815b-606cd825d854.jpg" /> such that<img src="3-5300329\1fd8ee10-3f4b-46af-b92b-e7086f877a42.jpg" />. Then</p><disp-formula id="scirp.27535-formula82084"><label>(2.2)</label><graphic position="anchor" xlink:href="3-5300329\92ea88f7-23d0-47d2-8338-e3935feaae27.jpg"  xlink:type="simple"/></disp-formula><p>for some absolute constant c &gt; 0, where <img src="3-5300329\a16fb885-ad5b-4f54-9b29-8ac25cb7ea94.jpg" /> is a stance function such that</p><p><img src="3-5300329\c1ce1e3c-dfc5-4aa4-a651-d862606a4477.jpg" /></p><p>We recall, an “exterior” estimate, usable to radially symmetric functions only, originally due to [<xref ref-type="bibr" rid="scirp.27535-ref11">11</xref>]:</p><disp-formula id="scirp.27535-formula82085"><label>(2.3)</label><graphic position="anchor" xlink:href="3-5300329\d175ba2f-4c43-429b-88ec-e5ca9b4b7f43.jpg"  xlink:type="simple"/></disp-formula><p>where c is independent of R &gt; 0. We recall the generally usable symmetric functions and for any function <img src="3-5300329\279b6f8a-1eaa-45d8-b0ef-c1f5c19b7bb2.jpg" /></p><disp-formula id="scirp.27535-formula82086"><label>(2.4)</label><graphic position="anchor" xlink:href="3-5300329\cb35cfaf-d53b-4b04-8063-d4a8f0650ee0.jpg"  xlink:type="simple"/></disp-formula><p>(2.3), (2.4) are Gagliardo-Nirenberg estimates for functions on<img src="3-5300329\7415d51d-a24e-4cf6-95c1-eafecd7f4e01.jpg" />.</p><p>Proof of Prop 2.1: Since by (1.3), <img src="3-5300329\352f86e7-0e23-47f5-ac6a-a2c96c6e431d.jpg" />as <img src="3-5300329\0ac7791c-950c-41dd-99d0-bb442356e984.jpg" /> by energy conservation, we have</p><p><img src="3-5300329\98f6cb37-c95c-4fb0-9f08-058e1cd842d7.jpg" />Thus, for t to be large enough to close to T</p><disp-formula id="scirp.27535-formula82087"><label>(2.5)</label><graphic position="anchor" xlink:href="3-5300329\56778f76-8f2e-4ecc-8d90-12b43eee38c4.jpg"  xlink:type="simple"/></disp-formula><p>By (2.3), the selection of <img src="3-5300329\005a7e64-bb75-4ff9-8c06-6bf34fc5e2cf.jpg" /> and mass conservation;</p><disp-formula id="scirp.27535-formula82088"><label>(2.6)</label><graphic position="anchor" xlink:href="3-5300329\c5ae353f-fe69-4f26-97a6-c7b0e5bdad1d.jpg"  xlink:type="simple"/></disp-formula><p>where c<sub>1</sub> in the deﬁnition of <img src="3-5300329\beaa19e4-6d8c-4217-8c64-fdbc2faca70b.jpg" /> has been selected to obtain the factor <img src="3-5300329\1b51e835-edee-4b2e-9233-5cd65e1f695b.jpg" /> here. By Sobolev embedding, (1.10), and the selected <img src="3-5300329\1fe75f8d-c63f-4a24-8c44-b63182e03708.jpg" /></p><disp-formula id="scirp.27535-formula82089"><label>(2.7)</label><graphic position="anchor" xlink:href="3-5300329\c710cb15-fe8c-4d5a-b7a3-1b8d15ef6a4e.jpg"  xlink:type="simple"/></disp-formula><p>where c<sub>2</sub> in the deﬁnition of <img src="3-5300329\1cda7e56-f5ee-477a-b308-de30ed14b4f4.jpg" /> has been selected to obtain the factor <img src="3-5300329\9ba74633-4a51-4dab-bd05-ff0633dea595.jpg" /> here. Bring together (2.5), (2.6), and (2.7), to obtain</p><disp-formula id="scirp.27535-formula82090"><label>(2.8)</label><graphic position="anchor" xlink:href="3-5300329\1a67bf51-b6f6-4ab0-932f-431bdaa6dbda.jpg"  xlink:type="simple"/></disp-formula><p>By (2.8) and (2.4), we obtain (2.1), completing the proof of part (1) of the proposition.