<?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.2013.35070</article-id><article-id pub-id-type="publisher-id">APM-36305</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>
 
 
  The Mass-Critical for the Nonlinear Schr&#246;dinger Equation in &lt;i&gt;d&lt;/i&gt; = 2
 
</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"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><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</email></corresp></author-notes><pub-date pub-type="epub"><day>23</day><month>07</month><year>2013</year></pub-date><volume>03</volume><issue>05</issue><fpage>482</fpage><lpage>490</lpage><history><date date-type="received"><day>February</day>	<month>13,</month>	<year>2013</year></date><date date-type="rev-recd"><day>March</day>	<month>16,</month>	<year>2013</year>	</date><date date-type="accepted"><day>April</day>	<month>19,</month>	<year>2013</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p><html>
 <head></head>
 
   This paper studies the global behavior defocusing nonlinear Schrodinger equation in dimension d = 2, and we will discuss the case <img src="Edit_67a41bb7-8e51-4eca-835d-07fdc786964f.bmp" width="47" height="20" alt="" />. This means that the solutions <img src="Edit_864e307d-5151-45a5-bc21-b4289b824408.bmp" width="176" height="20" alt="" />, and called critical solution. We show that u scatters forward and backward to a free solution and the solution is globally well posed. 
 
</html></p></abstract><kwd-group><kwd>NLS; Well Posed</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>We consider the Cauchy problem for the nonlinear Schr&#246;- dinger equation in dimension d = 2.</p><disp-formula id="scirp.36305-formula143631"><label>(1.1)</label><graphic position="anchor" xlink:href="8-5300438\5cdbf4c3-2bc1-4dd1-b9bf-d6741f8c10c0.jpg"  xlink:type="simple"/></disp-formula><p>where<img src="8-5300438\e5bf77cb-c101-4488-a746-72069d1a60a1.jpg" />, <img src="8-5300438\083ddba2-71c4-44bd-b75d-b03f6f9ad4d4.jpg" />, and<img src="8-5300438\5d24bc1e-41c4-4088-98bd-001347fde54e.jpg" />, When <img src="8-5300438\9b16b578-8def-4064-a7a0-9bcfab32fa57.jpg" /> (1.1) is called defocusing when <img src="8-5300438\40f11007-569c-473e-9db9-449c06def000.jpg" /> (1.1) is called focusing. In this paper we discuss the case when <img src="8-5300438\3e840547-8515-4d06-a616-68b347397192.jpg" /> and <img src="8-5300438\b68f177b-d569-48b7-b043-f2d17c860482.jpg" /> (defocusing case).</p><p>If <img src="8-5300438\ff512230-b970-49d6-b265-dc5273994ec5.jpg" /> is a solution to (1.1) on a time interval <img src="8-5300438\18b2538c-5279-417a-8db9-ae27ea27bd50.jpg" /> then</p><disp-formula id="scirp.36305-formula143632"><label>(1.2)</label><graphic position="anchor" xlink:href="8-5300438\0ed85c7c-24f9-4506-a02d-b8d78b7b57c5.jpg"  xlink:type="simple"/></disp-formula><p>is a solution to (1.1) on <img src="8-5300438\f2e5354c-4378-4432-88fb-c4c08b97659e.jpg" /> with<img src="8-5300438\29398447-c2c3-47ad-a69c-9f0948e508c6.jpg" />.</p><p>This scaling saves the <img src="8-5300438\640f106e-c0b6-4107-b5e8-5c5009391528.jpg" /> norm of u,</p><disp-formula id="scirp.36305-formula143633"><label>(1.3)</label><graphic position="anchor" xlink:href="8-5300438\bafd31b7-950c-4ce6-867e-0e25f58021e0.jpg"  xlink:type="simple"/></disp-formula><p>Thus (1.1) under previous hypotheses is called L<sup>2</sup>-critical or mass critical.</p><p>Proposition 1.1. Suppose that <img src="8-5300438\be1673c5-8426-433e-998e-937d42096720.jpg" /> and <img src="8-5300438\53b0791d-82a8-4b5f-873a-e9714c63cb15.jpg" /></p><p>then, for any initial data<img src="8-5300438\2909d051-2939-472c-9f55-ef583184c5c9.jpg" />, there exist <img src="8-5300438\10ed4220-387c-4303-a20f-d6bc0fc58278.jpg" /> such that there exists a unique solution</p><p><img src="8-5300438\189458cc-cfb9-4cbd-9abe-907f81cf713d.jpg" /></p><p>of the nonlinear Schr&#246;dinger Equation (1.1). If <img src="8-5300438\663e01dc-b81b-44ad-9acb-63395f2cbb6e.jpg" /> then <img src="8-5300438\3e34dd3d-0381-4ac7-bd50-d5cd04b46769.jpg" /> for some non-increasing, and if <img src="8-5300438\77602827-d6f6-4194-9507-2b0a1350b3b8.jpg" /> is sufficiently small u exists globally.</p><p>In this paper we will discuss the case, <img src="8-5300438\8de3af0d-5d80-4c99-bac8-55530138050b.jpg" /></p><p>This means that a solution u</p><p><img src="8-5300438\e6369e28-4fe0-4d77-a673-29517c4317e2.jpg" />and called critical solution.</p><p>Definition 1.1. Let<img src="8-5300438\f148e101-cf62-4a28-80c1-4b7fe8d56059.jpg" />, <img src="8-5300438\0b2a143d-546f-400d-8c9f-3f2215be0d79.jpg" />is a solution to (1.1) if for any compact</p><p><img src="8-5300438\3e94af0d-19fa-463d-bed7-67975827e86b.jpg" /></p><p>and for all <img src="8-5300438\69be5a3c-30cd-42c5-8154-3c8d01e15364.jpg" /></p><disp-formula id="scirp.36305-formula143634"><label>(1.4)</label><graphic position="anchor" xlink:href="8-5300438\cf718205-e39b-4b61-8570-b5e3071866dc.jpg"  xlink:type="simple"/></disp-formula><p>The space <img src="8-5300438\e8f7153a-e37c-40cc-9db1-b6ed357f4c3f.jpg" /> caused from strichartz estimates. This norm is invariant under the scaling (1.2).</p><p>Definition 1.2. If there exist <img src="8-5300438\f1fbfd70-21ad-441c-b713-08754e9b3768.jpg" /> a solution u to (1.1) defined on <img src="8-5300438\8ed19cde-b735-421c-adb9-175005390d96.jpg" /> blows up forward in time, such that</p><disp-formula id="scirp.36305-formula143635"><label>(1.5)</label><graphic position="anchor" xlink:href="8-5300438\c8711173-bf90-492e-bf1d-cd64b828adb4.jpg"  xlink:type="simple"/></disp-formula><p>And u blows up backward in time, such that</p><disp-formula id="scirp.36305-formula143636"><label>(1.6)</label><graphic position="anchor" xlink:href="8-5300438\611eaf9a-b01f-418c-9a38-be164cce7566.jpg"  xlink:type="simple"/></disp-formula><p>Definition 1.3. If there exist <img src="8-5300438\f8bb603b-8495-4e90-836a-70dd4d86c0ab.jpg" /> we say that a solution u to (1.1) scatter forward in time such that,</p><disp-formula id="scirp.36305-formula143637"><label>(1.7)</label><graphic position="anchor" xlink:href="8-5300438\2c3a1218-e6bb-4f9f-b494-2676759ba8a0.jpg"  xlink:type="simple"/></disp-formula><p>A solution is said to scatter backward in time if there exist <img src="8-5300438\c77d4c1c-016f-4253-ae91-6f86f6d9a4d7.jpg" /></p><p>Such that,</p><disp-formula id="scirp.36305-formula143638"><label>(1.8)</label><graphic position="anchor" xlink:href="8-5300438\feb810d9-455b-4feb-8dcb-5990e7f51d7e.jpg"  xlink:type="simple"/></disp-formula><p>We note that the Equation (1.1) has preserved quantities, the mass</p><disp-formula id="scirp.36305-formula143639"><label>(1.9)</label><graphic position="anchor" xlink:href="8-5300438\2c5114bb-1feb-4c93-bbbc-526e9fe64043.jpg"  xlink:type="simple"/></disp-formula><p>And energy</p><disp-formula id="scirp.36305-formula143640"><label>(1.10)</label><graphic position="anchor" xlink:href="8-5300438\918e80e8-31af-4b33-b736-addfc09da321.jpg"  xlink:type="simple"/></disp-formula><p>For more see [<xref ref-type="bibr" rid="scirp.36305-ref1">1</xref>].