<?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">IJMNTA</journal-id><journal-title-group><journal-title>International Journal of Modern Nonlinear Theory and Application</journal-title></journal-title-group><issn pub-type="epub">2167-9479</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ijmnta.2013.22015</article-id><article-id pub-id-type="publisher-id">IJMNTA-32976</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Engineering</subject><subject> Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Stability Solution of the Nonlinear Schr&#246;dinger Equation
 
</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>13</day><month>06</month><year>2013</year></pub-date><volume>02</volume><issue>02</issue><fpage>122</fpage><lpage>129</lpage><history><date date-type="received"><day>February</day>	<month>19,</month>	<year>2013</year></date><date date-type="rev-recd"><day>March</day>	<month>28,</month>	<year>2013</year>	</date><date date-type="accepted"><day>April</day>	<month>30,</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>
 
   In this paper we discuss stability theory of the mass critical, mass-supercritical and energy-subcritical of solution to the nonlinear Schrodinger equation. In general, we take care in developing a stability theory for nonlinear Schrodinger equation. By stability, we discuss the property: the approximate solution to nonlinear Schrodinger equation <img style="width:16px;height:14px;" alt="" src="Edit_2591676b-4a2f-4ed0-8738-973ec45d319b.bmp" width="19" height="17" /> obeying <img style="width:124px;height:18px;" alt="" src="Edit_7664acc5-6661-4d08-9d14-758083882dba.bmp" width="163" height="21" />  with e small in a suitable space and <img style="width:40px;height:14px;" alt="" src="Edit_d5d6897e-2d33-4481-9bdd-13bec36ee1ce.bmp" width="41" height="15" /> small in <img style="width:20px;height:19px;" alt="" src="Edit_46bcfd46-06d9-4d62-9a86-76c08b683193.bmp" width="23" height="21" /> and then there exists a veritable solution u to nonlinear Schrodinger equation which remains very close to <img alt="" src="Edit_f24e1d31-fe01-41e3-9a6f-3dfa55faaac0.bmp" width="16" height="15" />in critical norms. 
 
</html></p></abstract><kwd-group><kwd>NLS; Wellposed</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>In this paper, we study the stability theory of solutions to the nonlinear Schr&#246;dinger equation (NLS).</p><p>We consider the Cauchy problem for the nonlinear Schr&#246;dinger equation</p><disp-formula id="scirp.32976-formula55488"><label>(1.1)</label><graphic position="anchor" xlink:href="2-2340075\7364b8d9-7925-4e5a-b9c9-75b22aea10b0.jpg"  xlink:type="simple"/></disp-formula><p>where<img src="2-2340075\005a7e50-0c0b-41aa-9d50-432e73cc9ea6.jpg" />, <img src="2-2340075\51a73038-d616-4f96-9534-c9bf08af26cc.jpg" />the solution <img src="2-2340075\014f5438-c2ff-4f9e-b50f-173cfae5cc02.jpg" /></p><p>is a complex-valued function in <img src="2-2340075\ae0c3871-1773-4dd6-a111-eda548324187.jpg" /></p><p>The Equation (1.1) is called mass-critical or <img src="2-2340075\7cf56b3d-210a-4025-9d53-696bc724cbdd.jpg" />critical if<img src="2-2340075\9bc5a8d4-02c9-41cf-a36d-65d94edc8bea.jpg" />, and it is called mass-supercritical and energy-subcritical when<img src="2-2340075\452a2f9d-03fb-4b1f-833e-f205e0d7bc31.jpg" />.</p><p>The solutions to (1.1) have the invariant scaling</p><disp-formula id="scirp.32976-formula55489"><label>(1.2)</label><graphic position="anchor" xlink:href="2-2340075\1d681475-7242-48bd-9f9a-3477fc4f259a.jpg"  xlink:type="simple"/></disp-formula><p>Definition 1.1 (Solution) Let <img src="2-2340075\c3ef613a-6f82-4de5-bee2-989d6f33a8dd.jpg" /> such that<img src="2-2340075\0800da6c-9233-4cb1-b981-e6526fa41d7d.jpg" />. A function <img src="2-2340075\169e2611-4ff1-4930-af0f-0f318d7b599f.jpg" /> is a strong solution to (1.1)</p><p>if and only if it belongs to<img src="2-2340075\7b812adb-575f-42a1-ac97-1e9f99c7984b.jpg" />, and for all <img src="2-2340075\a7364a30-1b9b-444e-af59-90f7841d3e83.jpg" /> satisfies the integral equation</p><disp-formula id="scirp.32976-formula55490"><label>(1.3)</label><graphic position="anchor" xlink:href="2-2340075\c375113b-cb40-4f00-b3f6-77857fb70fae.jpg"  xlink:type="simple"/></disp-formula><p>A function <img src="2-2340075\2aa81d69-6291-4525-87eb-9fba8b513ef8.jpg" /> is a weak solution to (1.1)</p><p>if and only if<img src="2-2340075\6fe561fe-80c9-4f35-af86-3ae2eb85dda9.jpg" />, and for all <img src="2-2340075\a11dac11-7c4d-439c-bcef-9cfa1f697e8f.jpg" /></p><p>satisfies the integral Equation (1.3).</p><p>The solutions to (1.1) have the mass</p><p><img src="2-2340075\2cf39c51-ecf3-4ac9-94fb-3f15191bc35d.jpg" /></p><p>where</p><p><img src="2-2340075\1553bc3b-1dda-4ced-b2c3-8fb544b3557e.jpg" /></p><p>Energy <img src="2-2340075\5ebde768-020c-4578-9878-34ef24fe571e.jpg" /> where,</p><p><img src="2-2340075\f2ff6bd1-49e4-48a7-9a67-23f2385d9b25.jpg" /></p><p>Definition 1.2 The problem (1.1) is locally wellposed in <img src="2-2340075\65586e47-5890-469f-8d9b-3f8a29405a68.jpg" /> if for any <img src="2-2340075\3e64e52c-86d1-4b38-9ace-1de51b7fc10a.jpg" /> there exist a time <img src="2-2340075\c94f2529-656e-48c1-a915-98dbf78737a9.jpg" /> and an open ball <img src="2-2340075\d6ac3e53-a285-4298-adb8-287d92825758.jpg" />in <img src="2-2340075\15cff8b2-d85f-4034-914b-27554d5c25d1.jpg" /> such that</p><p><img src="2-2340075\046e1956-52c5-4261-8008-aa3a8450e294.jpg" />, and a subset <img src="2-2340075\6b89dee1-6978-4807-9bdf-9e97b9c06839.jpg" />of<img src="2-2340075\852afec8-7879-4ae2-9b3c-18d38019a928.jpg" />, such that for each <img src="2-2340075\d6e3ecd0-df91-4da3-be00-1ed24b68e49e.jpg" /> there exists a unique solution <img src="2-2340075\7051c428-3767-4cc5-825e-b6085382c147.jpg" /> to the Equation (1.3), and furthermore, the map <img src="2-2340075\7f4830cc-3a58-4737-aba8-cbb1122dd458.jpg" /> is continuous from<img src="2-2340075\0c985ecc-cf66-4d44-ae2f-3fc0a1e2cf62.jpg" />. If <img src="2-2340075\81c1fec8-686e-4e49-8fdf-9ffbbab16a54.jpg" /> can be taken arbitrarily large<img src="2-2340075\67ce3b2e-5a26-438e-82bc-2386eff07c18.jpg" />, the problem is globally wellposed.