</p><p>To prove part (2), we assume <img src="3-5300329\89594f29-4fcd-4efb-aeb8-92b8795d6a46.jpg" /> by (2.8)</p><p><img src="3-5300329\07a813cd-9ef0-40c6-8f8b-3040b8f22cf8.jpg" /></p><p>There exists <img src="3-5300329\83891468-ebd8-48f3-9b8a-5b4aa971d2f7.jpg" /> for which at least <img src="3-5300329\518fa7ea-eedc-44bf-83c7-8b66364949b5.jpg" /> of this supremum is attained. Thus,</p><p><img src="3-5300329\ef8532b2-d3c9-4c71-97da-d821155f393e.jpg" /></p><p>where we used H&#246;lder’s inequality in the last step. By the selected<img src="3-5300329\fc8be77b-8b3f-419b-8afd-fd935cde0eb1.jpg" />, we obtain (2.2). To complete the proof, it keeps to obtain the remind control on <img src="3-5300329\84cef0f5-b278-4d87-ade6-5462fb62cc40.jpg" /> which will be a consequence of the radial supposition and the supposed bound <img src="3-5300329\e4d90e64-c4e9-46e2-9f75-a880c5eb92ca.jpg" /></p><p>Assume <img src="3-5300329\269a2b82-704f-4c89-b37c-33bfb1103f87.jpg" /> along a sequence of times <img src="3-5300329\eb572c3c-74a3-4b35-90f8-4c7f8b870cc3.jpg" /> Assume the spherical annulus;</p><p><img src="3-5300329\2ae070cb-0122-42ab-8894-da4deceaf70f.jpg" /></p><p>And inside A place <img src="3-5300329\d665faae-ef2b-4bc9-ba44-4a474686385c.jpg" /> disjoint balls, at radius <img src="3-5300329\65c73a16-677d-4851-b601-a9a568fa301d.jpg" /> both the radius<img src="3-5300329\0a25f6b2-d999-42c1-8d06-0f3c1a9c8d90.jpg" />, centered on the sphere. By the radiality supposition, on all ball B, we have</p><p><img src="3-5300329\9a840a89-ba13-4b3c-bcce-9dff4500694a.jpg" />, and hence on the annulus A,</p><p><img src="3-5300329\69a0b229-107c-4da3-84b3-e6be2dd08383.jpg" />.</p><p>which contradicts the assumption<img src="3-5300329\e3350daf-d205-4b46-abb2-f0c8f518666b.jpg" />. <img src="3-5300329\39438608-b401-4466-a3c8-bd3d9648168b.jpg" /></p><p>We now point out how to obtain Theorem 1.2 as a consequence.</p><p>Proof of Theorem 1.2. By part (1) of Prop. 2.1 and the standard convolution inequality:</p><p><img src="3-5300329\b8abb676-3828-43d0-8c91-5188eae3e82e.jpg" />.</p><p>If <img src="3-5300329\03e38ef0-fed9-4708-9954-882374fcfc88.jpg" /> is not bounded, then there exists a sequence of times <img src="3-5300329\17cf8d1a-a4e8-4a3b-bd1c-a039119d323e.jpg" /> such that <img src="3-5300329\823c89ec-18fd-4f89-a55f-c3c0aa8feec3.jpg" /> Since</p><p><img src="3-5300329\690fcc78-b997-49ec-b150-2148d8b9e770.jpg" />, we have (1.8) in Theorem 1.2;</p><p>on the other hand, if<img src="3-5300329\b7247612-97de-4f1f-82f5-c7d1b76a1432.jpg" />, for some c<sup>*</sup>, as t &#174; Twe have (2.2) of Prop. 2.1. Since<img src="3-5300329\08060e91-8358-470c-b456-0a90079959f1.jpg" />, we have</p><p><img src="3-5300329\37648ee9-d50b-4c72-94ce-d826f90ad891.jpg" /></p><p>which gives (1.7) in Theorem 1.2. <img src="3-5300329\7c12ffb3-c14a-4c98-977a-9eaa334daa22.jpg" /></p></sec><sec id="s3"><title>3. Strichartz Estimates</title><p>In this section we show local theory and Strichartz estimates.</p>Strichartz Type Estimates<p>We say the pair <img src="3-5300329\5a3726ee-6b47-4a96-ab28-9fc0cbbd60ba.jpg" /> is <img src="3-5300329\f7cf6d70-1f01-475b-9fff-da1e62662745.jpg" /> Strichartz admissible if</p><p><img src="3-5300329\25d7ea33-bc57-49a7-984d-6fdd57dc0288.jpg" />, with<img src="3-5300329\2d5cba5c-7508-4653-b5d5-dc8a405d921c.jpg" />, <img src="3-5300329\f6950aef-2597-4827-b733-6b7b9afdf731.jpg" />and<img src="3-5300329\b7178c0e-8728-4fa8-b707-e26c60d36189.jpg" />. And the pair <img src="3-5300329\48dbf609-c03c-4808-92c8-b068b70045b4.jpg" /> is <img src="3-5300329\dc1d4a96-2591-49c3-b5aa-61738feb4fcc.jpg" />-passable if<img src="3-5300329\6f67b83c-e581-40dc-b3c1-d2b69f00f861.jpg" />, <img src="3-5300329\bb2ed350-5a00-4e0a-93cc-f86c5d825207.jpg" />, <img src="3-5300329\17b88db0-b208-4992-b70e-ac57c1bcdb0c.jpg" />or<img src="3-5300329\214925fc-16bb-4745-9ab1-e47ba7a1d1eb.jpg" />.