</p><p>Proposition 1.2. let p be the <img src="8-5300438\db13884a-0ec4-4fae-9e2c-2370eb7dc394.jpg" />-critical exponent</p><p><img src="8-5300438\b131cf76-813e-4a5c-83a4-80d49e7e16dc.jpg" />, then the NLS (1.1) is locally well posed in</p><p><img src="8-5300438\12b9ed53-c3a8-44f4-a788-6845503830ba.jpg" />in the critical case. More precisely, given any<img src="8-5300438\6c0ff84f-78ca-4a14-b8ac-23a42a0b0103.jpg" />, there exists <img src="8-5300438\0be28169-85e6-4cda-a9bf-600fe8ec50b7.jpg" /> such that whenever <img src="8-5300438\624dc6fc-754c-4ec5-8501-ee3bea08e00d.jpg" /> has norm at most R, and K is a time interval containing 0 such that</p><p><img src="8-5300438\cfba2434-d446-403b-9788-c23ca757a863.jpg" /></p><p>Then for any u<sub>0</sub> in the ball</p><p><img src="8-5300438\ebde2db2-e5d0-4638-9585-573aeee5ab91.jpg" /></p><p>there exists a unique strong <img src="8-5300438\511112a8-818e-41c0-a0ab-7f054e477d21.jpg" /> solution <img src="8-5300438\920e6560-80ec-451d-b2af-0bd8ac4f2403.jpg" /> to (1.1), and moreover the map<img src="8-5300438\8fc41527-9454-4f22-b634-4b5d69f8dc40.jpg" />, is Lipschitz from B to<img src="8-5300438\268b3a6e-adf6-4fa2-836a-3266c32c972e.jpg" />, where <img src="8-5300438\9099041b-7e77-4b52-bc51-d956b85f11f7.jpg" /> defined in Equation (2.5).</p><p>Proposition 1.3. let K be a time interval containing <img src="8-5300438\201014d0-0b7a-4d2a-b0e0-b2fe7e69af1e.jpg" /> and let <img src="8-5300438\6bc5e8ff-fa5d-4145-a104-a2a2e84163bb.jpg" /> be two classical solutions to (1.1) with same initial datum u<sub>0</sub> for some fixed μ and p, assume also that we have the temperate decay hypothesis <img src="8-5300438\8f0088d2-de6e-48af-84cc-fa641acb7f07.jpg" /> for q = 2, ∞. Then<img src="8-5300438\ebf06bc8-856f-4670-899e-97848eafe67d.jpg" />.</p><p>Proposition 1.4. Let<img src="8-5300438\0af80bed-ee32-4e5c-815e-30b863fc831f.jpg" />, given <img src="8-5300438\bebef8f8-b776-4209-af53-0456a8341d0c.jpg" /> there exists a maximal lifespan solution u to (1.1) define on<img src="8-5300438\35d0c484-cba5-4391-a38e-50fb1d12c81c.jpg" />, with<img src="8-5300438\2746f1aa-eb40-496c-bf0f-e22adc3b15be.jpg" />. Furthermore1) k is an open neighborhood of<img src="8-5300438\05dd9668-552e-4111-9869-f3c50bc601e0.jpg" />.</p><p>2) We say u is a blow up in the contrast direction If <img src="8-5300438\043aef21-6325-4f98-991a-fe5c461534c0.jpg" /> or <img src="8-5300438\c1aa54db-fdde-4707-b7e3-e52904631cab.jpg" /> is finite.</p><p>3) If we have compact time intervals for bounded sets of initial data, then the map that takes initial data to the corresponding solution is uniformly continuous in these intervals.</p><p>4) We say that u scatters forward to a free solution, if <img src="8-5300438\0386fb71-326e-449d-96f0-2de6b30ac9e0.jpg" /> and u does not blow up forward in time. And we say that u scatters backward to a free solution, if <img src="8-5300438\20d44c03-0dc8-4cb4-ae76-32b91b892c6c.jpg" /> and u does not blow up backward in time.</p><p>To Proof: see [1-3].</p></sec><sec id="s2"><title>2. Strichartz Estimates</title><p>In this section we discuss some notation and Strichartz estimates for critical NLS (1.1) and we turn to prove Propositions 1.1 and 1.3.</p><sec id="s2_1"><title>2.1. Some Notation</title><p>If X, Y are nonnegative quantities, we use <img src="8-5300438\1e7d9f19-e55a-457b-927a-637a613e39f8.jpg" /> or<img src="8-5300438\b69ba5c9-6b70-442e-ae43-76d290e3348f.jpg" />, to denote the estimate <img src="8-5300438\f073b155-b86c-45bf-ad9a-43badf388b16.jpg" /> for some c and <img src="8-5300438\b1be9efa-780f-433b-81c9-752446be99be.jpg" /> to denote the estimate <img src="8-5300438\7c19a29e-31d2-49cf-a78d-fd8e051dafca.jpg" /></p><p>We defined the Fourier transform on <img src="8-5300438\c8ae2aca-3c40-41d3-8b42-54178811a93e.jpg" /> by</p><p><img src="8-5300438\002e2357-b513-45dd-a875-2ed19381d87d.jpg" /></p><p>We use <img src="8-5300438\ba5b2031-572e-4b12-898d-0263c849767d.jpg" /> to denote the Banach space for any space time slab <img src="8-5300438\b934cb45-c778-4133-84e5-c231da17229a.jpg" /> of function <img src="8-5300438\d4647c97-daff-4dbb-ad0a-07a636ad5b4a.jpg" /> with norm is</p><p><img src="8-5300438\243a8dce-ca46-417f-9766-de40fe64c8cd.jpg" /></p><p>With the usual amendments when q or r is equal to infinity. When <img src="8-5300438\88a8617a-b67f-4dd3-9a16-f91e09b74c43.jpg" /> we cut short <img src="8-5300438\183282b1-7125-4ec2-9737-f29d2d01d701.jpg" /> as<img src="8-5300438\2b5fd239-1f4e-41d3-b061-471ddf356a2b.jpg" />.</p><p>Defined the fractional differentiation operators<img src="8-5300438\31703ef5-1ca9-4f71-b516-20a28441c203.jpg" />, <img src="8-5300438\8127693e-de49-42bf-bda3-b19c1e162d1d.jpg" />by</p><p><img src="8-5300438\b85733cc-3a37-4faf-8925-1d025e18f1d5.jpg" /><img src="8-5300438\b86fa98a-9a6b-4f73-9555-ee186786f37b.jpg" /></p><p>where<img src="8-5300438\308b9163-86aa-4a87-952e-5ccdca3f7bad.jpg" />, specially, we will use <img src="8-5300438\48c549d0-68b3-4864-8765-e100505cdd1b.jpg" /> to signify the spatial gradient <img src="8-5300438\2f1632ef-476e-4404-b002-bc2f586865cc.jpg" /> and define the Sobolev norms as</p><p><img src="8-5300438\e679582f-8895-45bf-a103-6a3c96efa4ae.jpg" /></p><p><img src="8-5300438\47c4032c-596b-4c1b-b140-9563167b8ae5.jpg" /></p><p>Let <img src="8-5300438\81fe64b1-9ddf-4524-8786-e91b5fe9f83d.jpg" /> be the free Schr&#246;dinger propagator; in terms of the Fourier transform, this is given by,</p><p><img src="8-5300438\3e4182a5-c652-4c8f-a351-ecf0efb5c3c3.jpg" />.