SPALL
发表于 2025-3-25 04:03:56
Hermann Brandenburg,Volker Fenchel causal future directed vectors. These diffeomorphisms, called proper causal relations, contain as a subset the well known group of conformal relations which can be characterized as those diffeomorphisms such that both the transformation itself and its inverse are proper causal relations. It turns o
联邦
发表于 2025-3-25 10:38:43
https://doi.org/10.1007/3-540-36973-2Accretion; Cosmology; Gravity; Lorentz transformation; astrophysics; black holes; numerical relativity; rel
休息
发表于 2025-3-25 13:08:50
978-3-662-14420-6Springer-Verlag Berlin Heidelberg 2003
Hyperalgesia
发表于 2025-3-25 17:09:02
Black Hole Thermodynamicsof their horizon area. The brick wall model and an operational approach are discussed. An attempt to understand at the microlevel how the quantum black hole acquires its thermal properties is included. The chapter concludes with some remarks on the extension of these techniques to describing the dynamical process of black hole evaporation.
样式
发表于 2025-3-25 23:16:37
Perturbations of Black Holesd polar. Their equations decouple and reduce to Schrödinger wave equations. Special attention is paid to quasi-normal modes for black holes and how they can be excited, since gravitational waves are emitted at their frequencies and they appear in many dynamical processes.
噱头
发表于 2025-3-26 01:37:13
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多嘴多舌
发表于 2025-3-26 04:17:54
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Inveterate
发表于 2025-3-26 08:52:17
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Rct393
发表于 2025-3-26 13:44:54
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Flawless
发表于 2025-3-26 16:48:07
Lorentzian Comments on Stokes Parametersers and the degree of polarization. The evolution equations for Stokes parameters on a curved space-time are obtained using the parallel transport of the polarization vector along a null geodesic. The interest of these equations in Astrophysics and Relativistic Cosmology is outlined.