</p><p>As habitual we denote by <img src="3-5300329\e6254fca-7d75-44b2-96c4-e1803d43ec3e.jpg" /> the H&#246;lder conjugates of q and r consecutive (i.e.<img src="3-5300329\13560514-b23c-4890-87b5-5bb1a07bc473.jpg" />).</p><p>Let</p><p><img src="3-5300329\17a2f024-8b83-45a8-9325-001651fd5041.jpg" /></p><p>We consider dual Strichartz norms. Let</p><p><img src="3-5300329\3beeb9fc-f29f-4e81-9489-d31011685e66.jpg" /></p><p>where <img src="3-5300329\1302a588-45f2-4d48-af33-a017a2bd6a33.jpg" /> is the H&#246;lder dual to<img src="3-5300329\21aa74f1-33c7-4d84-8390-d2334a8fd5a3.jpg" />. Also deﬁne</p><p><img src="3-5300329\94ce4db5-a338-496b-b766-4c58cda0c603.jpg" /></p><p>The Strichartz estimates are:</p><p><img src="3-5300329\3527ef10-a235-49fb-b67c-7332876d34fb.jpg" /></p><p>and</p><p><img src="3-5300329\778d028f-b99e-48ce-b59e-7578a0f28b41.jpg" />.</p><p>By bring together Sobolev embedding with the Strichartz estimates, we obtain</p><p><img src="3-5300329\60ea243c-0389-4b3d-ae4a-c82b9a54e6e8.jpg" /></p><p>and</p><disp-formula id="scirp.27535-formula82091"><label>(3.1)</label><graphic position="anchor" xlink:href="3-5300329\27bd3e42-ff80-4e4f-9bff-5ae6e546528d.jpg"  xlink:type="simple"/></disp-formula><p>We must also need the Kato inhomogeneous Strichartz estimate [<xref ref-type="bibr" rid="scirp.27535-ref12">12</xref>].</p><disp-formula id="scirp.27535-formula82092"><label>. (3.2)</label><graphic position="anchor" xlink:href="3-5300329\5f10ad46-a257-4b8b-97da-1338e60e71b5.jpg"  xlink:type="simple"/></disp-formula><p>To point out a restriction to a time subinterval <img src="3-5300329\40d7e139-3f50-43f9-a0a0-0fd014eb57e6.jpg" />, we will write <img src="3-5300329\68a98b51-eb80-4b05-8831-3fb32dfe2a62.jpg" /> or<img src="3-5300329\2b083cd9-fda2-4006-a0a7-209e80fd1423.jpg" />.</p><p>Proposition 3.1 Assume<img src="3-5300329\12d97c3c-db99-44f1-a50b-36e9179b9582.jpg" />. There is <img src="3-5300329\41ff8456-775e-495c-a8cb-963f97973a72.jpg" /> such that if<img src="3-5300329\fb20bb60-193e-4018-a71c-883025d46689.jpg" />, then u solving (1.1) is global (in<img src="3-5300329\aaf85743-2c15-4f17-8c4d-58016d823592.jpg" />) and</p><p><img src="3-5300329\338e9fd7-e173-4c5c-b666-5af5852be6f2.jpg" />,</p><p><img src="3-5300329\2440d2c6-2474-44f1-b841-896868d11195.jpg" />.</p><p>(Observe that, by the Strichartz estimates, the assumptions are satisﬁed if<img src="3-5300329\899a3bef-7585-4ff3-b1cc-15c942b29138.jpg" />).</p><p>Proof. Deﬁne</p><p><img src="3-5300329\8bf30c7a-6d3d-4278-b022-84d53e015b0d.jpg" />.</p><p>Applying the Strichartz estimates, we obtained</p><p><img src="3-5300329\cf73a2fd-60ea-4637-ab99-f6e7a669cd29.jpg" /></p><p>and</p><p><img src="3-5300329\d3615aef-52a2-4e7d-a349-ba9feba49548.jpg" /></p><p>We apply the H&#246;lder inequalities and fractional Leibnitz [<xref ref-type="bibr" rid="scirp.27535-ref13">13</xref>] to get</p><p><img src="3-5300329\29284fcd-855d-4b4e-80ff-84a2e5fdef58.jpg" /></p><p>Let</p><p><img src="3-5300329\7ffa8269-bf9e-46d7-895c-bd8a9d2bbf82.jpg" /></p><p>Then <img src="3-5300329\29556b00-dfb3-4e5e-bb81-0bdcb4c5b62b.jpg" /> where</p><p><img src="3-5300329\6a28de1a-3d45-4f05-846e-1344fd9f5923.jpg" /></p><p>and <img src="3-5300329\a7f87e2e-1460-4911-975e-d5d19a32654c.jpg" /> is a contraction on N. <img src="3-5300329\b35bb388-d442-4a10-9ce2-54a4d07c174e.jpg" /></p><p>Proposition 3.2. If <img src="3-5300329\cd038cec-0633-4c00-acdb-7ee5a7d4b799.jpg" /> is global with globally ﬁnite <img src="3-5300329\03e8b998-27d3-44d2-af4a-9fe0027cc6de.jpg" /> Strichartz norm <img src="3-5300329\d5719f02-9bd0-42a3-ab33-25f77700efa6.jpg" /> and a uniformly bounded H<sup>1</sup> norm <img src="3-5300329\832803ae-30e8-4390-b4f9-a2ecd3fd6527.jpg" /> then <img src="3-5300329\907b2647-e1ec-46a5-817a-86fc7db0b6b8.jpg" /> scatters in H<sup>1</sup> as<img src="3-5300329\3761a167-e30b-4023-b5e3-810658418d98.jpg" />.