</p><p>A Gagliardo-Nirenberg type inequality for Schr&#246;dinger equation the generator of the spurious conformal transformation <img src="8-5300438\70e28163-7f29-4293-819a-410f5f8cf861.jpg" /> plays the role of the partial differentiation.</p></sec><sec id="s2_2"><title>2.2. Strichartz Estimates</title><p>Let <img src="8-5300438\c602901b-5353-4d83-9fc5-14285043c903.jpg" /> be the free Schr&#246;dinger evolution, from the explicit formula</p><disp-formula id="scirp.36305-formula143641"><label>(2.1)</label><graphic position="anchor" xlink:href="8-5300438\b044b7c6-1c4a-4bef-9e89-8169ec28ac1d.jpg"  xlink:type="simple"/></disp-formula><p>Specially, as the free propagator saves the <img src="8-5300438\9af82368-44b2-44aa-b759-d48a614919f3.jpg" />-norm,</p><p><img src="8-5300438\28bd2c9b-4afa-493a-8cb8-ee19ca393006.jpg" /></p><p>For all <img src="8-5300438\0dd5e162-013d-40a9-8818-bf1b8881f1b2.jpg" /> and<img src="8-5300438\ab8a5da8-e6a7-4ad0-82ca-89ff555f95d4.jpg" />, where <img src="8-5300438\8a9abd6d-5509-4f7e-b03b-6b85fa6b96e6.jpg" /></p><p>Proposition 2.1. There holds that</p><disp-formula id="scirp.36305-formula143642"><label>(2.2)</label><graphic position="anchor" xlink:href="8-5300438\01cbdfd9-acc5-4aab-9820-f71a2301fefb.jpg"  xlink:type="simple"/></disp-formula><p>In fact, this follows directly from the formula (2.1).</p><p>Definition 2.1. Define an admissible pair to be pair</p><p><img src="8-5300438\b5682abc-2573-43df-af35-bb78802284ec.jpg" />with<img src="8-5300438\4447c071-bde5-4de2-9a95-920e8f435d4d.jpg" />, <img src="8-5300438\c7e82673-75b7-475d-89a8-d641a74049b3.jpg" />, With <img src="8-5300438\e7fca5de-5ed2-4a50-b003-36f5c1c9e2dc.jpg" /></p><p>Theorem 2.2. If <img src="8-5300438\5ddf2f2f-2c5b-4143-8508-f0500354a0e0.jpg" /> solves the initial value problem</p><p><img src="8-5300438\6c2874b9-93ab-48ea-b506-876f8a081678.jpg" /></p><p><img src="8-5300438\d05e3af0-f491-4e93-b18d-f66a2ece35c8.jpg" />On an interval K, then</p><disp-formula id="scirp.36305-formula143643"><label>(2.3)</label><graphic position="anchor" xlink:href="8-5300438\bf0cb797-8772-4d96-93df-dd03db68de00.jpg"  xlink:type="simple"/></disp-formula><p>For all admissible pairs<img src="8-5300438\26b7b601-9301-4cf8-b342-59747707a213.jpg" />,<img src="8-5300438\a7d7a9b3-f47c-4df1-b0f5-0606e9a10058.jpg" />. <img src="8-5300438\ac1230e1-2126-4007-886a-6b6fe8afb08c.jpg" />denotes the Lebesgue dual<img src="8-5300438\deba5416-6c91-4927-9d75-476e4c946add.jpg" />.</p><p>To prove: see [4,5].</p><p>Definition 2.2. Define the norm</p><disp-formula id="scirp.36305-formula143644"><label>(2.4)</label><graphic position="anchor" xlink:href="8-5300438\03db0875-c566-4012-a2d3-75b8200d2edb.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.36305-formula143645"><label>(2.5)</label><graphic position="anchor" xlink:href="8-5300438\1bfe9715-b711-439d-acdb-0587e7d2fd7b.jpg"  xlink:type="simple"/></disp-formula><p>We also define the space <img src="8-5300438\e101d2cf-e184-48a2-9dc7-7a82976ee4b4.jpg" /> to be the space dual to <img src="8-5300438\a41e214d-37fb-4415-9acc-fc7b653a8564.jpg" /> with suitable norm. By theorem.2.2,</p><disp-formula id="scirp.36305-formula143646"><label>(2.6)</label><graphic position="anchor" xlink:href="8-5300438\d3048e9d-ad16-44ab-9979-73b379facf62.jpg"  xlink:type="simple"/></disp-formula><p>Theorem 2.3. If <img src="8-5300438\abfca99f-7727-47ec-b39d-d60e31266fa9.jpg" /> is small, then (1.1) is globally well posed, for more see [6,7].</p><p>Proof: by (2.3) and (2.6)</p><disp-formula id="scirp.36305-formula143647"><label>(2.7)</label><graphic position="anchor" xlink:href="8-5300438\0bdcfa6c-1df2-401a-be11-bd9a8b381c73.jpg"  xlink:type="simple"/></disp-formula><p>If <img src="8-5300438\7f86c0d0-0c6d-459e-a201-2618ce6bdebe.jpg" /> is small enough and by the continuity method, then we have global well-posedness. Furthermore, for any <img src="8-5300438\232fb9dd-5731-4795-b1d4-c44bb9d16576.jpg" /> there exist <img src="8-5300438\518e54c8-ab3a-4513-9d0c-e2efe7b96307.jpg" /> such that</p><p><img src="8-5300438\90a38914-fb4b-4ddf-a572-9d28481beed3.jpg" /></p><p>Then</p><disp-formula id="scirp.36305-formula143648"><label>(2.8)</label><graphic position="anchor" xlink:href="8-5300438\73ec2f47-324d-4ab0-b208-f31c202adec5.jpg"  xlink:type="simple"/></disp-formula><p>So by (2.6), when <img src="8-5300438\36f727fc-d63d-431e-93df-816100f9f98c.jpg" /></p><disp-formula id="scirp.36305-formula143649"><label>(2.9)</label><graphic position="anchor" xlink:href="8-5300438\2da1d00b-a842-45fd-9c28-458a60a981d1.jpg"  xlink:type="simple"/></disp-formula><p>Thus, the limit</p><disp-formula id="scirp.36305-formula143650"><label>(2.10)</label><graphic position="anchor" xlink:href="8-5300438\0d74e2a3-ce82-419d-8a5d-ade7f1ab6525.jpg"  xlink:type="simple"/></disp-formula><p>Exists, and,</p><disp-formula id="scirp.36305-formula143651"><label>(2.11)</label><graphic position="anchor" xlink:href="8-5300438\49ce3483-4f34-41be-b503-890346e634a5.jpg"  xlink:type="simple"/></disp-formula><p>A conformable argument can be made for <img src="8-5300438\88c82911-8dfc-4fa4-83cc-7959b9d23fa4.jpg" /></p><p>indeed, if<img src="8-5300438\390a7725-8318-409a-8025-3af10478523e.jpg" />, then <img src="8-5300438\4e3ae3f5-506c-4355-bddd-be71cb8fe69c.jpg" /> can be division into <img src="8-5300438\75c5f2ac-cec4-4aa2-b051-2eebdb401ae0.jpg" /> subintervals K with <img src="8-5300438\a479c349-69ca-4b62-b410-0e3e32fa01d7.jpg" /></p><p>on each subinterval. Using the Duhamel formula on each interval individually, we obtain global well-posedness and scattering.&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160; <img src="8-5300438\0ba975f2-aa5c-4e7b-b069-f3ef04ec1c09.jpg" /></p><p>Now we return to prove Proposition 1.1 and Proposition 1.3.