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Titlebook: Current Topics in Astrofundamental Physics; The Early Universe N. Sánchez,A. Zichichi Book 1995 Springer Science+Business Media Dordrecht 1

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樓主: Capricious
11#
發(fā)表于 2025-3-23 11:43:44 | 只看該作者
12#
發(fā)表于 2025-3-23 17:11:45 | 只看該作者
13#
發(fā)表于 2025-3-23 19:27:12 | 只看該作者
New Multicarrier Modulations for 5G angular scales against the hypothesis that the observed temperature fluctuations reflect Gaussian initial density perturbations with random phases. The data are in excellent agreement with the Gaussian hypothesis and rule out certain “toy models” of non-Gaussian amplitude distribution.
14#
發(fā)表于 2025-3-23 23:02:27 | 只看該作者
Izzat Darwazeh,Ryan C. Grammenos,Tongyang Xun conjunction with X-ray maps from the ROSAT and Einstein satellites to place a limit on the Hubble constant of.. The implications of these observations are discussed in the context of continued CMB observations from ground-based sites and plans are presented for the Very Small Array.
15#
發(fā)表于 2025-3-24 05:51:26 | 只看該作者
A.E. Lutsky,I.V. Mursenkova,I.A. Znamenskayanal error). Eight methods that are independent of the Virgo cluster (Table 3) give H. = 50 within 10%. Criticisms of all the methods that have been said to give the short distance scale with H. ~ 85 are set out.
16#
發(fā)表于 2025-3-24 09:20:18 | 只看該作者
17#
發(fā)表于 2025-3-24 12:13:03 | 只看該作者
18#
發(fā)表于 2025-3-24 15:28:32 | 只看該作者
19#
發(fā)表于 2025-3-24 19:32:17 | 只看該作者
20#
發(fā)表于 2025-3-25 01:58:07 | 只看該作者
The Covariant and Gauge Invariant Approach to Perturbations in Cosmologyhe best available approach to proving spatial homogeneity of the universe. The extension of this approach to Sachs-Wolfe style analyses is not yet complete, and a series of issues to do with averaging scales and with modelling the real, lumpy universe by means of simpler, smoothed out models remain to be resolved.
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