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Nonlinear Wave Dynamics in Black Hol...
~
Princeton University.
Nonlinear Wave Dynamics in Black Hole Spacetimes.
紀錄類型:
書目-語言資料,手稿 : Monograph/item
正題名/作者:
Nonlinear Wave Dynamics in Black Hole Spacetimes./
作者:
Stogin, John.
面頁冊數:
1 online resource (568 pages)
附註:
Source: Dissertation Abstracts International, Volume: 78-11(E), Section: B.
Contained By:
Dissertation Abstracts International78-11B(E).
標題:
Mathematics. -
電子資源:
click for full text (PQDT)
ISBN:
9780355039795
Nonlinear Wave Dynamics in Black Hole Spacetimes.
Stogin, John.
Nonlinear Wave Dynamics in Black Hole Spacetimes.
- 1 online resource (568 pages)
Source: Dissertation Abstracts International, Volume: 78-11(E), Section: B.
Thesis (Ph.D.)
Includes bibliographical references
This thesis details a method for proving global boundedness and decay results for nonlinear wave equations on black hole spacetimes. The method is applied to five example problems of increasing difficulty. The first problem, which addresses the semilinear wave equation on Minkowski space, is quite simple and should be accessible to a reader who is still new to the field of partial differential equations. The final problem, which was posed by Ionescu and Klainerman in [IK14], constitutes a step toward proving stability for slowly rotating Kerr black holes. The remaining intermediate problems are: a semilinear wave equation on the Schwarzschild spacetime, a semilinear wave equation on any subextremal Kerr spacetime with the additional assumption of axisymmetry, and a restriction of the final problem to the Schwarzschild case.
Electronic reproduction.
Ann Arbor, Mich. :
ProQuest,
2018
Mode of access: World Wide Web
ISBN: 9780355039795Subjects--Topical Terms:
527692
Mathematics.
Index Terms--Genre/Form:
554714
Electronic books.
Nonlinear Wave Dynamics in Black Hole Spacetimes.
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Nonlinear Wave Dynamics in Black Hole Spacetimes.
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Source: Dissertation Abstracts International, Volume: 78-11(E), Section: B.
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Adviser: Sergiu Klainerman.
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Thesis (Ph.D.)
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Princeton University
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2017.
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Includes bibliographical references
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This thesis details a method for proving global boundedness and decay results for nonlinear wave equations on black hole spacetimes. The method is applied to five example problems of increasing difficulty. The first problem, which addresses the semilinear wave equation on Minkowski space, is quite simple and should be accessible to a reader who is still new to the field of partial differential equations. The final problem, which was posed by Ionescu and Klainerman in [IK14], constitutes a step toward proving stability for slowly rotating Kerr black holes. The remaining intermediate problems are: a semilinear wave equation on the Schwarzschild spacetime, a semilinear wave equation on any subextremal Kerr spacetime with the additional assumption of axisymmetry, and a restriction of the final problem to the Schwarzschild case.
520
$a
The method used in this thesis is based on a few particular developments that may be useful for other related problems. These include: a new method for constructing Morawetz-type estimates that is fairly robust (insofar as it may be successfully applied to all five problems), a strategy based on a decay hierarchy for energy estimates on uniformly spacelike hypersurfaces using, in particular, a notion of weak decay, and a technique for handling certain terms with factors that are singular on an axis of symmetry.
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Ann Arbor, Mich. :
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ProQuest,
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2018
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Mode of access: World Wide Web
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Princeton University.
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http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=10271342
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click for full text (PQDT)
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