</p><p>Definition 1.3 A global solution <img src="2-2340075\4ac2bf35-490b-40af-8fe3-f33dee5fba8e.jpg" /> to (1.1) is scattering in <img src="2-2340075\61014467-e300-4b1a-a4f3-e5d3a178600e.jpg" /> as <img src="2-2340075\5ce6ff23-c16c-495d-a223-80b6ff8f485c.jpg" /> if there exists <img src="2-2340075\1e1f7baa-7b45-42a5-8512-81d534657a4a.jpg" /> such that</p><p><img src="2-2340075\bf9519c1-c2b7-48bc-928a-cc4531c36b12.jpg" /></p><p>Similarly, we can define scattering in <img src="2-2340075\a90dbf96-d3d7-448a-ad9b-148af539ec12.jpg" /> for<img src="2-2340075\04fc2754-2d69-4750-818c-d9bf21e1f457.jpg" />.</p><p>For more definition of critical case see [1-3].</p><p>In this paper we discuss stability theory of the mass critical, mass-supercritical and energy-subcritical of solution to the nonlinear Schr&#246;dinger equation. In section three we discuss the stability of the mass critical solutions and in section four mass-supercritical and energysub-critical solutions are discussed.</p><p>Theorem 1.1 Let <img src="2-2340075\a1a3b8d7-c74e-49c9-b9a3-18637756407e.jpg" /> and<img src="2-2340075\b0878b12-0cff-4b3b-9c19-4ba9698a166f.jpg" />. Then there exists a unique maximal-lifespan solution <img src="2-2340075\c7f0b567-46e0-4ec5-a2c4-b6ff7d3bdc4f.jpg" /> <img src="2-2340075\f07051da-7363-4dad-89a6-58412fd536e4.jpg" />&#160;to (1.1) with <img src="2-2340075\12263edc-ebad-4dfd-8683-7a880383ada6.jpg" /> and initial data<img src="2-2340075\0be2748c-cb15-4147-a547-c65430c44b5f.jpg" />. Moreover:</p><p>1) The interval <img src="2-2340075\7127720d-7c29-4b26-b5d9-57b00c5072dd.jpg" /> is an open subset of<img src="2-2340075\edcdfa52-0e33-4a74-a2bc-f8f23c34911f.jpg" />.</p><p>2) For all<img src="2-2340075\25f43993-eaab-48e0-804f-6e28db68256a.jpg" />, we have <img src="2-2340075\c97dbb9b-da3e-4967-9399-805e2ebdf0c6.jpg" /> so, we deﬁne<img src="2-2340075\fd19007b-5262-411e-9654-3a979c14a993.jpg" />.</p><p>3) If the solution <img src="2-2340075\dd1a754c-e89f-4405-abca-c352ee720479.jpg" /> does not blow up forward in time, then<img src="2-2340075\157c8a84-8061-42b5-940c-60f984361229.jpg" />, and moreover <img src="2-2340075\df5548e0-f377-493a-9284-85d358b0fdf2.jpg" /> scatters forward in time to <img src="2-2340075\17937434-6bc6-434e-93db-65bacbc0b3ed.jpg" /> for some<img src="2-2340075\9099beed-2c2c-4343-bc25-caf3c354e5b4.jpg" />. Converselyif <img src="2-2340075\56019fc1-8949-4c9b-9888-687be766809b.jpg" /> then there exists a unique maximallifespan solution <img src="2-2340075\a428581e-a46d-4f52-813e-46f22d0de353.jpg" /> which scatters forward in time to<img src="2-2340075\4b0585f7-4fa1-41f3-bb79-9ba821c83784.jpg" />.</p><p>4) If the solution u does not blow up backward in time, then <img src="2-2340075\8f1503d9-5fa2-452f-ab53-2bdf092090dd.jpg" /> and moreover <img src="2-2340075\63d6412c-0c7e-45f0-b76d-fd52126f50d6.jpg" /> scatters backward in time to <img src="2-2340075\438a5226-0eef-4d03-8e20-20ccc2e218ea.jpg" /> for some<img src="2-2340075\8d040934-d995-4dff-a6f3-36f57484885c.jpg" />. Conversely, if</p><p><img src="2-2340075\1754564f-e2fa-4dbb-b0f2-3f7e24743ddd.jpg" />then there exists a unique maximallifespan solution <img src="2-2340075\b982bd14-2668-46d4-ba77-8498a5a0b7ec.jpg" /> which scatters backward in time to<img src="2-2340075\b98c177a-c978-4697-9b14-668ab65be83b.jpg" />.</p><p>5) If <img src="2-2340075\694af8cb-42d3-4cee-98f4-fc7ff12d0a18.jpg" /> where a constant <img src="2-2340075\53ec75ed-8363-4307-bc20-0c65c6f12954.jpg" /> depending only on <img src="2-2340075\7c3aecea-db79-4401-8290-df2d6ff643ae.jpg" /> then</p><p><img src="2-2340075\cbd0ac36-60ed-4d64-81a5-3d9fd3b68172.jpg" />.</p><p>In particular, no blowup occurs and we have global existence and scattering both ways.</p><p>6) For every <img src="2-2340075\38d091a2-045b-4d18-9210-f7d0fc23f2dc.jpg" /> and <img src="2-2340075\3f3de451-43c9-4b9e-92ac-df247e2417f1.jpg" /> there exists <img src="2-2340075\52740ac3-d7e8-4527-949c-a735a9d70d2b.jpg" /> With property: if <img src="2-2340075\6f29ef3b-158e-40c0-b476-bcbdc2faa931.jpg" /> is a solution (not necessarily maximal-lifespan) such that</p><p><img src="2-2340075\b311470d-17cc-4203-84ba-83c718a0b77a.jpg" />and<img src="2-2340075\d7265660-c898-4e26-8b41-79cc9d1017cd.jpg" />, <img src="2-2340075\fffdc22c-f3a2-478b-970e-fae90ea8a35b.jpg" />are such that<img src="2-2340075\aa790ce6-42af-42dc-a438-fed6df49570d.jpg" />, then there exists a solution</p><p><img src="2-2340075\ab7cb1a1-3a51-46ac-a1e8-dd70edb08491.jpg" />with <img src="2-2340075\0167034d-0a8f-4260-9a6a-04b4b1cf5713.jpg" /> such that <img src="2-2340075\05a36f39-e3f6-4290-8684-e9927cab56c2.jpg" /></p><p>and <img src="2-2340075\cf11e1c2-b376-4ce1-adf3-a8f233b79b19.jpg" /> for all<img src="2-2340075\060b7390-dfc1-475e-af0a-400ce3399868.jpg" />.