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Global Nonlinear Stability of Schwarzschild Spacetime under Polarized Perturbations /
Essential mathematical insights into one of the most important and challenging open problems in general relativity—the stability of black holes One of the major outstanding questions about black holes is whether they remain stable when subject to small perturbations. An affirmative answer to this qu...
| Clasificación: | Libro Electrónico |
|---|---|
| Autor principal: | |
| Otros Autores: | |
| Formato: | eBook |
| Idioma: | Inglés |
| Publicado: |
Princeton :
Princeton University Press,
2020.
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| Colección: | Annals of mathematics studies.
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| Temas: | |
| Acceso en línea: | Texto completo |
MARC
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| 100 | 1 | |a Szeftel, Jérémie. | |
| 245 | 1 | 0 | |a Global Nonlinear Stability of Schwarzschild Spacetime under Polarized Perturbations / |c Sergiu Klainerman, Jérémie Szeftel |
| 260 | |a Princeton : |b Princeton University Press, |c 2020. | ||
| 300 | |a 1 online resource (xviii, 840 pages). | ||
| 520 | |a Essential mathematical insights into one of the most important and challenging open problems in general relativity—the stability of black holes One of the major outstanding questions about black holes is whether they remain stable when subject to small perturbations. An affirmative answer to this question would provide strong theoretical support for the physical reality of black holes. In this book, Sergiu Klainerman and Jérémie Szeftel take a first important step toward solving the fundamental black hole stability problem in general relativity by establishing the stability of nonrotating black holes—or Schwarzschild spacetimes—under so-called polarized perturbations. This restriction ensures that the final state of evolution is itself a Schwarzschild space. Building on the remarkable advances made in the past fifteen years in establishing quantitative linear stability, Klainerman and Szeftel introduce a series of new ideas to deal with the strongly nonlinear, covariant features of the Einstein equations. Most preeminent among them is the general covariant modulation (GCM) procedure that allows them to determine the center of mass frame and the mass of the final black hole state. Essential reading for mathematicians and physicists alike, this book introduces a rich theoretical framework relevant to situations such as the full setting of the Kerr stability conjecture. | ||
| 590 | |a JSTOR |b Books at JSTOR All Purchased | ||
| 590 | |a JSTOR |b Books at JSTOR Demand Driven Acquisitions (DDA) | ||
| 590 | |a JSTOR |b Books at JSTOR Evidence Based Acquisitions | ||
| 650 | 0 | |a Schwarzschild black holes. | |
| 650 | 0 | |a Perturbation (Mathematics) | |
| 650 | 6 | |a Perturbation (Mathématiques) | |
| 650 | 7 | |a Perturbation (Mathematics) |2 fast | |
| 650 | 7 | |a Schwarzschild black holes |2 fast | |
| 700 | 1 | |a Klainerman, Sergiu. | |
| 776 | 0 | 8 | |i Print version: |a Szeftel, Jérémie |t Global Nonlinear Stability of Schwarzschild Spacetime under Polarized Perturbations : (ams-210) |d Princeton : Princeton University Press,c2020 |z 9780691212432 |
| 830 | 0 | |a Annals of mathematics studies. | |
| 856 | 4 | 0 | |u https://jstor.uam.elogim.com/stable/10.2307/j.ctv15r57cw |z Texto completo |
| 938 | |a Askews and Holts Library Services |b ASKH |n AH37884752 | ||
| 938 | |a ProQuest Ebook Central |b EBLB |n EBL6403713 | ||
| 938 | |a EBSCOhost |b EBSC |n 2583264 | ||
| 994 | |a 92 |b IZTAP | ||