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Titlebook: Generation of Cosmological Large-Scale Structure; David N. Schramm,P. Galeotti Book 1997 Kluwer Academic Publishers 1997 Astronomical Obse

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發(fā)表于 2025-3-25 03:36:37 | 只看該作者
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發(fā)表于 2025-3-25 22:45:43 | 只看該作者
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發(fā)表于 2025-3-26 02:38:14 | 只看該作者
the current situation on the age of the universe and the Hubble constant are reviewed since they provide the framework for the basic density arguments. It is shown that the Big Bang Nucleosynthesis constraints on the cosmological baryon density, when compared with dynamical arguments, demonstrate th
27#
發(fā)表于 2025-3-26 07:10:30 | 只看該作者
https://doi.org/10.1007/978-94-009-8024-2er distribution. The amplitude of those velocities is regulated by the spatial scale and the amplitude of the matter density irregularities as well as by the value of the mean matter density. The direct measurement of peculiar velocities thus provides a means to infer the characteristics of the mass
28#
發(fā)表于 2025-3-26 11:46:05 | 只看該作者
29#
發(fā)表于 2025-3-26 16:33:13 | 只看該作者
https://doi.org/10.1007/978-3-662-64682-3luminosity. In this chapter I review some topics which I considered in my thesis. In the presence of large scale structure sophisticated techniques are needed for luminosity function. I will discuss one of these and its extension to a photometric data set. All luminosity function estimation techniqu
30#
發(fā)表于 2025-3-26 18:37:40 | 只看該作者
Methodologies, Methods and Data,on the range of predictions of several Standard Solar Models (SSM) [1] [2] [3] is listed for each type of experiment together with the calculated contributions of the strongest solar neutrino branches. A basic analysis shows that the result of Kamiokande [4], which is only sensitive to the high ener
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