</p><p>For proof: See [4-6].</p><p>Now in the following we will discuss Standard local well-posedness theorem.</p><p>Theorem 1.2 Let<img src="2-2340075\7ad3c03f-8be3-4d3c-b5f8-b9b42831e779.jpg" />, <img src="2-2340075\f3234221-2ef5-4a57-9493-7b93cd10d5f1.jpg" />and let</p><p><img src="2-2340075\a1694b23-6176-420a-975e-0fb486f1537c.jpg" />Assume that <img src="2-2340075\e217c44d-abf4-46bb-8b9c-de6f6ffe123a.jpg" /> if <img src="2-2340075\c8dd5508-9182-4b50-97c2-20b7a9791a87.jpg" /> is not an even integer. Then there exists <img src="2-2340075\20d53076-75bc-42f3-81d9-5fb3b19c9119.jpg" /> such that if between <img src="2-2340075\ae533554-46df-4bb0-9520-22646de70184.jpg" /> and <img src="2-2340075\7c81cef8-3428-482b-937f-a00ee957940a.jpg" /> there is a compact interval containing zero such that</p><disp-formula id="scirp.32976-formula55491"><label>(1.4)</label><graphic position="anchor" xlink:href="2-2340075\d6665820-d847-4618-84be-5d628526c268.jpg"  xlink:type="simple"/></disp-formula><p>then there exists a unique solution u to (1.1) on<img src="2-2340075\c48db2ad-a97d-43d4-be0c-6492d17bce42.jpg" />. Furthermore, we have the bounds</p><disp-formula id="scirp.32976-formula55492"><label>(1.5)</label><graphic position="anchor" xlink:href="2-2340075\3b1de2e0-ad84-4b03-a2ba-35ab19c57317.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.32976-formula55493"><label>(1.6)</label><graphic position="anchor" xlink:href="2-2340075\06b8df5c-5a56-4cdf-9477-2245275583f4.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.32976-formula55494"><label>(1.7)</label><graphic position="anchor" xlink:href="2-2340075\0506c121-c0b6-48e4-b72d-e91884416593.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="2-2340075\1c2774a4-ab75-4954-8510-ad99579e0d9c.jpg" /> for the closure of all test functions under this norm.</p></sec><sec id="s2"><title>2. Strichartz Estimate</title><p>In this section we discus some notation and Strichartz estimate.</p><sec id="s2_1"><title>2.1. Some Notation</title><p>We write <img src="2-2340075\83735c5b-1e1f-46b8-9cb4-f1803d69fd8c.jpg" /> anywhere in this work whenever there exists a constant <img src="2-2340075\be541746-f770-4025-ba9b-d58e857dec67.jpg" /> independent of the parameters, so that<img src="2-2340075\e1fa45a7-e76e-4d71-a9e3-1063d6d1d068.jpg" />. The shortcut <img src="2-2340075\e41d527b-f631-4652-9d54-69341abb5816.jpg" /> denotes a finite linear gathering of terms that “look like” X, but possibly with some factors changed by their complex conjugates.</p><p>We start by the definition of space-time norms</p><p><img src="2-2340075\f22ef946-1878-435f-96fd-12c4973ac725.jpg" /></p><p>The inhomogeneous Sobolev norm <img src="2-2340075\ff74ca23-82ed-4215-9ea3-e69ab96b1c75.jpg" />(when <img src="2-2340075\b1a5d1f3-453f-428a-8aa3-3dcadb1692db.jpg" /> is an integer) is defined by:</p><p><img src="2-2340075\e7aad18a-17a7-4cee-b8b1-3dd6a0265f10.jpg" /></p><p>When s is any real number as</p><p><img src="2-2340075\f618cb4c-fc96-4bf2-a8b7-340817fb81dc.jpg" /></p><p>The homogeneous Sobolev norm <img src="2-2340075\b1e93790-7aab-4793-acb8-c1525ed776b7.jpg" /> defines as:</p><p><img src="2-2340075\c7346c9f-0d72-44b8-950a-3b9d51d277a6.jpg" /></p><p>For any space time slab<img src="2-2340075\954a8fa6-8aa9-4f2f-8a05-e8054fd3e986.jpg" />We use <img src="2-2340075\dc9e67ef-7321-4ab1-98ac-388c501ae122.jpg" /> to denote the Banach space of function <img src="2-2340075\a493ee62-e730-4814-8580-94c17603709e.jpg" /> whose norm is</p><p><img src="2-2340075\04ec9856-9439-4d20-bfd8-13916aa31d2f.jpg" /></p><p>With the usual adjustments when <img src="2-2340075\b668fec6-03ec-490b-aa49-90bfa9311b82.jpg" /> or <img src="2-2340075\8c7a444e-e930-48b2-8fe7-15ef93bdf04b.jpg" /> is equal to infinity. When <img src="2-2340075\0676a2d7-9891-4849-9c5d-febf926946ed.jpg" /> we abbreviate <img src="2-2340075\b7596455-39f8-44b7-9538-b94561fd46ed.jpg" /> as<img src="2-2340075\f4cf29a0-efd9-4202-b18b-8b7cee85ff69.jpg" />.</p><p>A Gagliardo-Nirenberg type inequality for Schr&#246;- dinger equation the generator of the pseudo conformal transformation <img src="2-2340075\be6b3670-f99c-473a-b33e-6e08eed5d408.jpg" /> plays the role of partial differentiation.</p></sec><sec id="s2_2"><title>2.2. Strichartz Estimate</title><p>Definition 2.1 The exponent pair <img src="2-2340075\60eb982e-6184-451a-821e-944870276c18.jpg" /> is says the Schr&#246;dinger-admissible if</p><p><img src="2-2340075\67923275-325b-4a26-828c-a9daf0ea270e.jpg" />, and <img src="2-2340075\f1b04605-5726-441d-81fa-4f1c37aa7195.jpg" /></p><p><img src="2-2340075\a9f61876-b94b-4fa5-bbb5-9ad3316e4e81.jpg" /></p><p>Definition 2.2 The exponent pair <img src="2-2340075\6ec6e327-6f1a-4aad-99a7-1275bf77beb3.jpg" /> is says the Schr&#246;dinger-acceptable if</p><p><img src="2-2340075\d0a2ca64-40a4-4d4a-953f-ef716fa15c1d.jpg" /></p><p>Let <img src="2-2340075\fbdc0954-e144-46e1-a3fd-e2708e708aed.jpg" /> be the free Schr&#246;dinger evolution. From the explicit formula</p><p><img src="2-2340075\d5207192-71b0-4266-b8e8-e9706a1045d4.jpg" /></p><p>we obtain the standard dispersive inequality</p><disp-formula id="scirp.32976-formula55495"><label>(2.1)</label><graphic position="anchor" xlink:href="2-2340075\4c11266f-cd2c-4d73-a100-0c7326c0ac52.jpg"  xlink:type="simple"/></disp-formula><p>for all<img src="2-2340075\32c910bc-32a3-4e8e-8fe4-f2f321be52ce.jpg" />.