</p><sec id="s2_2_1"><title>Proof proposition 1.1:</title><p>We suppose in what follows that<img src="8-5300438\e4a89491-c861-413f-ac3c-fa83336c2262.jpg" />. Let</p><p><img src="8-5300438\1e4a43b9-fe08-47ea-b4ae-0974972b3cb3.jpg" />and for some <img src="8-5300438\c04dab41-7170-4fa6-925a-e1d9a3ec8a30.jpg" /> to be chosen,<img src="8-5300438\83043dc9-6f08-4a46-b0dc-903847ae780f.jpg" /> be such that</p><disp-formula id="scirp.36305-formula143652"><label>(2.12)</label><graphic position="anchor" xlink:href="8-5300438\6333983b-f491-4a8e-a4c1-0ef90bc82ae8.jpg"  xlink:type="simple"/></disp-formula><p>We deem the space</p><p><img src="8-5300438\e4d45141-3526-4c48-9e72-2c13567c2df1.jpg" /></p><p>And the mapping,</p><disp-formula id="scirp.36305-formula143653"><label>(2.13)</label><graphic position="anchor" xlink:href="8-5300438\da6dea2a-548b-4707-844e-d9c4eac4b8a9.jpg"  xlink:type="simple"/></disp-formula><p>We want to prove that the δ small adequate, <img src="8-5300438\fb035264-a008-4ec8-848d-0ea1e0a65362.jpg" /> is contraction. We use first Strichartz estimates, to compute that</p><p><img src="8-5300438\9a264265-dc42-43c1-a824-fac1f38560d5.jpg" /></p><p>where <img src="8-5300438\9d3689f3-9997-460b-8fd9-59608d7fd289.jpg" /></p><p>Then, distinctly,</p><p><img src="8-5300438\c8073a14-ce4d-41ba-a8b3-199a10cb02b1.jpg" /></p><p><img src="8-5300438\86c03ae6-48ed-42da-9f4b-d526e86f68d0.jpg" /></p><p>So that for <img src="8-5300438\9e1dff8f-a570-457b-a14e-7eb26e7465db.jpg" /> is small enough, <img src="8-5300438\06040e96-ca4d-4590-abf3-76c3b202061b.jpg" />is settled under<img src="8-5300438\d2a394e7-6788-4082-8cdb-22d5d8585dd6.jpg" />. In addition,</p><p><img src="8-5300438\5a06c19e-ef88-443b-b2bd-2c4ec69973e5.jpg" /></p><p>Again, decreasing may be<img src="8-5300438\74fda071-14ff-4c32-b4e7-3f94e553c672.jpg" />, we get a contraction.</p><p>If<img src="8-5300438\13923781-569b-4cfc-9a96-9510119ded7b.jpg" />, then<img src="8-5300438\f3b734c7-5761-4f75-8501-b5a8543c85ba.jpg" />, and from Strichartz estimateswe see that if <img src="8-5300438\97fec1fb-544f-4809-a078-fa1c43d65b6a.jpg" /> is small enough, then (2.12) is satisfied for <img src="8-5300438\72601652-1561-4a18-8a9e-7c5d3d509704.jpg" /> &#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;<img src="8-5300438\bafc47c0-c873-42c3-b925-ce3a7391fe4c.jpg" /></p><p>Proof Proposition 1.3: By time translation symmetry we can take<img src="8-5300438\845233c6-3368-42e0-bc90-96dc9b9dc30d.jpg" />. By time reversal symmetry we may assume that K lies in the upper time axis<img src="8-5300438\099aeedc-3107-4f83-a685-100d104439d9.jpg" />. Let<img src="8-5300438\dfc123ec-e5a2-4c66-9a6e-c9615a7912d3.jpg" />, and then, <img src="8-5300438\86970a9e-b0db-4d4c-bf86-2c248e1a05e9.jpg" />, <img src="8-5300438\97d190be-6b06-45d2-8e5d-f9ad555c0f78.jpg" />and v obey the variance equation</p><p><img src="8-5300438\01ef0d74-01f2-4fab-bcc2-1b38ccac10e9.jpg" /></p><p>Since v and <img src="8-5300438\c3350dec-34aa-4f1b-b950-e264927bf59c.jpg" /> lies in the <img src="8-5300438\0f6dfca0-6d4b-4f5c-9d6b-a483622ad558.jpg" /> we may calling Duhamel’s and conclude</p><p><img src="8-5300438\6e5c93c2-32bb-4d0c-9849-5263335e1b95.jpg" /></p><p>for all. By Minkowski’s inequality, and the unitarity of<img src="8-5300438\a0d62190-1776-4e59-a6a7-5c99fa4dd339.jpg" />, conclude that,</p><p><img src="8-5300438\56a3973d-0aa4-454f-bbc3-97326c2fedf1.jpg" /></p><p>Since u and v are in<img src="8-5300438\96d0d8b7-95af-43df-8108-560db493c363.jpg" />, and the function <img src="8-5300438\c50a431e-5f75-4872-8f4a-1cd610dc3a72.jpg" /> is locally Lipcshitz, we have the bound</p><p><img src="8-5300438\b66b8af2-8174-4ea1-a924-d1ad374c0e77.jpg" /></p><p>Apply Gronwall’s inequality to conclude that</p><p><img src="8-5300438\d37b2f85-c9d3-43b8-b495-dc0c6c429bb0.jpg" />for all <img src="8-5300438\593cc2a6-52ce-4cc3-bc09-77a75c6dd808.jpg" /> and hence<img src="8-5300438\0d9606a1-cbb2-43fc-9d64-3b7ce67d2d06.jpg" />. &#160;&#160;<img src="8-5300438\297b3f95-e629-4df5-80d4-85a93e642348.jpg" /></p></sec></sec></sec><sec id="s3"><title>3. Decay Estimates</title><p>Consider the defocusing nonlinear Schr&#246;dinger Equation (1.1), in<img src="8-5300438\0a62f8f6-a435-4b26-ae59-bdb6cb448f62.jpg" />, where <img src="8-5300438\6575ab41-f9d9-4500-87b3-d956d3296a00.jpg" /> and<img src="8-5300438\ec32944e-2163-4bd7-9910-fabefab8aa70.jpg" />, for<img src="8-5300438\a1ba0786-e9d5-4c52-96c7-cb6c336a88d9.jpg" />. We suppose that at <img src="8-5300438\6697874e-e4e6-4adb-a695-5ecbab64284d.jpg" /></p><disp-formula id="scirp.36305-formula143654"><label>(3.1)</label><graphic position="anchor" xlink:href="8-5300438\6e039eb4-744c-4452-8b34-a34b7732ec57.jpg"  xlink:type="simple"/></disp-formula><p>First we have the following result.</p><p>Theorem 3.1. Suppose that<img src="8-5300438\4428fb38-7f6d-4871-a735-faa3f913773e.jpg" />, if <img src="8-5300438\fb48365a-a808-4ad7-9d2c-531dd620334d.jpg" /> and let u be a solution to (1.1), identical to an initial data</p><p><img src="8-5300438\55790884-037c-4bb7-8b41-a20e2da26e12.jpg" />such that<img src="8-5300438\f89bf3ba-1733-4811-93de-4531c2ce76ab.jpg" />. If d = 2let r be such that, <img src="8-5300438\d9221c77-e1a4-4f97-88dc-bda058bb9fd6.jpg" />, then there exists a constant c &gt; 0 such that if R is the solution of, <img src="8-5300438\dc3dc245-1e64-4a44-94bf-9f76aaa780ad.jpg" />, with</p><p><img src="8-5300438\04e69861-2b31-4bdd-be04-d6efc687b682.jpg" /><img src="8-5300438\b5611f1c-028d-4f19-868c-97dc75e5bcfa.jpg" />, <img src="8-5300438\8c9412b1-7e05-4fba-aa75-80f1637a2500.jpg" />then</p><p><img src="8-5300438\4d4c2ea3-db5a-4250-8e51-facff2783ebb.jpg" /></p><p>Furthermore, c depends only on d, p, r and,</p><p><img src="8-5300438\e68142f2-01a6-4528-ab94-557c5d94d599.jpg" />.