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Titlebook: Current Topics in Astrofundamental Physics: The Cosmic Microwave Background; Norma G. Sánchez Book 2001 Kluwer Academic Publishers 2001 Ac

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樓主: Madison
11#
發(fā)表于 2025-3-23 11:59:32 | 只看該作者
The High Redshift Radio Universeoch..It is shown, that Russian new generation CMBA“Cosmological Gene” project can help in the extention of the observable part of the Universe, and some questions, connected with post-SKA instrumentation will be discussed as well.
12#
發(fā)表于 2025-3-23 17:48:09 | 只看該作者
13#
發(fā)表于 2025-3-23 22:01:26 | 只看該作者
14#
發(fā)表于 2025-3-23 22:53:59 | 只看該作者
1389-2185 ysics framework, werethe maingoals ofthe course. Lectures ranged from a motivation and pedagogical introduction for students and participants not directly worki978-0-7923-6856-4978-94-010-0748-1Series ISSN 1389-2185
15#
發(fā)表于 2025-3-24 05:23:36 | 只看該作者
Current Topics in Astrofundamental Physics: The Cosmic Microwave Background
16#
發(fā)表于 2025-3-24 09:37:34 | 只看該作者
17#
發(fā)表于 2025-3-24 14:31:33 | 只看該作者
18#
發(fā)表于 2025-3-24 17:27:42 | 只看該作者
New Dual Relations Between Quantum Field Theory and String Regimes In Curved BackgroundsThis operation maps the characteristic length of one regime into the other (and, as a consequence, mass domains as well). The .-transform is not an assumed or . imposed symmetry but is revealed by the QFT and String dynamics in curved backgrounds. The Hawking-Gibbons temperature and the string maxim
19#
發(fā)表于 2025-3-24 22:15:20 | 只看該作者
Detectability of Relic Squeezed Gravitational Waves by Laser Interferometersons, is within the reach of sensitive gravity-wave detectors. In the favorable case, the detection of relic gravitational waves can be achieved by initial laser interferometers in LIGO, VIRGO, GE0600. In more conservative cases, the sensitivity of advanced ground-based and cosmic laser interferomete
20#
發(fā)表于 2025-3-25 02:55:56 | 只看該作者
Gravitational Field and Its Energy-Momentum Tensorm tensor which is 1) derivable from the Lagrangian in a regular prescribed way, 2) tensor under arbitrary coordinate transformations, 3) symmetric in its components, 4) conserved due to the equations of motionderived from the same Lagrangian, 5) free of the second (highest) derivatives of the field
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