</p><p>In particular, as the free propagator conserves the <img src="2-2340075\fbf78113-d8a9-4d7f-b186-6e4ef4ba61de.jpg" />- norm,</p><disp-formula id="scirp.32976-formula55496"><label>(2.2)</label><graphic position="anchor" xlink:href="2-2340075\0aeb12f6-fc64-4b69-bbaa-845e0e81f679.jpg"  xlink:type="simple"/></disp-formula><p>For all <img src="2-2340075\f4f38f00-cdab-4552-a1dc-bb507eede20d.jpg" /></p><p><img src="2-2340075\d5f5937e-17f4-44a0-a380-5aaee53ed1eb.jpg" /></p><p>If <img src="2-2340075\9606e18b-d6d9-4680-b3ed-117fa4c8d13e.jpg" /> solves the inhomogeneous Equation (1.1) for some</p><p><img src="2-2340075\3ceb1f61-8452-496b-b8b3-639251c7e182.jpg" />and <img src="2-2340075\0fb58248-6ae5-42c1-8e20-4e6d4b90b48b.jpg" /></p><p>in the integral.</p><p>Duhamel (1.3). Then we have</p><disp-formula id="scirp.32976-formula55497"><label>(2.3)</label><graphic position="anchor" xlink:href="2-2340075\e5dfd6b8-3e89-4d6a-bb5a-cf88e277d174.jpg"  xlink:type="simple"/></disp-formula><p>for some constant <img src="2-2340075\ed3d4359-7cc9-485d-9c45-0306ead848d6.jpg" /> depending only on the dimension<img src="2-2340075\e842fe39-8c49-4993-93f7-440f438604a6.jpg" />.</p><p>For some constant <img src="2-2340075\fa5e283c-3dc3-48b0-b302-ac01475e1c7c.jpg" /> depending only on <img src="2-2340075\dbc2c4b4-32a9-4a4c-86a7-a870c4e40421.jpg" /> we have the Holder inequality</p><p><img src="2-2340075\32cec1b4-55e8-4a28-ac75-79f0da1e3355.jpg" /></p><p>We now return to prove Theorem 1.2.</p><p>Proof Theorem 1.2 The theorem follows from a contraction mapping argument. More accurate, defined</p><p><img src="2-2340075\fc61057e-5ee9-47d4-984e-03883c99635a.jpg" /></p><p>using the Strichartz estimates, we will show that the map <img src="2-2340075\1d32a6cd-94f2-463a-b439-3c00360d260b.jpg" /> is a contraction on the set <img src="2-2340075\2e4efbf8-5323-493e-ac1b-8c000c462387.jpg" /> where</p><p><img src="2-2340075\a3fd418e-6051-4583-aee3-08d3ba499a47.jpg" /></p><p><img src="2-2340075\62c4df47-e998-4be8-b482-3554d108066d.jpg" /></p><p>under the metric given by</p><p><img src="2-2340075\75c1c34a-dad9-477a-9a55-ba8761f9ee76.jpg" /></p><p>Here <img src="2-2340075\24852c8e-af7e-403f-9dd4-9b78ad1774d6.jpg" /> denotes a constant that changes from line to line. Note that the norm appearing in the metric scales like<img src="2-2340075\41705356-fac0-4a1a-aa92-9562b396aa49.jpg" />. Note also that both <img src="2-2340075\c5a425c1-c6b9-435c-8000-9a4ea9ee0ec3.jpg" /> and <img src="2-2340075\e9cf2979-296f-4719-af89-397d56d32375.jpg" /> are closed (and hence complete) in this metric.</p><p>Using the Strichartz inequality and Sobolev embedding, we find that for <img src="2-2340075\229b5b48-0fc2-47b4-a27f-eeda5dbe240e.jpg" /></p><p><img src="2-2340075\20a7562c-f124-45f5-8bfb-fd9ccdb9561e.jpg" /></p><p>And similarly,</p><p><img src="2-2340075\6fe72511-5a4c-435b-99ae-d5fc43a3391a.jpg" /></p><p>Arguing as above and invoking (1.4), we obtain</p><p><img src="2-2340075\664de217-768f-4dfd-a215-93a8b245028b.jpg" /></p><p>Thus, choosing <img src="2-2340075\c310ae59-96c5-410b-804e-a627a3d8a705.jpg" /> suciently small, we see that for<img src="2-2340075\853fd7e4-a9f6-422e-aab4-e56a87926877.jpg" />, the functional <img src="2-2340075\a5ef0c2c-c144-4017-9d15-ff5af7b82c90.jpg" />&#160;maps the set <img src="2-2340075\e671a4b9-3425-4f9a-9994-785e08bb0dda.jpg" /> back to itself. To see that <img src="2-2340075\5301a981-2396-4b3c-887f-aaae76ed8160.jpg" /> is a contraction, we repeat the above calculations to obtain</p><p><img src="2-2340075\6cedcca4-2a02-4312-bef1-ec43d7541053.jpg" /></p><p>Therefore, choosing <img src="2-2340075\8e182453-dc67-4e25-94a1-d5b3f5e971c2.jpg" /> even smaller (if necessary), we can ensure that <img src="2-2340075\7b58af35-c559-4661-b69d-0543343a32ea.jpg" /> is a contraction on the set<img src="2-2340075\a07642c7-171e-4686-9cf8-a49f351f2b65.jpg" />. By the contraction mapping theorem, it follows that <img src="2-2340075\e4223369-d1e8-4449-87ad-b29c68dacbf2.jpg" /> has a fixed point in<img src="2-2340075\3481541b-ec4d-48e9-97c9-df78f21fc4fb.jpg" />. Furthermore, noting that <img src="2-2340075\3c1da4fc-240c-4af6-964e-c381d6f7a98e.jpg" /> maps into <img src="2-2340075\d8a1c953-ae17-4c25-bb3e-b5c16aa6545c.jpg" /> (not just<img src="2-2340075\7ad36e05-b481-43ed-9b63-e0996b079d4f.jpg" />). We now turn our attention to the uniqueness. Since uniqueness is a local property, it enough to study a neighbourhood of <img src="2-2340075\3e287909-78e1-4d7d-8245-0807ed4abf32.jpg" /> By Deﬁnition of solution (and the Strichartz inequality), any solution to (1.1) belongs to <img src="2-2340075\53ccb76b-393c-45ce-ae87-0a74a8980794.jpg" /> on some such neighbourhood. Uniqueness thus follows from uniqueness in the contraction mapping theorem.</p><p>The claims (1.6) and (1.7) follow from another application of the Strichartz inequality. □</p><p>Remark 2.1 By the Strichartz inequality, we know that</p><p><img src="2-2340075\9880dc76-5f12-48d8-a7e0-c2e7001108d9.jpg" /></p><p>Thus, (1.4) holds with <img src="2-2340075\a105df19-bf7d-44c0-88d7-82751a97c2d7.jpg" /> for initial data with suciently small norm instead that, by the monotone convergence theorem, (1.4) holds provided <img src="2-2340075\2c760ade-9639-4de7-8976-e6812cdbccce.jpg" /> is chosen suciently small. Note that by scaling, the length of the interval <img src="2-2340075\b2c87561-5b86-4125-98f7-705cb01f5261.jpg" /> depends on the fine properties of<img src="2-2340075\5a3e867f-5ddb-4dbf-8008-c321edfadb66.jpg" />, not only on its norm.