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Titlebook: Einstein Equations: Physical and Mathematical Aspects of General Relativity; Domoschool 2018 Sergio Cacciatori,Batu Güneysu,Stefano Pigola

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樓主: complicated
11#
發(fā)表于 2025-3-23 11:16:35 | 只看該作者
Methoden der Geburtsvorbereitung,y various recent results concerning the large-scale geometric structure of asymptotically flat spaces. In the last section, we outline the construction, due to Schoen and the author, of localized solutions of the Einstein constraints and discuss its implications both on the physical and the geometric side.
12#
發(fā)表于 2025-3-23 16:46:37 | 只看該作者
13#
發(fā)表于 2025-3-23 21:04:56 | 只看該作者
Four Lectures on Asymptotically Flat Riemannian Manifoldsy various recent results concerning the large-scale geometric structure of asymptotically flat spaces. In the last section, we outline the construction, due to Schoen and the author, of localized solutions of the Einstein constraints and discuss its implications both on the physical and the geometric side.
14#
發(fā)表于 2025-3-23 23:39:54 | 只看該作者
15#
發(fā)表于 2025-3-24 02:33:09 | 只看該作者
16#
發(fā)表于 2025-3-24 06:45:43 | 只看該作者
Komplikationen in der Nachgeburtsphase, has a direct connection with the classical description. This technique is particularly useful to model several astrophysical situations. We show two particular applications related to radiation processes and accretion disc physics.
17#
發(fā)表于 2025-3-24 10:53:31 | 只看該作者
,Der mensuelle Zyklus und seine St?rungen, and non-rotating compact objects in general relativity. It is then shown how WKB methods can be used to approximate the spectrum and reconstruct the underlying perturbation potential by using different Bohr–Sommerfeld rules. The uniqueness and properties of the reconstructed relations are discussed as well.
18#
發(fā)表于 2025-3-24 17:52:22 | 只看該作者
19#
發(fā)表于 2025-3-24 20:13:24 | 只看該作者
Schwangerenberatung und -vorbereitung,ls. A short discussion of canonical charges associated to the BMS transformations and the possible relation between superrotations and transition from asymptotically flat to locally asymptotically flat spacetimes is also summarised.
20#
發(fā)表于 2025-3-25 02:11:55 | 只看該作者
Lectures on Linear Stability of Rotating Black Holeskolsky equation can be fully separated to a system of coupled ordinary differential equations. Linear stability of the non-extreme Kerr black hole is stated as a pointwise decay result for solutions of the Cauchy problem for the Teukolsky equation. The stability proof is outlined, with an emphasis on the underlying ideas and methods.
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