</p><p>The method made up in rescheduling, by the average of a time dependent rescheduling the equation, and to use the energy of the equation, to get by interpolation decay estimates in suitable norms. The asymptotically average, is normally obtained directly by using the pseudo conformal law, the above result was in fact partially proved in [<xref ref-type="bibr" rid="scirp.36305-ref8">8</xref>], under a bit different point of view: look for a time dependent change of coordinates, which maintain the Galilean invariance, and the construction directly a Lyapunov functional by a suitable ansatz. This Lyapunov functional is surely the energy of the rescaled equation. Our aim here is to study with further details the rescaled wave function and its energy. Found to be the method provides rates which are seems completely new in the limiting case of the logarithmic nonlinear Schr&#246;dinger equation. Because of the reversibility of the Schr&#246;dinger equation and standard results of scattering theory, one cannot foresee the convergence of the rescaled wave function to some a intuition given limiting wave function, but found to be some convexity properties of the energy can be used to state an asymptotically stabilization result. From the general theory of Schr&#246;dinger equations, it is well known that the Cauchy problems (1.1)-(3.1) is well posed for any initial data in <img src="8-5300438\746bccaa-3ba7-4a70-beb8-06e40c48ce63.jpg" /> when<img src="8-5300438\39d16ef4-fa39-4249-8b14-4740ed7dc6ce.jpg" />, and that the solution u belongs to</p><p><img src="8-5300438\1bb53ff2-5ec0-45c2-a59f-2474e8f1ad34.jpg" /></p><p>As usual for Schr&#246;dinger equations is critical when<img src="8-5300438\14e90b5e-fedd-4dc5-8acb-6e12acc461a9.jpg" />.</p><p>Let <img src="8-5300438\bf09addc-8b4e-4b46-9fd1-267bf9642e91.jpg" /> be such that</p><p><img src="8-5300438\0001d3e5-e1a5-4cd7-926b-1d6e34a7d663.jpg" />.</p><p>where and <img src="8-5300438\f8a321d4-73ae-4016-b3d1-a22c7fba458c.jpg" /> are positive derivable real functions of the time.</p><p>It is simple to check that with this change of coordinates, <img src="8-5300438\f63e9545-f567-4f93-99ce-933d50f85ff6.jpg" />satisfies the following equation,</p><p><img src="8-5300438\6033f377-d5a5-495d-8ccd-84560e46a045.jpg" /></p><p>where<img src="8-5300438\2e953f04-0d47-4f0e-b48c-9f98eeb3d8da.jpg" />, with the choice<img src="8-5300438\6e4c2fe2-1263-41b6-a525-4048bc7f2fdd.jpg" />, which means that <img src="8-5300438\73542caa-270a-4a3e-ae53-1f3aacfc5a9a.jpg" /> and u are linked by,</p><disp-formula id="scirp.36305-formula143655"><label>(3.2)</label><graphic position="anchor" xlink:href="8-5300438\e2502d9c-f4c1-442b-9ae9-8c802c207342.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="8-5300438\3ba9a62d-fb67-4f43-93ed-f150a8a60aa2.jpg" /> and <img src="8-5300438\a56eaecb-55bd-4cc7-9743-4e1762ec51ad.jpg" /> and <img src="8-5300438\42821efa-f961-4f0b-afa1-67ebf2ffc6bc.jpg" /> has to satisfy the following time-dependent defocusing nonlinear Schr&#246;- dinger equation,</p><disp-formula id="scirp.36305-formula143656"><label>(3.3)</label><graphic position="anchor" xlink:href="8-5300438\fbbfd9a2-8202-447d-8b53-0a62986e1662.jpg"  xlink:type="simple"/></disp-formula><p>We note that <img src="8-5300438\0456e283-93d1-40a7-8555-fa90314387cd.jpg" /> so that</p><p><img src="8-5300438\9a4ea02b-f7fc-4694-82ed-a4034da5c771.jpg" /></p><p>for all<img src="8-5300438\02418551-58aa-4210-a7c6-fe3fef61f188.jpg" />.</p><p>Also we note that if <img src="8-5300438\d3a253c6-2125-4890-bfb0-ea217ee3ac32.jpg" /> and <img src="8-5300438\4d3a2a23-59f9-40c8-a01d-014e6e8a21e5.jpg" /> then</p><disp-formula id="scirp.36305-formula143657"><label>(3.4)</label><graphic position="anchor" xlink:href="8-5300438\41cfa1e3-a1a4-402a-a402-e1613a856745.jpg"  xlink:type="simple"/></disp-formula><p>To extract the controlling impacts as <img src="8-5300438\9d9c58b0-b43a-4cc5-8dbf-5dc21555a8aa.jpg" /> we fix <img src="8-5300438\9b710218-9e24-46cb-b177-5439814dd1d1.jpg" /> and R such that,</p><p><img src="8-5300438\efdabdda-52bd-4cfd-bb5a-4c0b730d0abb.jpg" /></p><p>where</p><disp-formula id="scirp.36305-formula143658"><label>(3.5)</label><graphic position="anchor" xlink:href="8-5300438\1f727779-0e60-4270-ad30-3de5cc1901b0.jpg"  xlink:type="simple"/></disp-formula><p>Because p is critical, this ansatz is actually the only one that sets to 1 at least three of the four coefficients in the equation for<img src="8-5300438\6dab76bb-baf5-45e3-8842-fddc4eddc33e.jpg" />, with <img src="8-5300438\733e27d2-5774-4b5a-933a-570702110a34.jpg" /> and <img src="8-5300438\97bd71e6-a961-4b3d-88a0-edf339c13a02.jpg" /> solves the equation,</p><disp-formula id="scirp.36305-formula143659"><label>(3.6)</label><graphic position="anchor" xlink:href="8-5300438\a41ed552-0c92-44f6-b9e8-9f62e3a03bfa.jpg"  xlink:type="simple"/></disp-formula><p>With the choice <img src="8-5300438\950f4262-97b7-4241-9c5a-94622346edf1.jpg" /> and<img src="8-5300438\2de7baf0-c6e1-4752-adbf-2d871bed3c77.jpg" />, integration of (3.5) with respect to t gives <img src="8-5300438\08ede723-02ed-4dcd-bec4-f87242729a44.jpg" /> and this is possible if, and only if, <img src="8-5300438\e0dbaeb6-5405-4098-be8e-1a4e8cc7293d.jpg" />for all <img src="8-5300438\01327387-9fad-4517-88ff-be392792e04a.jpg" /> thus the function <img src="8-5300438\7a3ba6e5-2ed6-4fa3-bfb3-e1ed31940163.jpg" /> is globally defined on <img src="8-5300438\9db32ba7-8f09-4b41-8ca2-d1468dd382c5.jpg" /> increasing, <img src="8-5300438\3d7e64d8-e793-4e1b-8d92-a7fb0c94ee67.jpg" />and <img src="8-5300438\a4377111-e198-46fb-a462-0daa5f08db6c.jpg" /> as<img src="8-5300438\96fc6eda-1111-4764-8a36-396042c07ad4.jpg" />.</p><p>Supposing that<img src="8-5300438\783094b9-23dc-472f-8460-c278141c867a.jpg" />, <img src="8-5300438\5ca1c9ae-2d93-442a-978d-14c2c9e77f13.jpg" />is an increasing positive function such that, <img src="8-5300438\13b0a7f5-171d-4b8b-a9eb-c654c75484d7.jpg" />, where <img src="8-5300438\eb2d8736-fb49-402e-a4f9-cc8558e3f2c9.jpg" /> if<img src="8-5300438\63ce629f-dc3b-4900-9d03-5d15bff910c1.jpg" />.</p><p>Consider now the energy functional linked to Equation (3.6)</p><disp-formula id="scirp.36305-formula143660"><label>(3.7)</label><graphic position="anchor" xlink:href="8-5300438\41e85434-2b32-41e5-8408-393747d7226f.jpg"  xlink:type="simple"/></disp-formula><p>where R has to be understood as a function of.</p><p>Lemma 3.2. Suppose that<img src="8-5300438\9bd08697-7297-4d02-ad57-404214ed2d0e.jpg" />, if<img src="8-5300438\67e4e8d3-34c7-41b9-a798-e51398224b04.jpg" />, and let u be a solution to (1.1), identical to an initial data,</p><p><img src="8-5300438\abe4e91f-5a6b-453a-955d-f6ee1a64f841.jpg" />such that<img src="8-5300438\1fd97066-8530-4840-abe3-3950558833cf.jpg" />.</p><p>With the above notations, E is a decreasing positive functional. Thus <img src="8-5300438\21141c1c-69b1-4f07-9782-e64524637260.jpg" /> is bounded by<img src="8-5300438\4f961a71-98c1-457c-9bf9-eff798e8ad82.jpg" />, with the notations of Theorem 3.1.