</p></sec></sec><sec id="s3"><title>3. Stability of the Mass Critical</title><p>In this section we discuss the stability theory at mass critical case. Consider the initial-value problem (1.1)</p><p>with <img src="2-2340075\7d6d8ee7-3915-4471-9030-754c38ede380.jpg" /> .An important part of the local well-posedness theory is the study of how the strong solutions built in the past subsection depend upon the initial data. More accurate, we want to know if the small perturbation of the initial data gives small changes in solution. In general, we take care in developing a stability theory for nonlinear Schr&#246;dinger Equation (1.1). Even though stability is a local question, it plays an important role in all existing treatments of the global well-posedness problem for nonlinear Schr&#246;dinger equation at critical case, for more see [<xref ref-type="bibr" rid="scirp.32976-ref7">7</xref>]. It has also proved useful in the treatment of local and global questions for more exotic nonlinearities [8,9]. In this section, we will only discus the stability theory for the mass-critical NLS.</p><p>Lemma 3.1 Let <img src="2-2340075\8719bbce-b880-4230-96c1-bdc5b14c29b6.jpg" /> be a compact interval and let <img src="2-2340075\fa706d29-d36e-4b1e-abf3-165981f2cccd.jpg" />be an approximate solution to (1.1) meaning that</p><p><img src="2-2340075\a3eccfc1-3246-4293-a6ca-8f152e897511.jpg" /></p><p>for some function<img src="2-2340075\5d345e73-c81e-46bf-bb35-dba2fa938fe9.jpg" />. Suppose that</p><disp-formula id="scirp.32976-formula55498"><label>(3.1)</label><graphic position="anchor" xlink:href="2-2340075\f4951479-a90f-4568-ad08-b39b6ddabc40.jpg"  xlink:type="simple"/></disp-formula><p>for some positive constant<img src="2-2340075\4a55227a-4ff9-4c1e-a557-194be05f17ae.jpg" />. Let <img src="2-2340075\2362e105-d24f-4b7c-b31a-e087d60622f1.jpg" /> and let <img src="2-2340075\c4d413e9-013c-4975-80f6-63012003edb4.jpg" /> be such that</p><disp-formula id="scirp.32976-formula55499"><label>(3.2)</label><graphic position="anchor" xlink:href="2-2340075\8771cf49-d42b-48ca-8125-9004e1f1a17f.jpg"  xlink:type="simple"/></disp-formula><p>for some<img src="2-2340075\e39b1a75-8542-4b57-a9a0-c0a05e036d21.jpg" />. Suppose also the smallness conditions</p><disp-formula id="scirp.32976-formula55500"><label>(3.3)</label><graphic position="anchor" xlink:href="2-2340075\0503d3a0-9335-41b1-b92d-5d70e1fc8b19.jpg"  xlink:type="simple"/></disp-formula><p><img src="2-2340075\6ea26d37-26f1-4025-81d9-446db9166ca1.jpg" /> &#160;&#160;&#160;(3.4) <img src="2-2340075\8e429565-703c-468a-bf9b-589c013e6905.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;(3.5)</p><p>for some <img src="2-2340075\a246974d-1c77-42a0-a197-d48e24cdf1d8.jpg" />&#160; where <img src="2-2340075\f0f2b8fa-caec-4e3e-8346-3c7c30f278f8.jpg" /> is a small constant. Then, there exists a solution <img src="2-2340075\bbad31d1-1706-4232-9876-98257ad7ad12.jpg" /> to (1.1) on <img src="2-2340075\12316054-0a5d-416f-8359-afa65ebb6d6a.jpg" /> with initial data <img src="2-2340075\7b863ea9-2ee8-4c9a-86ad-fda2e0270168.jpg" /> at time <img src="2-2340075\d8f7ac32-d876-4f8b-a273-b4a2cc4ead2e.jpg" /> satisfying</p><disp-formula id="scirp.32976-formula55501"><label>(3.6)</label><graphic position="anchor" xlink:href="2-2340075\293af81a-489c-4688-a6c1-bcc971633fec.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.32976-formula55502"><label>(3.7)</label><graphic position="anchor" xlink:href="2-2340075\49bd86f5-064a-4db7-9688-08a66ecaf1f7.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.32976-formula55503"><label>(3.8)</label><graphic position="anchor" xlink:href="2-2340075\55a060df-95dd-4e81-85b1-ec6e600e7cfe.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.32976-formula55504"><label>(3.9)</label><graphic position="anchor" xlink:href="2-2340075\d5f09f2e-841b-4a31-8c7a-d3e80ab916ec.jpg"  xlink:type="simple"/></disp-formula><p>Proof: By symmetry, we may assume<img src="2-2340075\2a6819b0-facc-471f-8fc2-372905bdd852.jpg" />. Let<img src="2-2340075\69065c2c-1c94-478f-bbbc-88d46145da9e.jpg" />. Then <img src="2-2340075\76be5305-b3e1-4904-a815-e0fa9d987aba.jpg" /> satisfies the initial value problem</p><p><img src="2-2340075\94e9d896-c11b-4d6d-9c31-3b948a6ec78e.jpg" /></p><p>For <img src="2-2340075\5d0ac9f4-69b7-423a-8c07-6e76c11285a5.jpg" /> we define</p><p><img src="2-2340075\8a9120a1-8c44-4876-95c1-cc3877068f7b.jpg" /></p><p>By (3.3),</p><disp-formula id="scirp.32976-formula55505"><label>(3.10)</label><graphic position="anchor" xlink:href="2-2340075\137b852d-946c-4d15-9899-919ca5631d80.jpg"  xlink:type="simple"/></disp-formula><p>Furthermore, by Strichartz, (3.4), and (3.5), we get</p><disp-formula id="scirp.32976-formula55506"><label>(3.11)</label><graphic position="anchor" xlink:href="2-2340075\fe0957c9-91e6-4326-b419-c03e76b575e7.jpg"  xlink:type="simple"/></disp-formula><p>Combining (3.10) and (3.11), we obtain</p><p><img src="2-2340075\87c3f384-931b-4871-843d-3bd772d2f169.jpg" /></p><p>A standard continuity argument then shows that if <img src="2-2340075\328adb28-7535-4063-b6bb-1a291f0bd935.jpg" /> is taken sufficiently small,</p><p><img src="2-2340075\307d0fcf-f69c-4d5c-b85f-981c098d8eb5.jpg" /></p><p>which implies (3.9). Using (3.9) and (3.11), we obtained (3.6). Furthermore, by Strichartz, (3.2), (3.5), and (3.9),</p><p><img src="2-2340075\aa340516-52ad-4e31-be2a-ea48b2bfdc40.jpg" /></p><p>which establishes (3.7) for <img src="2-2340075\e38183f7-8b4c-44a8-98eb-03d498d4fb53.jpg" /> sufficiently small.