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The Extremal Collapse Threshold and the Third Law of Black Hole Thermodynamics.
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The Extremal Collapse Threshold and the Third Law of Black Hole Thermodynamics.
자료유형  
 학위논문
Control Number  
0017161785
International Standard Book Number  
9798382807065
Dewey Decimal Classification Number  
510
Main Entry-Personal Name  
Unger, Ryan.
Publication, Distribution, etc. (Imprint  
[S.l.] : Princeton University., 2024
Publication, Distribution, etc. (Imprint  
Ann Arbor : ProQuest Dissertations & Theses, 2024
Physical Description  
373 p.
General Note  
Source: Dissertations Abstracts International, Volume: 85-12, Section: B.
General Note  
Advisor: Dafermos, Mihalis.
Dissertation Note  
Thesis (Ph.D.)--Princeton University, 2024.
Summary, Etc.  
요약In this dissertation, we investigate extremal black holes in general relativity. Extremal black holes are exceptional solutions of Einstein's equations which have absolute zero temperature in the celebrated thermodynamic analogy of black hole mechanics.Our first main result is a definitive disproof of the "third law of black hole thermodynamics." We construct examples of black hole formation from regular, one-ended asymptotically flat Cauchy data for the Einstein-Maxwell-charged scalar field system which are exactly isometric to extremal Reissner-Nordstrom after a finite advanced time along the event horizon. Moreover, in each of these examples the apparent horizon of the black hole coincides with that of a Schwarzschild solution at earlier advanced times. We also prove similar black hole formation results for very slowly rotating Kerr black holes in vacuum.Our second main result is a proof that extremal black holes arise on the threshold of gravitational collapse. More precisely, we construct smooth one-parameter families of smooth, spherically symmetric solutions to the Einstein-Maxwell-Vlasov system which interpolate between dispersion and collapse and for which the critical solution is an extremal Reissner-Nordstrom black hole. We call this critical phenomenon extremal critical collapse and the present work constitutes the first rigorous result on the black hole formation threshold in general relativity.The above mentioned results constitute Part I of this dissertation and were all obtained in joint work with Christoph Kehle.In Part II of this dissertation, we study extensions of the celebrated positive mass theorem to a very general class of initial data, including extremal black holes. These results were obtained in collaboration with Dan A. Lee, Martin Lesourd, and Shing-Tung Yau. We provide a resolution of the spacetime positive mass theorem on manifolds with boundary, a resolution of the remaining cases of Schoen and Yau's Liouville conjecture for locally conformally flat manifolds, and demonstrate a novel scalar curvature shielding phenomenon for the ADM mass.
Subject Added Entry-Topical Term  
Mathematics.
Subject Added Entry-Topical Term  
Theoretical physics.
Subject Added Entry-Topical Term  
Astrophysics.
Subject Added Entry-Topical Term  
Thermodynamics.
Index Term-Uncontrolled  
Black holes
Index Term-Uncontrolled  
Critical collapse
Index Term-Uncontrolled  
Black hole thermodynamics
Index Term-Uncontrolled  
Positive mass theorem
Index Term-Uncontrolled  
Scalar curvature
Index Term-Uncontrolled  
Third law
Added Entry-Corporate Name  
Princeton University Mathematics
Host Item Entry  
Dissertations Abstracts International. 85-12B.
Electronic Location and Access  
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Control Number  
joongbu:654768
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