到婚嫁年龄
发表于 2025-3-25 04:04:15
http://reply.papertrans.cn/19/1890/188950/188950_21.png
敌意
发表于 2025-3-25 07:37:28
Krankengeschichten und Behandlungsberichte,tic field, aligned along the Debever-Penrose directions of the Weyl tensor of Petrov type D. Among them, because of their interpretation as black holes, the Reissner-Nordström static solution and the Kerr-Newman stationary axisymmetric solution are singled out.
Malleable
发表于 2025-3-25 12:49:41
http://reply.papertrans.cn/19/1890/188950/188950_23.png
exclamation
发表于 2025-3-25 18:59:37
Lehrbuch der psychoanalytischen Therapie in numerical black hole simulations, I discuss a series of calculations from axisymmetry to full 3D that can be seen as stepping stones to simulations of the full 3D coalescence of two black holes. In particular, I emphasize the interplay between perturbation theory and numerical simulation that bu
赞美者
发表于 2025-3-25 20:07:57
http://reply.papertrans.cn/19/1890/188950/188950_25.png
chondromalacia
发表于 2025-3-26 00:11:12
http://reply.papertrans.cn/19/1890/188950/188950_26.png
Offstage
发表于 2025-3-26 05:34:25
Qualitätssicherung und Konstanzprüfungeneral relativistic irreversible thermodynamics and derive a universal parameter thermodynamics for rotating fluids ("rotating bodies"). To extend the procedure to black holes, the black hole limit of the rigidly rotating disk of dust solution is discussed. It then turns out that the first law of bl
Condyle
发表于 2025-3-26 11:10:47
http://reply.papertrans.cn/19/1890/188950/188950_28.png
cruise
发表于 2025-3-26 14:26:32
E. A. Zimmer,Marianne Zimmer-Brossy effects on the geometry near the inner (Cauchy) horizon because of a diverging blueshift. Determining the inner structure of the hole is really an evolutionary problem with precisely known initial data. The evolution can in principle be followed to within Planck distances of the singularity at the
Conjuction
发表于 2025-3-26 17:29:28
Röntgenologische StandardprojektionenWe investigate the possible gravitational redshift values for boson stars with a self-interaction, studying a wide range of possible masses. We find a limiting value of . for stable boson star configurations. We can rule out the direct observability of boson stars. X-ray spectroscopy is perhaps the most interesting possibility.