</p><p>Meaning that there exist <img src="3-5300329\71282a11-806c-4a64-bf93-3dbad0d957b3.jpg" /> such that</p><p><img src="3-5300329\3a408efd-bcb4-4619-b444-74e8f7069405.jpg" /></p><p>Proof. Since <img src="3-5300329\e5c3b2ff-33ae-4923-9e6d-f23022faba8e.jpg" /> resolves the integral equation</p><p><img src="3-5300329\0628fce5-2ac4-4c9c-9c0f-843fedd725cf.jpg" /></p><p>we have</p><disp-formula id="scirp.27535-formula82093"><label>(3.3)</label><graphic position="anchor" xlink:href="3-5300329\00ccf7ff-b6ed-48c3-9200-8e41a739c829.jpg"  xlink:type="simple"/></disp-formula><p>where</p><p><img src="3-5300329\ba191ab5-9505-47c8-97c7-290b07da52aa.jpg" /></p><p>Apply the Strichartz estimates to (3.3), to get</p><p><img src="3-5300329\bfbea66f-d617-4f6e-ba3b-963c3be3026c.jpg" /></p><p>As <img src="3-5300329\06fc81c1-5475-4aca-9a9d-d2d1ba8a90f6.jpg" /> above inequality get the claim. <img src="3-5300329\0f5e9d12-54ed-479f-84c5-26cc34feac28.jpg" /></p></sec><sec id="s4"><title>4. Some Lemma</title><sec id="s4_1"><title>4.1. Here We Discuss the Precompactness of the Flow Implies Regular Localization</title><p>Let u be a solution to (1.1) such that</p><disp-formula id="scirp.27535-formula82094"><label>(4.1)</label><graphic position="anchor" xlink:href="3-5300329\61159bd1-0d6d-46a0-a7ba-f3f61dd76fc0.jpg"  xlink:type="simple"/></disp-formula><p>is precompact in H<sup>1</sup>. Then for each <img src="3-5300329\d5fe2211-d408-4b98-9ae5-9f2640f734b6.jpg" /> there exist &#160;R &gt; 0 so that <img src="3-5300329\898d3e0f-4952-4a60-8c71-a6ed3017cf62.jpg" /> for all <img src="3-5300329\b97eec81-1b4e-4759-885f-1fe54ba9589b.jpg" /></p><p>We proof (4.2) by contradiction, there exists <img src="3-5300329\9016f6ba-f728-44d9-8c94-d481557fecfc.jpg" /> and a sequence of times <img src="3-5300329\1d9f4853-5555-431d-9229-537403ac8b64.jpg" /> and by changing the variables,</p><disp-formula id="scirp.27535-formula82095"><label>(4.3)</label><graphic position="anchor" xlink:href="3-5300329\79a2bb09-54ad-47d6-a54a-3a94f9b7486b.jpg"  xlink:type="simple"/></disp-formula><p>Since K is precompact, there exists<img src="3-5300329\d5362820-97c7-42be-800e-5d6abaefab7b.jpg" />, such that <img src="3-5300329\b7b46b77-2ec6-49b3-ba7f-33076469876e.jpg" /> in H<sup>1</sup>, by (4.3),</p><p><img src="3-5300329\56d23909-9813-43ca-8d52-c622fec67626.jpg" /></p><p>Which is a contradiction with the fact that <img src="3-5300329\1dd6d365-c6c9-4a05-b0c4-e11c21981943.jpg" /> The proof is complete.</p><p>Lemma 4.1. Let u be a solution of (1.1) deﬁned on<img src="3-5300329\34652d05-b4dc-4c1f-9bb5-a7849dc31b9c.jpg" />, such that <img src="3-5300329\a4e4a8ea-078d-4829-9671-1245174f0967.jpg" /> and K such as in (4.1) is precompact in H<sup>1</sup>, for some continuous function <img src="3-5300329\d0cd24db-a739-4344-b708-c0a8f3e30f81.jpg" /> then;</p><disp-formula id="scirp.27535-formula82096"><label>(4.4)</label><graphic position="anchor" xlink:href="3-5300329\2835408f-60a2-4d2a-acdd-052a4c400ce8.jpg"  xlink:type="simple"/></disp-formula><p>Proof. Suppose that (4.4) does not hold. Then there exists a sequence<img src="3-5300329\72982742-d98f-44dd-92dc-0433a4d58be8.jpg" />, such that <img src="3-5300329\f96dd4cb-5ff8-4536-9b69-97647d3e5303.jpg" /> for