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樓主: Definite
11#
發(fā)表于 2025-3-23 11:31:27 | 只看該作者
Nachrichtenfaktoren und Rezeptionl implications. Traschen’s integral constraint vectors have a particularly simple relation to the Killing vectors of de Sitter spaces. Integral constraints, of which Traschen’s are a special class, exist on any hypersurface with any vector field and on any background..Integral constraints for non-linear perturbations are also given here.
12#
發(fā)表于 2025-3-23 16:51:36 | 只看該作者
13#
發(fā)表于 2025-3-23 21:09:08 | 只看該作者
14#
發(fā)表于 2025-3-24 00:57:18 | 只看該作者
Topological Censorship and Chronology Protection, neither appears common in the macroscopic universe. Several recent results on topological censorship and chronology protection seek to explain why the macroscopic topology and causal structure of spacetime are ordinary.
15#
發(fā)表于 2025-3-24 03:55:58 | 只看該作者
16#
發(fā)表于 2025-3-24 08:33:07 | 只看該作者
The Gravitational Instability Picture and the Epoch of Galaxy Formationlaxy distribution. There is evidence the luminous central parts of the giant galaxies were present at redshift . = 3. In the cold dark matter model for structure formation the galaxies would have to have been assembled not much earlier than this, in pronounced collapses that may be observable. The g
17#
發(fā)表于 2025-3-24 12:32:43 | 只看該作者
Active Galaxies at Large Redshiftsave shown that active star formation in galaxies has continued over the same redshift interval over which active galaxies display strong cosmological evolution. At redshifts greater than 2, there is evidence that many galaxies underwent bursts of continued star formation and that, at the largest red
18#
發(fā)表于 2025-3-24 17:37:21 | 只看該作者
19#
發(fā)表于 2025-3-24 21:52:45 | 只看該作者
20#
發(fā)表于 2025-3-25 01:48:13 | 只看該作者
Inspiraling Compact Binaries potential sources of gravitational radiation to be observed by the future detectors LIGO and VIRGO. Emphasizing the highly relativistic nature of inspiraling compact binaries, we discuss their modelisation by a system of two non-spinning point masses, emitting gravitational waves at a high post-New
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