</p><p>To prove (3.8), we use Strichartz, (3.1), (3.2), (3.9), and (3.3):</p><p><img src="2-2340075\9dedf9c1-9c6f-47f2-9b5d-c1bd0a837e32.jpg" /></p><p>Choosing <img src="2-2340075\95c01a2c-67b2-4d60-b360-e5c8a1ad7224.jpg" /> sufficiently small, this finishes the proof. □</p><p>Based on the previous result, we are now able to prove stability for the mass-critical NLS.</p><p>Theorem 3.2 Let <img src="2-2340075\1a12f257-c66e-4ac6-8d1c-9d28250ccb41.jpg" /> be a compact interval and let <img src="2-2340075\b18c7664-ef79-4acc-8d55-07191b8ba53c.jpg" /> be an approximate solution to (1.1) in the sense that</p><p><img src="2-2340075\944e0eae-900e-4a51-86d0-bb6fea4ac792.jpg" /></p><p>for some function<img src="2-2340075\946c2e23-bac6-48ff-84aa-0c148da1f33d.jpg" />. Assume that condition (3.1) in Lemma 3.1 holds and</p><disp-formula id="scirp.32976-formula55507"><label>(3.12)</label><graphic position="anchor" xlink:href="2-2340075\c940bfbe-e3e4-4be3-bd2b-a3c5eaae3a9e.jpg"  xlink:type="simple"/></disp-formula><p>for some positive constant<img src="2-2340075\595852aa-dc3b-453c-9337-d24e651642f3.jpg" />. Let <img src="2-2340075\1f7b4284-f3e6-42b1-b1ec-c75d24ebe524.jpg" /> and let <img src="2-2340075\faa87bd3-cbf7-43fb-b9be-f7cd52269fca.jpg" /> obey (3.2) for some<img src="2-2340075\3e70c224-b471-455a-8755-74de5d2bcb7a.jpg" />. Furthermore, suppose the smallness conditions (3.4), (3.5) in Lemma 3.1. For some <img src="2-2340075\5ea5bb4e-7729-4360-b80d-0e1b2b58baf6.jpg" /> where</p><p><img src="2-2340075\f8687a66-b96c-4b5e-80d7-6ee9a3789d9f.jpg" />is a small constant. Then, there exists a solution <img src="2-2340075\5a4e377e-8a66-4cb2-9b98-707fda4407d5.jpg" /> to (1.1) on <img src="2-2340075\52bcd257-e372-48b3-a7ca-fa177db44066.jpg" /> with initial data <img src="2-2340075\ac4e0d49-85e6-4f92-b4df-e1f8b2e0dcde.jpg" /> at time <img src="2-2340075\2c22d1ad-96d4-45bf-a4c6-7438220907f1.jpg" /> satisfying</p><disp-formula id="scirp.32976-formula55508"><label>(3.13)</label><graphic position="anchor" xlink:href="2-2340075\07955b0a-e929-4505-8fc3-2929f9e24a0c.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.32976-formula55509"><label>(3.14)</label><graphic position="anchor" xlink:href="2-2340075\f02c8389-c35f-4ee8-9b15-9a0c745931b6.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.32976-formula55510"><label>(3.15)</label><graphic position="anchor" xlink:href="2-2340075\e7d57d7e-4453-4d69-8fab-c7e40b921214.jpg"  xlink:type="simple"/></disp-formula><p>Proof: Subdivide <img src="2-2340075\e17e4cb6-80dc-422a-90e0-86615db9b59c.jpg" /> into <img src="2-2340075\a159aa68-ad20-4d38-b4e3-e82064a065e5.jpg" /> subintervals <img src="2-2340075\be856ef9-8fb1-4a9d-ba46-370407dacc87.jpg" /> such that</p><p><img src="2-2340075\5762483f-f60c-4181-ba33-4a88a1ce88ac.jpg" /></p><p>where <img src="2-2340075\0b773f96-1292-4f23-acb3-6e29a6ba1fd9.jpg" /> is as in Lemma 3.1. We replaced <img src="2-2340075\5b44c154-99fc-451c-bf5c-99751d69a9e7.jpg" /> by <img src="2-2340075\aa054588-6e2b-45db-b1dc-c4eca02c90af.jpg" /> as the mass of the difference <img src="2-2340075\c61e04ab-4ced-42b7-80f0-d7aaf431aac5.jpg" /> might grow slightly in time. By choosing <img src="2-2340075\9fd3cc33-9fa0-4f71-ac1f-495faafdd442.jpg" /> sufficiently small depending on <img src="2-2340075\139a5105-9382-44e8-be2f-873182595d28.jpg" />and<img src="2-2340075\16a03a1a-bc68-4406-9865-d68b984607be.jpg" />, we can apply Lemma 3.1 to obtain for each <img src="2-2340075\c62fd6f0-919c-46c6-96e3-4ac45b3b3d3c.jpg" /> and all <img src="2-2340075\4b8f149b-ad90-42d4-b210-05bd2f8e50c1.jpg" /></p><p><img src="2-2340075\e501b3e6-3d4b-407e-97b4-f497258b1ae4.jpg" /></p><p><img src="2-2340075\1a427fa5-b880-4712-b24d-404304dce9d0.jpg" /></p><p><img src="2-2340075\c2c87f64-a85f-42b5-9b62-b2f38320b43c.jpg" /></p><p><img src="2-2340075\b2469642-92b6-4bad-a3d6-76002a21ec81.jpg" /></p><p>Provided, we can prove that their counterparts of (3.2) and (3.4) hold with replace <img src="2-2340075\eec60cd0-f717-43ba-9f05-2afd3d04913d.jpg" /> by<img src="2-2340075\6ca5c8fc-ce07-4b8d-a57b-76c246976f97.jpg" />. To verify this, we use an inductive argument. By Strichartz, (3.2), (3.5), and the inductive hypothesis,</p><p><img src="2-2340075\2c80fdb5-b7bd-450b-ab24-ec024853dbc8.jpg" /></p><p>Similarly, by Strichartz, (3.4), (3.4), and the inductive hypothesis,</p><p><img src="2-2340075\aed1d24d-89dc-4a8e-89c6-1dc9e122f669.jpg" /></p><p>Choosing <img src="2-2340075\403c2e99-9397-4502-8952-d1c78a1adb05.jpg" /> sufficiently small depending on <img src="2-2340075\94eebb14-f5a4-438b-9199-9a0c9b4b2890.jpg" /> and<img src="2-2340075\f6e5e820-0849-43d2-bf77-129cba47bc19.jpg" />, we can ensure that hypotheses of Lemma 3.1 continue to hold as j varies. □</p><p>Lemma 3.3 (Stability) Fix <img src="2-2340075\5ab625a3-bacf-4cd3-91a5-fb8a5e2a6fbd.jpg" /> and<img src="2-2340075\50f07835-89ed-406c-a3fc-56c9f885eba8.jpg" />. For every <img src="2-2340075\bf811186-e523-415c-82ad-c21d41ed44e8.jpg" /> and <img src="2-2340075\d40896d2-235f-44f7-ad39-8f352a02a7c5.jpg" /> there exists <img src="2-2340075\ad08951f-959b-4ba8-bcb0-361a9e3fa570.jpg" /> with the property: if <img src="2-2340075\72a59ac7-f8dc-4a81-a66b-a6424e739c1f.jpg" /> is such that <img src="2-2340075\4982a67d-fb6d-425c-ac89-b658b4438973.jpg" /> and that <img src="2-2340075\266c13c0-e8ef-435d-8b0d-1e16b8b8bcfc.jpg" /> approximately solves (1.1) in the sense that</p><disp-formula id="scirp.32976-formula55511"><label>. (3.16)</label><graphic position="anchor" xlink:href="2-2340075\7557fe14-548c-4b12-8dc0-764379069604.jpg"  xlink:type="simple"/></disp-formula><p>And<img src="2-2340075\9ab44ffe-7d2f-41a6-9719-e233cad89b89.jpg" />, <img src="2-2340075\e4da618d-938c-489e-a36d-011448d7ac2a.jpg" />are such that</p><p><img src="2-2340075\90ae8852-c65e-4f68-b5b2-decfa6c0b661.jpg" /></p><p>Then there exists a solution <img src="2-2340075\c4637d43-1c97-441a-9ff8-ba98de20fb12.jpg" /> to (1.1) with <img src="2-2340075\0c894de2-b967-4e11-9a7f-47dbdd6b0756.jpg" /> such that</p><p><img src="2-2340075\23a129b2-c262-4092-a9f9-3ceabdc3730d.jpg" />.