some ε<sub>0</sub> &gt; 0. Retaining generality, we assume <img src="3-5300329\5c7444f8-d0e6-4111-85dd-d8db687a8ed8.jpg" /> For R &gt; 0, let</p><p><img src="3-5300329\cc2a9528-c3cd-4c14-b593-48d9b0762c47.jpg" /></p><p>i.e. <img src="3-5300329\5dd14d73-e389-43b1-88dc-ebe8045fb417.jpg" />is the ﬁrst time when <img src="3-5300329\4c4a0498-f28a-472a-866f-b0f6140cccb4.jpg" /> arrives at the boundary of the ball of radius R. By continuity of<img src="3-5300329\179b6501-9029-4a95-b8ee-bff2d8055784.jpg" />, the value <img src="3-5300329\925159c0-b05c-4dad-9c5d-104a217b1a92.jpg" /> is well-deﬁned. Furthermore, the following hold:</p><p>1) <img src="3-5300329\79eca473-30ac-4eff-830e-a8c93119521c.jpg" /></p><p>2) <img src="3-5300329\aade96df-e05f-48d3-9bfb-69306f68e4e1.jpg" /></p><p>3)<img src="3-5300329\c9b1d7aa-4ea1-4b51-8e25-730c4ea4a38f.jpg" />.</p><p>Let <img src="3-5300329\55db91a9-0049-4a02-a4da-7ba8ffa15402.jpg" /> and <img src="3-5300329\fc0bba6b-b87f-4e27-aed9-0e0b687bee7a.jpg" /> We note that<img src="3-5300329\e6fcf897-e824-451f-a973-aaa6ea9112b2.jpg" />, which combined with<img src="3-5300329\449921cd-5977-4912-ae64-dbe9d7ea1890.jpg" />, gives<img src="3-5300329\773037f0-d630-41c1-ba76-ad507bc219c1.jpg" />. Since <img src="3-5300329\bbe40deb-cd9f-4ff4-af2c-a5b4349a34a8.jpg" /> and<img src="3-5300329\d7c85e8c-bb49-49cf-b00a-302fd3246b36.jpg" />, we have <img src="3-5300329\37a7f70c-5fe8-4aed-83c5-033674e80ff9.jpg" /> Thus <img src="3-5300329\b65bcee3-c88b-4153-aedc-563f4a17c592.jpg" /> We can disregard<img src="3-5300329\ef3dcd71-1b5d-4d6e-bd33-45efd786a875.jpg" />. We will concentrate our work on the time interval<img src="3-5300329\e8dd7c92-5dd1-4ab2-9768-63c96c375e88.jpg" />, and we will use in the proof:</p><p>1) <img src="3-5300329\acf5a5af-3f4c-47bd-b6b1-003a000408c6.jpg" />we have <img src="3-5300329\52437c8a-cf53-4bed-b80d-8f34d3532fff.jpg" /></p><p>2) <img src="3-5300329\383dcd17-b47e-49c5-8cd0-092af4959e59.jpg" /></p><p>3) <img src="3-5300329\e97a08e9-ebde-479a-8490-1409bcca79e6.jpg" />and <img src="3-5300329\18375f06-2e7f-4c28-9605-220088a224c6.jpg" /></p><p>By the precompactness of K and (4.2) it follows that for any<img src="3-5300329\88449716-a1f6-495a-a5f0-ea864239bd4e.jpg" />, there exists<img src="3-5300329\47340827-6408-4dfc-bb42-5e915acb983f.jpg" />, such that for any <img src="3-5300329\aed41a00-7789-4b9c-b0d0-b0bda74e69bb.jpg" /></p><disp-formula id="scirp.27535-formula82097"><label>(4.5)</label><graphic position="anchor" xlink:href="3-5300329\c6ba6ed2-d4dd-4643-b7c2-c31eed42beff.jpg"  xlink:type="simple"/></disp-formula><p>We will select ε later; for <img src="3-5300329\b16b60c5-41ef-402a-9c40-ea5edc19008c.jpg" /> let <img src="3-5300329\1bf980e6-a5e8-4d12-aedc-68d019e88073.jpg" /> be such that <img src="3-5300329\7aca0216-20d8-4b16-9865-62103595b2c1.jpg" /> for<img src="3-5300329\85011813-6dc1-4b12-a976-8b3f78ffb095.jpg" />, <img src="3-5300329\ff4a6bac-7e4d-4657-a282-6a8a0bd78b98.jpg" />for</p><p><img src="3-5300329\8abd5450-5c81-48be-9f43-23d5221292d0.jpg" />, <img src="3-5300329\ecb90d1c-c8b0-4a56-9731-7bc1b0ba479e.jpg" />, <img src="3-5300329\72101184-6459-41c4-91bd-bd3d9dfa72ab.jpg" />and <img src="3-5300329\f8061d0c-287e-43e3-9d19-de1b005c30ee.jpg" /> for</p><p><img src="3-5300329\50906c36-95f9-4bb5-ad80-9257d27ffc86.jpg" />. Let <img src="3-5300329\bcd2c106-ae5b-4abb-b215-d95e71644964.jpg" /></p><p>Then <img src="3-5300329\9e362a3c-6e67-4e80-a84a-178075d1a573.jpg" /> for <img src="3-5300329\ea9602ed-e3b7-41d3-83d6-595564cc3706.jpg" /> and <img src="3-5300329\a3199b1f-e076-41cd-9ad2-4c8814cab912.jpg" /> For R &gt; 0, set <img src="3-5300329\996a8f3b-ad24-49ae-9f66-bf972783fadd.jpg" /> Let <img src="3-5300329\85693913-1a29-4626-87a1-f28f885cccb1.jpg" /> be the truncation center of mass given by</p><p><img src="3-5300329\9cc32d0f-71b3-4e50-9fda-599388047551.jpg" /></p><p>Then<img src="3-5300329\71e1f665-9384-4b71-902c-847eac94e213.jpg" />, where</p><p><img src="3-5300329\fba1cacb-da64-46ed-963c-8d654bf8fa51.jpg" /></p><p>Observe that <img src="3-5300329\b3ef6596-854e-45f6-b5fb-25ac01fc1ee1.jpg" /> for<img src="3-5300329\93b7cce5-2a84-4062-b3a9-1d05d1ea129c.jpg" />. By the zero momentum property</p><p><img src="3-5300329\af7ba84e-9e54-40a8-ad27-245f28d460f8.jpg" />.</p><p>Thus,</p><p><img src="3-5300329\35dcb2cb-645b-4e2b-b7ab-f53ab037869d.jpg" /></p><p>By Cauchy-Schwarz, we obtain;</p><disp-formula id="scirp.27535-formula82098"><label>(4.6)</label><graphic position="anchor" xlink:href="3-5300329\5d3b6205-f5ec-4214-8708-75fe2671556f.jpg"  xlink:type="simple"/></disp-formula><p>Set <img src="3-5300329\97e5d8e3-bf0e-4b04-bee6-259b32913e8f.jpg" /> Observe that for <img src="3-5300329\c5c778b5-8390-486e-b228-50b701c0f166.jpg" /> and</p><p><img src="3-5300329\b2c2a61d-2373-49c4-9b6b-51ef9f630194.jpg" />, we have<img src="3-5300329\37f297dd-d935-4ca8-84c8-7d976b44167e.jpg" />, and thus</p><p>(4.6), (4.5) give</p><disp-formula id="scirp.27535-formula82099"><label>(4.7)</label><graphic position="anchor" xlink:href="3-5300329\ee6e7e25-d819-4165-9a4d-1b5983306a82.jpg"  xlink:type="simple"/></disp-formula><p>We now obtain an upper bound for <img src="3-5300329\51c591f6-f774-401c-bff3-f31f911f2fda.jpg" /> and a lower bound for <img src="3-5300329\9b749957-d1c3-40ec-a0c1-4030289671ea.jpg" /></p><p><img src="3-5300329\31c2a869-210b-4b55-a785-17235d9e0824.jpg" /></p><p>Hence, by (4.5) we have</p><disp-formula id="scirp.27535-formula82100"><label>(4.8)</label><graphic position="anchor" xlink:href="3-5300329\2d2eefe2-846d-467d-ab1e-61e6eb0b2012.jpg"  xlink:type="simple"/></disp-formula><p>For<img src="3-5300329\3df979dc-3202-4526-beb7-cf971cff3b5f.jpg" />, we divide <img src="3-5300329\31882153-3487-462d-87f7-6b08f2c27729.jpg" /> as</p><p><img src="3-5300329\b9099a72-2a4e-4301-952e-4827ab9d5aa7.jpg" /></p><p>To deduce the expression for I, we observed that <img src="3-5300329\9d40ce79-7f8e-46eb-8fbd-3763a4d32f93.jpg" /></p><p>And use (4.5) to obtain <img src="3-5300329\f8151624-6d1b-4f30-9dd6-a39a9ba470b4.jpg" /></p><p>For II we first observe that,</p><p><img src="3-5300329\9cc56234-6ceb-4ec0-a08e-bed553002acd.jpg" /></p><p>and thus <img src="3-5300329\96f0bd9f-c400-45a9-a461-1081a47a1691.jpg" /></p><p>We rewrite II as</p><p><img src="3-5300329\544a6f3b-e960-4eb4-9879-7b307b1f2581.jpg" /></p><p>Trivially, <img src="3-5300329\ae20a493-2b6a-46d3-94a4-f14e9566361d.jpg" />and by (4.5)</p><p><img src="3-5300329\2c0377e1-9eff-4ed3-b3f6-4c2eaadb1adb.jpg" />.</p><p>Thus,</p><p><img src="3-5300329\f3a65ce3-6670-428c-a72f-9f8dde070850.jpg" /></p><p>Taking<img src="3-5300329\2916e695-060c-458b-8b14-8d147232efad.jpg" />, we can get</p><disp-formula id="scirp.27535-formula82101"><label>(4.9)</label><graphic position="anchor" xlink:href="3-5300329\a03a9f22-f0a9-4d11-af9e-667b92bf6655.jpg"  xlink:type="simple"/></disp-formula><p>Combining (4.7), (4.8), and (4.9), we have</p><p><img src="3-5300329\5abc1df3-de5b-4107-a96b-0a509e5bd644.jpg" /></p><p>Suppose <img src="3-5300329\74d02b6e-0a60-4a57-be31-61a60cd55f1e.jpg" /> and use <img src="3-5300329\1a653d6e-7024-4b25-948f-476a5a9b53ad.jpg" /> to