未成熟
发表于 2025-3-25 05:30:29
Kimio Uchiyama,Kazushige Tanabese, howthey change the dynamics of the expansion and how they decouple from the electrons and positrons. The neutrinos provide an example of the type of decoupling process which is important for other unknown types of weakly interacting particle.
柔美流畅
发表于 2025-3-25 10:02:31
Waste Management: A Policy Paradox,hat the dominant dark matter must be in some non-baryonic form. We will develop the dark matter models in much more detail in Chap. 13, using many of the tools developed in this chapter. First of all, we need to deal with a number of key issues concerning cosmological horizons and superhorizon perturbations which we have glossed over so far.
Override
发表于 2025-3-25 14:14:59
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obstruct
发表于 2025-3-25 17:00:26
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CREEK
发表于 2025-3-25 23:09:59
An Introduction to Relativistic Gravityrimental and observational status of General Relativity is reviewed and it is shown that it has triumphantly survived the many critical tests of the theory which have been devised since its inception in 1915.. If you are happy to accept General Relativity at its face value, you may advance to Chap. 7.
GAVEL
发表于 2025-3-26 03:32:36
The Friedman World Modelsfluid moves along streamlines in the universal expansion and so behaves like a perfect fluid for which the energy–momentum tensor is given by the T. of (6.33). .– General Relativity, which enables us to relate the energy–momentum tensor to the geometrical properties of space–time through (6.47) or (6.48).
TRUST
发表于 2025-3-26 05:39:12
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laparoscopy
发表于 2025-3-26 12:08:35
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龙卷风
发表于 2025-3-26 14:55:29
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Ingenuity
发表于 2025-3-26 18:15:25
978-3-662-49579-7Springer-Verlag Berlin Heidelberg 2008