</p><p>Note that, the masses of <img src="2-2340075\b25ccb3b-e421-466c-85e7-b3d70f813bb5.jpg" /> and <img src="2-2340075\8fc783ad-f0ed-4282-a780-52828ecd9608.jpg" /> do not appear immediately in this lemma, although it is necessary that these masses are ﬁnite. Similar stability results for the energy-critical NLS (in<img src="2-2340075\8ba0284e-a0d9-48e9-a22f-c0004d4846f2.jpg" />) instead of<img src="2-2340075\709bf676-cf29-49a1-828b-37c22e5a1968.jpg" />, of course) have appeared in [10-14]. The mass-critical case it is actually slightly simpler as one does not need to deal with the existence of a derivative in the regularity class. For more see [<xref ref-type="bibr" rid="scirp.32976-ref15">15</xref>].</p><p>Proof: (Sketch) First let prove the claim when <img src="2-2340075\b9468d29-7122-4cc8-95dc-420b951916e6.jpg" /> is suciently small depending on<img src="2-2340075\62dc7bca-9842-47e3-ba17-e3c8d2a12fc6.jpg" />. Let <img src="2-2340075\ddf7928d-b959-4257-aba4-08d0b498350c.jpg" /> be the maximal-lifespan solution with initial data<img src="2-2340075\0b65d51f-c467-4b23-a80f-372b325cd961.jpg" />. Writing <img src="2-2340075\a87e25f3-3230-4574-8bdb-d419d5cd6c96.jpg" /> on the interval<img src="2-2340075\c6678bab-ded6-4702-acf2-b66934911329.jpg" />, we see that</p><p><img src="2-2340075\852aecd8-39bb-4465-8a89-fce3d8da77f7.jpg" /></p><p>and</p><p><img src="2-2340075\63628ca9-368d-4172-96e5-b1187ab47699.jpg" />.</p><p>Thus, if we set</p><p><img src="2-2340075\ac169c51-2773-4f8c-a853-9afe7a9cb66a.jpg" /></p><p>by the triangle inequality, (2.3), and (3.16), we have</p><p><img src="2-2340075\38943ea3-8fc6-4b40-b7fb-573d55283069.jpg" /></p><p>hence, by (2.4) and the hypothesis<img src="2-2340075\d4390c01-e483-4897-a60b-0c9c2ce254d7.jpg" />,</p><p><img src="2-2340075\ef118d37-c854-4449-94ac-15f8e6c5b625.jpg" /></p><p>where <img src="2-2340075\ba7ddd80-c4a3-4da5-8193-34237ce35e20.jpg" /> depends only on<img src="2-2340075\3156a5a9-1b9c-4d5f-b0c4-d9307699ae48.jpg" />. If <img src="2-2340075\26d66599-1af4-4ad7-8282-75f81c06afc2.jpg" /> is suciently small depending on<img src="2-2340075\deaef323-e525-43f6-93e2-ff1df08e834b.jpg" />, and <img src="2-2340075\a1634714-63f2-4ca6-b9c4-f0d3611d52ba.jpg" /> is suciently small depending on <img src="2-2340075\c3493882-0e11-4dc0-a9fd-42839a2b812b.jpg" /> and<img src="2-2340075\6cbfe4d2-6e61-4789-aa38-e4c941ad0930.jpg" />, then standard continuity arguments give <img src="2-2340075\2c133d90-4e95-4a80-93ed-d65d42c6e8cf.jpg" /> as desired. To deal with the case when <img src="2-2340075\87d06766-325c-4200-94b5-3f95e283bd71.jpg" /> is large, simply iterate the case when <img src="2-2340075\4b855f3d-a51d-40cb-a437-6afe20f8037d.jpg" /> is small (shrinking<img src="2-2340075\5d255452-e2f7-4849-8b4b-1a810e620d5c.jpg" />, <img src="2-2340075\9a5df841-72a9-49fc-b2a6-1bfe8179f0bf.jpg" />repeatedly) after a subdivision of the time interval<img src="2-2340075\ac0c8578-76e6-4b32-895d-125f232cdc70.jpg" />.</p></sec><sec id="s4"><title>4. Stability of the Mass-Supercritical and Energy-Subcritical</title><p>In this section we discuss the Stability theory of the mass-supercritical and energy-subcritical to the nonlinear Schr&#246;dinger equation. Consider the initial-value problem (1.1) with <img src="2-2340075\48191d6c-0aea-402d-a2c4-0fa5b2ab725d.jpg" /> and <img src="2-2340075\ec87d769-7146-4204-b5ed-8c36caa9f7ad.jpg" /> we chose<img src="2-2340075\d1e32a5f-6f06-48d8-9fdd-70dbfb4d3dcd.jpg" />.</p><p>In this case the initial-value problem <img src="2-2340075\0c544ccc-12ae-485c-bddc-e74f31ac430b.jpg" /> is locally well-posed in<img src="2-2340075\fe41a7f9-d2e3-40d5-80b2-d9d634609869.jpg" />. Now we rewrite (1.1) as</p><p><img src="2-2340075\529ac618-cffb-47aa-89ad-782d891d1710.jpg" />&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160; (1.1)<sup>*</sup></p><p>We discuss the stability by the following proposition. Before beginning we need define the Kato inhomogeneous Strichartz estimate. See [<xref ref-type="bibr" rid="scirp.32976-ref16">16</xref>]</p><disp-formula id="scirp.32976-formula55512"><label>(4.1)</label><graphic position="anchor" xlink:href="2-2340075\b70e19b5-b0e7-43e8-90e2-6e1b7e41b69a.jpg"  xlink:type="simple"/></disp-formula><p>Proposition 4.1 For each <img src="2-2340075\87be9d0d-99c4-4ac6-85f8-34d2fbbe8cc3.jpg" /> there exists <img src="2-2340075\b4b4cdee-1fe5-442d-bc85-d3c382b1e5a6.jpg" /> and <img src="2-2340075\f0f47031-adf6-4d4a-ad6e-733d700b32b5.jpg" /> such that the following holds.</p><p>Let <img src="2-2340075\f033975a-fd3d-4995-90ed-883e07ae7c5f.jpg" /> and solve</p><p><img src="2-2340075\0e252de1-7c3c-48bc-81fc-bc5150334fab.jpg" />.