obtain</p><p><img src="3-5300329\56293943-0bcd-440f-a9e4-8825a5f19a93.jpg" /></p><p>Since <img src="3-5300329\27db08b0-2d63-4292-9e3a-a5db64cb9244.jpg" /> we have</p><p><img src="3-5300329\44b4b27e-67d2-4d4d-a325-26c9b44292ba.jpg" /></p><p>(Assume<img src="3-5300329\af3b380d-70ba-4604-befb-4dad6f5d54ec.jpg" />) take<img src="3-5300329\be3c357f-1b01-4c09-b626-04cfafd222f0.jpg" />, as <img src="3-5300329\6332ba5d-53f0-446c-ac8e-8d04e1c61728.jpg" /> since <img src="3-5300329\8783e296-8381-429e-9da7-a6fbe87cba1b.jpg" /> we get a contradiction. <img src="3-5300329\672c0b36-3676-490b-9619-7f576d65bf64.jpg" /></p></sec><sec id="s4_2"><title>4.2. We Now Prove the Following Rigidity Theorem</title><p>Lemma 4.2. If (1.5) and (1.6) hold, then for all t</p><disp-formula id="scirp.27535-formula82102"><label>(4.10)</label><graphic position="anchor" xlink:href="3-5300329\6c99e4ce-26c1-4c6a-9078-674a7d92fe5a.jpg"  xlink:type="simple"/></disp-formula><p>where<img src="3-5300329\e08c4831-5d12-4059-9883-1363bfc11436.jpg" />. We have also the bound for all t;</p><disp-formula id="scirp.27535-formula82103"><label>(4.11)</label><graphic position="anchor" xlink:href="3-5300329\3a58cc96-4bba-47d6-b233-772b3dbaa22f.jpg"  xlink:type="simple"/></disp-formula><p>The hypothesis here is <img src="3-5300329\613de412-911d-42b1-92dd-55c59c627587.jpg" /> except if <img src="3-5300329\4e7e6aec-a3fd-4988-9c4b-41da314e6d7a.jpg" /> In fact, <img src="3-5300329\a56a87c1-d7e1-49c5-8b86-fe9a528b855f.jpg" /></p><p>Theorem 4.3. Assume <img src="3-5300329\cb8e2112-f3ed-4a0f-9363-a8a5890907c0.jpg" /> satisfies<img src="3-5300329\43460df0-c031-4e99-a0a1-6a0a301282a0.jpg" />,</p><disp-formula id="scirp.27535-formula82104"><label>(4.12)</label><graphic position="anchor" xlink:href="3-5300329\e7ef714f-1f08-4e06-be1d-8c51bd856860.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.27535-formula82105"><label>(4.13)</label><graphic position="anchor" xlink:href="3-5300329\38b8f50a-d0f5-42d6-9d5f-50afd5b6c23a.jpg"  xlink:type="simple"/></disp-formula><p>Let u be the global H<sup>1</sup> solution of (1.1) with initial data u<sub>0</sub> and assume that <img src="3-5300329\b2b50109-b0f7-4904-8472-68c9ecd278e9.jpg" /> is precompact in H<sup>1</sup>. Then <img src="3-5300329\e936668c-22cd-4b01-8cec-3014cec6c304.jpg" /> .</p><p>Proof. Let <img src="3-5300329\c33e3032-d169-4e78-b006-fc9a770eb80b.jpg" /> be redial with</p><p><img src="3-5300329\a6df68ad-b979-4803-9ada-280e1a5b6e9e.jpg" />.</p><p>For R &gt; 0, we define</p><p><img src="3-5300329\51c23709-a052-4910-ab67-734376f1ca7d.jpg" /></p><p>Then</p><p><img src="3-5300329\ca1a5f40-5886-4856-a19b-2eb67b52a15a.jpg" /></p><p>By the H&#246;lder inequality:</p><disp-formula id="scirp.27535-formula82106"><label>(4.14)</label><graphic position="anchor" xlink:href="3-5300329\1adefa42-bac1-4ca1-bec5-8bc67500ed98.jpg"  xlink:type="simple"/></disp-formula><p>By calculation, we have the local Virial identity</p><p><img src="3-5300329\ab257db5-0347-4037-bfcc-16cc02469f9b.jpg" /></p><p>Since <img src="3-5300329\90a9616b-b411-4eb4-be95-14c3800081bc.jpg" /> is radial we have</p><disp-formula id="scirp.27535-formula82107"><label>(4.15)</label><graphic position="anchor" xlink:href="3-5300329\5601e95c-77eb-421a-8038-f147059fa4f7.jpg"  xlink:type="simple"/></disp-formula><p>where</p><p><img src="3-5300329\18b7dcc3-cabb-44ac-ab7a-7c6582567292.jpg" /></p><p>Thus, we obtain</p><disp-formula id="scirp.27535-formula82108"><label>(4.16)</label><graphic position="anchor" xlink:href="3-5300329\f6cd58e0-21e6-4c12-8d01-ee901a42a2d5.jpg"  