</p><p>Proof: The proof follows by a direct computation.</p><p>Because of (3.6), only the coefficients of<img src="8-5300438\b877a126-833e-4a7e-8bcc-7f643f74fda2.jpg" />, and <img src="8-5300438\436ed15a-9ffe-4bc0-b929-d49e693714cc.jpg" /> contribute to the decay of the energy.</p><p>For more see [<xref ref-type="bibr" rid="scirp.36305-ref9">9</xref>].&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160; &#160;&#160;&#160;&#160;<img src="8-5300438\8b120a58-c0b5-43a0-b688-84d26b7b57d1.jpg" /></p><p>Proof of Theorem 3.1: Suppose that p is critical. By Lemma 3.2 and pursuant to the time-dependent rescaling (3.2),</p><p><img src="8-5300438\4052fb21-c8b3-4e37-ac6a-0e0f6d4331b1.jpg" /></p><p>Thus</p><p><img src="8-5300438\5a25a1e8-3936-47c1-81db-8e2f12f96390.jpg" /></p><p>Is bounded by<img src="8-5300438\bc9205d4-2661-4f8c-b7ac-0c2935985782.jpg" />, the remainder of the proof follows the same lines that in Theorem 7.2.1 of [<xref ref-type="bibr" rid="scirp.36305-ref10">10</xref>], see also [11,12], using maintain the L<sup>2</sup>-norm and the Sobolev-Gagliardo-Nirenberg inequality.&#160;&#160;&#160;&#160;&#160;&#160; <img src="8-5300438\8a32d3c9-9a35-4ca8-85bc-95285525f249.jpg" /></p><p>Proposition 3.3. Consider the two-dimensional defocusing cubic NLS (1.1), (is <img src="8-5300438\d315728f-f86b-424f-a91e-7712f6c56faa.jpg" />-critical). Let <img src="8-5300438\03cdd0e3-1dcb-4220-ba11-4907d3a86d7c.jpg" /> then there exists a global <img src="8-5300438\27d24d75-0ce9-459b-89d3-8b4c615e0f50.jpg" />-well posed solution to (1.1), and moreover the <img src="8-5300438\f0c8a3e1-a693-4a4a-ab64-66c768a7987a.jpg" /> norm of u<sub>0</sub> is finite.</p><p>Proof: By time reflection symmetry and adhesion arguments we may heed attention to the time interval <img src="8-5300438\e59b1480-a7a6-4e4d-a47c-a13531101a0f.jpg" /> Since u<sub>0</sub> lies in<img src="8-5300438\f5d58f5c-5ff6-48f2-954a-eae7cbd7d8d6.jpg" />, it lies in<img src="8-5300438\a4afa876-f875-4582-9922-232692115ff4.jpg" />. Apply the <img src="8-5300438\d6b76452-2d9d-4017-85dd-df9cff95d341.jpg" /> well posedness theory (Proposition 1.2) we can find an <img src="8-5300438\e104877f-bb40-46f4-9912-0f167fd46380.jpg" />-well posed solution<img src="8-5300438\21b15cf5-fd99-488a-8f52-c6ffcc470392.jpg" />, on some time interval <img src="8-5300438\9d0353c4-76e1-41c1-9091-87e7088207c9.jpg" />with <img src="8-5300438\c9fcd567-d555-46b6-937f-cb0f281099ef.jpg" /> depending on the profile of u<sub>0</sub>.</p><p>Specially the <img src="8-5300438\07ce83da-f7ba-4bd9-a214-6f9cbc157fa1.jpg" /> norm of u is finite. Next we apply the pseudoconformal law to deduce that,</p><p><img src="8-5300438\cc843325-ac19-4ecf-ba9b-b7c8fb4544c0.jpg" /></p><p>Since<img src="8-5300438\d96ecb73-76d4-47bd-bde3-827917aef158.jpg" />, we got a solution from t = 0 to t = T. To go to all the way to<img src="8-5300438\b162e4f4-a0b7-443c-9fbe-18129a3916e9.jpg" />. We apply the pseudoconformal transformation at time t = T, obtaining an initial datum <img src="8-5300438\561aa4a9-cf00-4943-bdf6-d1a7680eef5a.jpg" /> at time <img src="8-5300438\e666828f-ab4e-435a-baa1-556504416e22.jpg" /> by the formula</p><p><img src="8-5300438\3e3e210b-981d-4455-9d61-b6db9c08069a.jpg" /></p><p>From <img src="8-5300438\c6c3d703-0c2c-4a6f-8867-2acb8e00b392.jpg" /> we see that v has finite energy:</p><p><img src="8-5300438\f4c6859b-b3bd-406a-aa83-37599eabc8e6.jpg" /></p><p>And, the pseudoconformal transformation saves mass and hence</p><p><img src="8-5300438\c9d34029-8f54-4fdc-87d1-c86d49893e46.jpg" /></p><p>So we see that <img src="8-5300438\19b91e3d-a1b5-4bce-99eb-b289ba541308.jpg" /> has a finite <img src="8-5300438\ca56940d-71c9-4130-86a5-66533880ed1b.jpg" /> norm. Thus, we can use the global <img src="8-5300438\4c6d429d-ea88-498a-8414-7c21d08ecaa8.jpg" />-well posedness theory, backwards in time to obtain an <img src="8-5300438\d1209212-d8c4-4839-aa72-330d1865fda3.jpg" />-well posed solution</p><p><img src="8-5300438\d42eed26-4090-4697-bb45-15fe7e542ab8.jpg" />, to the equation <img src="8-5300438\cb539625-104c-4773-8663-afc6c1bc772e.jpg" /> particularly, <img src="8-5300438\bed4dee3-52d4-4f04-8592-b6206b99932c.jpg" /></p><p>We reverse the pseudoconformal transformation, which defines the original field u on the new slab <img src="8-5300438\2d451355-b3cf-4ccf-b575-63445efc2a1b.jpg" /></p><p><img src="8-5300438.files/image017.gif" />We see that the<img src="8-5300438\7c1f176b-1175-4020-a04e-1293d100b4a5.jpg" />, and</p><p><img src="8-5300438\09f271ab-8203-422d-b76d-dcbcdecaafe7.jpg" />norm of u are finite. This is sufficient to make u an <img src="8-5300438\aa1071ac-08c7-4a50-9d29-dbe991f15688.jpg" />-well posed solution to NLS on the time interval<img src="8-5300438\005248fa-2e15-4073-8454-ed232c321adb.jpg" />; for v classical. And for general<img src="8-5300438\36420cc5-825a-4576-a395-4e0c79af8dd9.jpg" />, the claim follows by a limiting argument using the <img src="8-5300438\ddb2774e-ffb3-4e7c-88b4-fe564ff65c18.jpg" />-well posedness theory. Adhesion together the two intervals <img src="8-5300438\fab7f49c-aa67-4c74-a897-f15f6fcadd53.jpg" /> and<img src="8-5300438\45f240d5-e4fb-4381-82c5-0892a2ed8236.jpg" />, we have obtained a global <img src="8-5300438\e2e36ee1-3166-4a3b-b3db-b13a86b40b82.jpg" /> solution u to (1.1).</p></sec><sec id="s4"><title>4. Some Lemma</title><p>Consider the defocusing case of the NLS (1.1) and if<img src="8-5300438\dba8064b-82f0-46c6-b2b0-64014f2b0998.jpg" />, the energy and mass together will control the <img src="8-5300438\c8ac1937-b237-429c-adeb-561bdfd74ae6.jpg" /> norm of the solution:</p><p><img src="8-5300438\43bc85c8-0035-4acd-8ace-c155fe3f7775.jpg" /></p><p>Conversely, energy and mass are controlled by the <img src="8-5300438\ecda8c2b-b35e-481d-a4f8-0854c92d6dee.jpg" /> norm (the Gagliardo-Nirenberg inequality showed that):</p><p><img src="8-5300438\dbe26ce3-0c3f-4e50-bab4-acecff228782.jpg" /></p><p><img src="8-5300438\554ec166-4255-4ad1-9c8b-3a8361a7ce2c.jpg" /></p><p>This bound and the energy conservation law and mass conservation law showed that for any <img src="8-5300438\8072be6a-a927-44a5-99a1-48454bedba25.jpg" />-well posed solution, the <img src="8-5300438\68b74748-4aa6-40ba-a7c8-ca20e35bc41c.jpg" /> norm of the solution <img src="8-5300438\f9503f9d-2641-48fb-abec-1517bd3c4cf0.jpg" /> at time t is bounded by a quantity depending only on the <img src="8-5300438\94c3c856-7f50-4830-9d5e-4d9a3d6455e5.jpg" /> norm of the initial data.