</p><p>Let <img src="2-2340075\7f6a0c23-1232-456f-a4bb-b425a205ade2.jpg" /> for all <img src="2-2340075\1640ccab-d06f-4dee-b09f-414f8130e0af.jpg" /> and define</p><p><img src="2-2340075\388c3d35-0073-4470-956c-632c86225611.jpg" /></p><p>If</p><p><img src="2-2340075\c4ef13fb-716f-4d2f-b227-de1e146e1fa4.jpg" /></p><p>And</p><disp-formula id="scirp.32976-formula55513"><label>(4.2)</label><graphic position="anchor" xlink:href="2-2340075\13c78a7a-9072-4b84-aad2-2fc70c69c9f0.jpg"  xlink:type="simple"/></disp-formula><p>Then</p><p><img src="2-2340075\9f2ccb5d-eb18-4e47-9419-c75412eac93e.jpg" /></p><p>Proof: Let w be deﬁned by <img src="2-2340075\db60faec-95b1-46e1-9e75-1ab3df690bd4.jpg" /> then <img src="2-2340075\9193b0ac-a150-4eb5-a212-78118838183d.jpg" /> solves the equation</p><disp-formula id="scirp.32976-formula55514"><label>(4.3)</label><graphic position="anchor" xlink:href="2-2340075\ecf72030-32f6-484b-be6e-acaeab8eca2f.jpg"  xlink:type="simple"/></disp-formula><p>since<img src="2-2340075\68f9746b-5b0c-4bd2-80d7-c193d1cfd305.jpg" />.Can be divided <img src="2-2340075\941a23ce-9a7d-4141-b3d9-75e68ae9a02a.jpg" /> into</p><p><img src="2-2340075\620e8d5e-49d9-43fd-a4ff-468152d7197b.jpg" />in intervals <img src="2-2340075\1787f9ab-e64f-4184-ab5b-90a49f689a81.jpg" /> Such that for all<img src="2-2340075\6aacfa97-193b-471b-93c3-5ded0fc76404.jpg" />, the quantity<img src="2-2340075\04691162-d086-4c8b-a082-4b7acc3ff16f.jpg" />, is Appropriate small</p><p>(δ to be selected below).</p><p>Integration (4.3) with initial time <img src="2-2340075\42945af0-362d-470a-be42-fee8a09703d7.jpg" /> is</p><disp-formula id="scirp.32976-formula55515"><label>(4.4)</label><graphic position="anchor" xlink:href="2-2340075\4a801025-ba35-43de-9c1e-f2e08f9830c5.jpg"  xlink:type="simple"/></disp-formula><p>where</p><p><img src="2-2340075\8daa6043-2dd5-40ca-9f7d-16481f3a04e5.jpg" />.</p><p>Applying the Kato Strichartz estimate (4.1) on<img src="2-2340075\457a412f-9f85-4d48-ba45-d2fd46309e55.jpg" />, to obtain</p><disp-formula id="scirp.32976-formula55516"><label>. (4.5)</label><graphic position="anchor" xlink:href="2-2340075\0bc578e8-51d8-4ac4-baed-2f4cee3ffdfd.jpg"  xlink:type="simple"/></disp-formula><p>Note that</p><p><img src="2-2340075\edaae2da-2b00-48cc-8419-1cec8f5ae634.jpg" />.</p><p>Similarly,</p><p><img src="2-2340075\565425c5-1df8-48c0-9cfb-aa8f7a44fc55.jpg" /></p><p>and</p><p><img src="2-2340075\e80a6c88-ba6d-4838-8cdf-5478f06853af.jpg" /></p><p>Substituting the above estimates in (4.5), to get,</p><disp-formula id="scirp.32976-formula55517"><label>(4.6)</label><graphic position="anchor" xlink:href="2-2340075\4d9af0c0-ddee-43b1-9935-aadaf0554d9a.jpg"  xlink:type="simple"/></disp-formula><p>As long as</p><p><img src="2-2340075\0ba47ae6-b886-4626-9ddf-0d458bd10337.jpg" /></p><p>and</p><disp-formula id="scirp.32976-formula55518"><label>(4.7)</label><graphic position="anchor" xlink:href="2-2340075\157e9deb-26dd-46f5-b432-1d22fc5c73ed.jpg"  xlink:type="simple"/></disp-formula><p>We obtain</p><disp-formula id="scirp.32976-formula55519"><label>(4.8)</label><graphic position="anchor" xlink:href="2-2340075\9988bdad-1762-49b8-9ccf-a2f07066e16e.jpg"  xlink:type="simple"/></disp-formula><p>Taken now <img src="2-2340075\85dad084-c7b8-4211-a051-7e2b17c02d6b.jpg" /> in (4.4) and apply <img src="2-2340075\d586031f-f60d-4fa6-9595-a4aa0fdebab2.jpg" /> to both sides to obtain</p><disp-formula id="scirp.32976-formula55520"><label>(4.9)</label><graphic position="anchor" xlink:href="2-2340075\0fbb3e00-3caf-4f7c-a526-3d7e48911c57.jpg"  xlink:type="simple"/></disp-formula><p>Since the Duhamel integral is restricted to<img src="2-2340075\9dc78131-6758-4417-9dc7-6c08ec699e5b.jpg" />by again applying the Kato estimate, similarly to (4.6) we obtain,</p><p><img src="2-2340075\29c02e83-fb5a-40b7-a167-60a1d0bfc9a6.jpg" /></p><p>By (4.8) and (4.9), we bound the Former of expression to obtain</p><p><img src="2-2340075\32dd0d5b-9174-411b-8096-aa2d163473ba.jpg" /></p><p>Start iterates with<img src="2-2340075\83fe4a3c-3f44-474a-8cf2-1e8c0c004cac.jpg" />, we obtain</p><p><img src="2-2340075\1d5d9d82-6d34-47fd-a0f2-c1cdb0fa7363.jpg" /></p><p>To absorb the second part of (4.7) for all intervals <img src="2-2340075\5bb35457-7193-404e-9be4-52dedb3be5d1.jpg" /> <img src="2-2340075\81508d75-24e0-41ec-9005-306695311fed.jpg" /> we require</p><disp-formula id="scirp.32976-formula55521"><label>(4.10)</label><graphic position="anchor" xlink:href="2-2340075\03108615-caec-424c-8095-f2e4c284ba30.jpg"  xlink:type="simple"/></disp-formula><p>We review that the dependence of parameters δ is an absolute constant chosen to meet the first part of (4.7). The inequality (4.10) determines how the small <img src="2-2340075\244215d5-a6d1-4276-8f80-924e68554c53.jpg" /> needs to be taken in terms of <img src="2-2340075\b2728847-6520-4b9b-bd4e-95b1225279b5.jpg" />(and thus, in terms of<img src="2-2340075\55458a78-7384-4a67-b9bb-66fc4fdef558.jpg" />). We were given <img src="2-2340075\04089fcb-49c0-40d2-81dc-c520243f9945.jpg" /> which then determined <img src="2-2340075\1afb4ca3-f865-49ed-9796-d42571a8f3e4.jpg" /> □</p></sec><sec id="s5"><title>REFERENCES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.32976-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">S. Keraani, “On the Blow-Up Phenomenon of the Critical Nonlinear Schrodinger Equation,” Journal of Functional Analysis, Vol. 235, No. 1, 2006, pp. 171-192.  
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