xlink:type="simple"/></disp-formula><p>Now discuss <img src="3-5300329\c8aaf56a-9b19-4587-8c1f-c0a94fbf05be.jpg" /> for R chosen appropriate large and selection time interval <img src="3-5300329\02bffc0b-d25f-40ed-99a7-a92b7fe4cfa6.jpg" /> where<img src="3-5300329\22533bf3-e3a4-4eb6-9705-3a982f2c9384.jpg" />. By (4.15) and (4.11) we have</p><disp-formula id="scirp.27535-formula82109"><label>(4.17)</label><graphic position="anchor" xlink:href="3-5300329\c222a8e2-b3c8-4a54-b860-6874b086b8bd.jpg"  xlink:type="simple"/></disp-formula><p>Set <img src="3-5300329\013b0b14-396c-40ad-aba4-e391daf423ae.jpg" /> in (4.2), <img src="3-5300329\9a15c9e7-f89f-413d-bf52-48035970c9bb.jpg" />, such that <img src="3-5300329\c76e8372-bcff-4385-add1-21199db11dc5.jpg" /></p><disp-formula id="scirp.27535-formula82110"><label>(4.18)</label><graphic position="anchor" xlink:href="3-5300329\af5e52ce-0a1b-40e4-9552-d9458fcefb1c.jpg"  xlink:type="simple"/></disp-formula><p>Choosing <img src="3-5300329\ed15a140-c382-45b2-a4ae-eb75c00c792b.jpg" /> Then (4.16), (4.17) and</p><p>(4.18) imply that for all<img src="3-5300329\627eda0a-96c8-47e5-879c-ecf7629fc728.jpg" />,</p><disp-formula id="scirp.27535-formula82111"><label>(4.19)</label><graphic position="anchor" xlink:href="3-5300329\147dcc77-757a-4eca-997c-1e52bc9e1e56.jpg"  xlink:type="simple"/></disp-formula><p>By Lemma 4.1, there exists <img src="3-5300329\bea1bdd1-dba1-4b37-9acc-0866d7fdec5f.jpg" /> such that for all <img src="3-5300329\038327de-a69e-49dd-9520-9be2b42c087a.jpg" /> we have <img src="3-5300329\2335f4f7-6888-49d9-a706-9323f2f91f85.jpg" /> with <img src="3-5300329\fa165d27-3d45-4090-8924-0634a5fcd81d.jpg" /> By taking R =<img src="3-5300329\30f26db9-3f5a-4448-9c02-b52c79708475.jpg" />, we obtain that (4.18) holds for all <img src="3-5300329\9b515fa3-2323-4e57-a86f-15f5e951c181.jpg" />. Integrating (4.19) over <img src="3-5300329\72227fab-0a17-44b7-943c-48a479394ede.jpg" /> we obtain</p><disp-formula id="scirp.27535-formula82112"><label>(4.20)</label><graphic position="anchor" xlink:href="3-5300329\591a4e8a-1db2-48f7-96f7-808417db3e33.jpg"  xlink:type="simple"/></disp-formula><p>On the other hand, for all<img src="3-5300329\5a02fe64-692d-4e79-a0b2-22b0ef233320.jpg" />, by (4.10) and (4.14), we have</p><disp-formula id="scirp.27535-formula82113"><label>(4.21)</label><graphic position="anchor" xlink:href="3-5300329\73ad4884-9ea3-4350-abd5-a313616f9143.jpg"  xlink:type="simple"/></disp-formula><p>Combining (4.20) and (4. 21), we obtained</p><p><img src="3-5300329\94d5750f-ae5a-4821-bd57-85f67b2735cc.jpg" /></p><p>It is important to mention that <img src="3-5300329\c3432f3d-596d-4051-9bda-71ab208cc211.jpg" /> and <img src="3-5300329\b476e505-0070-43f7-a7c3-f74dc7b82682.jpg" /> are constant depending only on<img src="3-5300329\2e408636-1978-4913-abc1-0142bd5dd882.jpg" />, and<img src="3-5300329\b4901d3f-9a15-4df9-b9ff-638b182855bb.jpg" />.</p><p>Putting <img src="3-5300329\bddd0d12-640f-4de3-9f4e-c7ef897c874c.jpg" /> and setting<img src="3-5300329\5355437f-6e00-4734-a7a3-c847bd500d4e.jpg" />, we obtain a contradiction except if<img src="3-5300329\a3883dad-ca1b-4ce0-9473-79e57e7ffc9f.jpg" />, which implies <img src="3-5300329\1a9e3b8b-6a2f-43f0-a8b7-a7b9097f21cc.jpg" /> <img src="3-5300329\12d70204-ed87-4b58-86b7-378ea5c5c09b.jpg" /></p></sec></sec><sec id="s5"><title>REFERENCES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.27535-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">T T. 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