</p><p>Proposition 4.1. The cubic NLS (1.1) with<img src="8-5300438\f127d327-6214-46b6-9554-9d8d2e9640fd.jpg" />, d = 2 is globally well posed in<img src="8-5300438\6b6325e0-16e8-4078-98c3-04687bd0b1d4.jpg" />. Actually, for <img src="8-5300438\f05f6302-2d19-4294-a14d-8603a6ddcd17.jpg" /> and any time interval, K the Cauchy problem (1.1) has a <img src="8-5300438\4aeca544-c210-468b-a1de-b26d7fadf725.jpg" /> well posed solution</p><p><img src="8-5300438\9a1e8226-b4af-493a-a0c6-c3bbece4ba52.jpg" /></p><p>Lemma 4.2. If <img src="8-5300438\2d711a17-13e7-42c9-94c6-208c6ba981d3.jpg" /> the following holds:</p><p><img src="8-5300438\63ac2933-86c2-48d7-b89d-c1d8872e1d39.jpg" />.</p><p>Proof: The proof depends on the noticing that;</p><p><img src="8-5300438\9998febb-752f-4eef-bb85-94978ad8f1cc.jpg" />.</p><p>With</p><p><img src="8-5300438\86bebb61-67b7-42a2-b41b-fcbc4f43ab2f.jpg" /></p><p>Thus</p><p><img src="8-5300438\b6370777-5a40-435f-a487-26b3f25f95a2.jpg" /></p><p>By standard Gagliardo-Nirenberg inequality,</p><p><img src="8-5300438\4ebe06ca-e404-4cbf-900b-2155bd68cd23.jpg" /></p><p>Lemma.4.3. Let<img src="8-5300438\eebd74fc-d228-4b09-aa80-8b539657e928.jpg" />. For any spacetime slab<img src="8-5300438\9c5200a0-5050-42df-9c2f-855a1055cdf7.jpg" />, <img src="8-5300438\2a8d97fc-c752-4286-987f-266238ff3c3a.jpg" />, and for any <img src="8-5300438\ac017faf-47ac-4b4f-a4eb-01df16e2e030.jpg" /></p><disp-formula id="scirp.36305-formula143661"><label>(4.1)</label><graphic position="anchor" xlink:href="8-5300438\1290155f-4443-423f-991f-a8317bd3d74e.jpg"  xlink:type="simple"/></disp-formula><p>The estimate (4.1) is very helpful when u is high hesitancy and v is low hesitancy, as it moves abundance of derivatives onto the low hesitancy term. In particular, this estimate shows that there is little interaction between high and low hesitancy. This estimate is basically the repeated Strichartz estimate of Bourgain in [<xref ref-type="bibr" rid="scirp.36305-ref13">13</xref>]. We make the trivial remark that the <img src="8-5300438\510e3e8a-9cdc-4bea-9681-5542fdab4ec4.jpg" /> norm of uv is the same as that of<img src="8-5300438\8c68e5ec-f7a0-43e5-ab00-dff487cbfaca.jpg" />, <img src="8-5300438\98b1689d-da58-4419-8c8a-a54728b7c5a0.jpg" />, or<img src="8-5300438\bd9e78ef-87c3-40fa-a144-cb30874e4296.jpg" />, thus the above estimate also applies to expressions of the form <img src="8-5300438\01f07fae-b07f-4add-8e5a-50c87776f0e3.jpg" /></p><p>Proof: We fix<img src="8-5300438\971f5b02-dd8a-4c92-9d3d-2ddc1c797352.jpg" />, and permit our tacit constants to depend on<img src="8-5300438\a3ed5052-6d5b-4f5b-95d5-356b834943ea.jpg" />. We begin by dealing with homogeneous case, with <img src="8-5300438\32cc7ca9-3fb9-4f75-b197-6883ab493f15.jpg" /> and<img src="8-5300438\315ba725-d1c3-4a9d-b34a-1910d6afb308.jpg" />, And consider the more general problem of proving,</p><disp-formula id="scirp.36305-formula143662"><label>(4.2)</label><graphic position="anchor" xlink:href="8-5300438\609e9100-a82c-4af7-9826-8b09a615c3c6.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="8-5300438\0d8e8e4d-7212-44a4-af8a-1d756fd87795.jpg" /> the scaling invariance of this estimate, first, our objective is to prove this for <img src="8-5300438\5959c8f7-bd2a-457c-8148-dc96965dba11.jpg" /> and<img src="8-5300438\1ec316cf-f4b7-489d-9a97-12f27805416e.jpg" />.</p><p>May be recast (4.2) using duality and renormalization as</p><disp-formula id="scirp.36305-formula143663"><label>(4.3)</label><graphic position="anchor" xlink:href="8-5300438\0171dc8b-b0e7-4aee-aadd-4fc1a670994e.jpg"  xlink:type="simple"/></disp-formula><p>Since<img src="8-5300438\65f1d707-45e3-46e0-a2ad-9743995466a4.jpg" />, we may restrict attention to the interactions with <img src="8-5300438\44793b88-0d48-4b32-a33f-b1ada053fb07.jpg" /></p><p>In fact, in the residual case we can multiply by</p><p><img src="8-5300438\ccdc7887-e1ab-4c65-a628-a8d5ceb5e8f9.jpg" />to return to the condition under discussion. In fact, we may further restrict attention to the case where <img src="8-5300438\4d73c195-d73c-4278-bf7e-6ceee074de1c.jpg" /> since, in the other case, we can move the frequencies between the two factors and reduce the case where<img src="8-5300438\4da14d8f-e405-40c3-a46a-e2b87581680b.jpg" />, which can be dealt by <img src="8-5300438\b2ba1cc8-65b7-4e79-ae0d-b7c15cb84f3f.jpg" /> Strichartz estimates when <img src="8-5300438\63dfc36c-72fb-460e-b4f0-2e452c565fd2.jpg" /> Next, we decompose <img src="8-5300438\11578214-074f-4776-a09e-4f8c0025b558.jpg" /> dyadically and <img src="8-5300438\94516bf1-1495-4968-9595-cb603d33b693.jpg" /> in dyadic multiples of the size of <img src="8-5300438\a46746c7-9250-4202-9cde-aa5c3de10b80.jpg" /> by rewriting the quantity to be controlled as (N, <img src="8-5300438\80e1e21d-16d9-43c5-9971-c59d184e352d.jpg" />dyadic):</p><p><img src="8-5300438\cec14e9b-198c-4188-a2d0-7b1f281a6013.jpg" /></p><p>Note that subscripts on <img src="8-5300438\92e13fda-2691-4c23-adb6-65c7a959202f.jpg" /> have been inserted to invoke the localizations to<img src="8-5300438\27105927-aa85-44ac-8180-0d8e82ed2d52.jpg" />, <img src="8-5300438\17ff0016-39a6-487b-ad21-e93a718b47e0.jpg" />, <img src="8-5300438\e7ce7429-70f2-46bd-a117-ff73922f794a.jpg" />, consecutive. In the case<img src="8-5300438\507cd835-5d19-412c-ba99-e3fb736ce11a.jpg" />, we have that <img src="8-5300438\360e8046-ea2c-4a48-a9c8-96fcbd314dd5.jpg" /> and this expound, why g may be so localized. By renaming components, we may suppose that <img src="8-5300438\04466d48-f427-4d1d-ae98-0c29361ca411.jpg" /> and<img src="8-5300438\f80be997-0b1b-4e9b-98de-104f873445d4.jpg" />.</p><p>Write <img src="8-5300438\7ee1ee18-29ea-44d0-8fd2-159b5fbdb82d.jpg" /> We change variables by writing</p><p><img src="8-5300438\b8580be2-7959-42b2-8474-2597f4f74c6b.jpg" /></p><p>And <img src="8-5300438\ccff7488-5cc5-439d-99d1-403efa3c30ee.jpg" /></p><p>We show that by calculation</p><p><img src="8-5300438\7fab6217-f581-48ee-9c52-505b2d09744d.jpg" /></p><p>Thus, upon changing variables in the inner two integrals, we encounter</p><p><img src="8-5300438\b87f1b09-9567-4e5f-b780-2a29eef80c82.jpg" /></p><p>where</p><p><img src="8-5300438\c45fe0f0-4d33-47c5-9a3f-1cb5c5a73dc8.jpg" /></p><p>Apply the Cauchy-Schwarz on the u, v integration and change back to the original variables to obtain</p><p><img src="8-5300438\2798af16-4e04-49f7-9725-7f7c108f83f9.jpg" /></p><p>We recall that <img src="8-5300438\ca3b4971-af7a-4e9f-aec9-46d28b9630ae.jpg" /> and use Cauchy-Schwarz in the integration, taking into consideration the localization<img src="8-5300438\433b6070-1323-4a96-b2e8-50f8c2a6d51e.jpg" />, to get</p><p><img src="8-5300438\ae8ca94c-ef44-49fb-9842-d29464ff78fb.jpg" /></p><p>Choose <img src="8-5300438\95f1c1de-d6d1-41fe-8fd8-f4d4b8b1e736.jpg" /> and<img src="8-5300438\e8d16efa-283a-4e16-b10f-15e470154232.jpg" />. with <img src="8-5300438\7cc6a7ef-9a0e-416f-813b-9c8e6fbe9a60.jpg" /> to obtain</p><p><img src="8-5300438\b31f80f2-aa32-4a30-9de1-341493bf4438.jpg" /></p><p>This summarizes to get the claimed homogeneous estimate. Now we discuss the inhomogeneous estimate (4.1). For simplicity we set, <img src="8-5300438\5312d3a2-3b79-4e38-9a00-a90c43fad373.jpg" />and <img src="8-5300438\c05811cb-bdd3-4922-b863-239aa69aeeb9.jpg" />. Then we use Duhamel’s formula to write</p><p><img src="8-5300438\14b27395-e438-4fb1-aa86-7a83a4d7cadb.jpg" /></p><p><img src="8-5300438\09575348-aade-4ce8-bb59-865e34b5351d.jpg" /></p><p>We obtain</p><p><img src="8-5300438\bb786dad-0fa9-485c-8a81-fbf6c9a314aa.jpg" /></p><p>The first term was treated in the first part of the proof. The second and the third are similar and so we consider I<sub>2</sub> only. By the Minkowski inequality,</p><p><img src="8-5300438\4bbec2ef-d0b5-43ce-bb1c-897344d4c67f.jpg" /></p><p>And in this case the lemma follows from the homogeneous estimate proved above. Finally, again by Minkowski’s inequality we have</p><p><img src="8-5300438\15dd02a6-264b-46d2-aaea-f148bfdc8032.jpg" /></p><p><img src="8-5300438.files/image017.gif" />And the proof follows by inserting in the integral the homogeneous estimate above.&#160; &#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;<img src="8-5300438\9b9c3471-c277-409d-a3ae-e3369b95fcb4.jpg" /></p><p>Lemma.4.4. Let <img src="8-5300438\15512d4e-d438-4c30-858c-f1d1e19d3b3f.jpg" /> is nearly periodic modulo G. Then there exist functions<img src="8-5300438\29ab1f77-94bd-4922-81a9-cfc22c0fb399.jpg" />, <img src="8-5300438\c56ea5d4-22f3-4b63-8e3e-f1b6fe5ef4f0.jpg" />and<img src="8-5300438\73258ac4-0bac-4528-b315-4f0503a59a7a.jpg" />, and for every <img src="8-5300438\dbdc6f6a-d227-4f28-a407-6109190cc4e7.jpg" /> there exists <img src="8-5300438\bc45a628-f8ba-4546-90ee-92442cd7ff40.jpg" /> such that we have the spatial concentration estimate,</p><disp-formula id="scirp.36305-formula143664"><label>(4.3)</label><graphic position="anchor" xlink:href="8-5300438\a5e94a75-4710-40d9-9ce8-a3da5f137fbf.jpg"  xlink:type="simple"/></disp-formula><p>And hesitancy concentration estimate,</p><disp-formula id="scirp.36305-formula143665"><label>(4.4)</label><graphic position="anchor" xlink:href="8-5300438\79b781d7-4080-4b58-9f55-bb0d239abc06.jpg"  xlink:type="simple"/></disp-formula><p>For all <img src="8-5300438\d29a1d3b-5988-40b3-b05c-da22a4af545c.jpg" /></p><p>Remark 4.5. Informally, this lemma confirms that the mass <img src="8-5300438\9e6361f9-5802-4fd4-bd87-b59eaec433fc.jpg" />is spatially concentrated in the ball</p><p><img src="8-5300438\9685266f-54d3-4bf3-b561-b618a76d75b0.jpg" />And is hesitancy concentrated in the ball</p><p><img src="8-5300438\1a15245e-8fb3-4e1c-8736-0e49ebbba976.jpg" />.</p><p>Note that we have presently no control about how<img src="8-5300438\ad067a6a-f65e-436b-a97c-dbcb963ed054.jpg" />, <img src="8-5300438\2bbe8cc4-f9df-4103-99c0-cec40f6fb859.jpg" />, <img src="8-5300438\4e73c9a3-741f-4715-80a6-95c5c6f256bf.jpg" />vary in time; (for more see [14- 17]).</p><p>Proof: By hypothesis, <img src="8-5300438\9e280847-d11f-42d2-bdb2-f8af39a5e07d.jpg" />lay in GI for some compact subset I in<img src="8-5300438\28f91bf9-96a7-43ae-965d-eb7a2b147afd.jpg" />. For every<img src="8-5300438\658d23bd-6cc9-4919-a17c-cff9245d69eb.jpg" />, compactness argument shows that there exists<img src="8-5300438\249f9c64-6679-40b1-96f6-f7452b0fbc61.jpg" />, (depending on) such that</p><p><img src="8-5300438\0784611e-db1a-41fb-963c-5f506ec8f2ec.jpg" /></p><p>And hesitancy concentration estimate</p><p><img src="8-5300438\1546ada6-4e33-4a70-a885-cc2dc855d9fa.jpg" /></p><p><img src="8-5300438.files/image018.gif" />For all<img src="8-5300438\e5ad5f6a-6a6b-4674-bb47-a19f8404813c.jpg" />. By inspecting what the symmetry group G does to the spatial and hesitancy distribution of the mass of a function, then the claim follows. &#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;<img src="8-5300438\acb1c38b-45bd-48a6-b943-cc201a699dea.jpg" /></p><p>Corollary 4.6. Fix <img src="8-5300438\fc5fc7a1-7405-4506-a4f0-9fedf50d3bc4.jpg" /> and d, and assume that m<sub>0</sub> is finite. Then there exists a maximal-lifespan solution <img src="8-5300438\37812dd8-236a-4623-a590-683976650177.jpg" /> of mass precisely m<sub>0</sub> which blows up both forward and backward in time, and functions, <img src="8-5300438\31ee1daa-faba-457e-aa73-35ea2659673a.jpg" />, <img src="8-5300438\45dfb8f2-a4e8-474d-b4c2-547725bac5a4.jpg" />and<img src="8-5300438\156bd3dd-228a-4796-b914-d0ba823701e5.jpg" />, with property<img src="8-5300438\d8217872-b9ba-4a61-8a4c-c6092ae56a41.jpg" />, for every <img src="8-5300438\9cd2b627-7c07-4a87-9dec-d16013a4203e.jpg" /> (depending on<img src="8-5300438\8acdaa8d-9e03-475e-b65c-9b844aab362e.jpg" />, d, m<sub>0</sub>) such that we have the concentration estimates (4.3), (4.4) For all <img src="8-5300438\dcc51056-0f34-4929-9756-cdb4afa98102.jpg" /></p></sec><sec id="s5"><title>REFERENCES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.36305-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">T. 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