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Titlebook: Cosmology in Scalar-Tensor Gravity; Valerio Faraoni Book 2004 Springer Science+Business Media Dordrecht 2004 Cosmology.Dust solution.EFE.G

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發(fā)表于 2025-3-26 21:55:54 | 只看該作者
32#
發(fā)表于 2025-3-27 01:55:16 | 只看該作者
Rogier Crijns,Nina D?rner,Philip Langeral relativity, with the modifications dictated by the anomalous coupling of the Einstein frame scalar to ordinary matter and its consequences. A ., the mathematical equivalence need not be a physical one. The literature using conformal transformations in cosmology and in alternative theories of gr
33#
發(fā)表于 2025-3-27 05:27:44 | 只看該作者
Regina H?nchen,Johannes Schnitzergravity. An array of detectors could distinguish between massless tensor modes with spin two the only ones present in general relativity and modes of different spin, such as the spin zero modes of the scalar gravitational field in scalar-tensor gravity [887, 307, 308, 909]. Regarding the astrophysic
34#
發(fā)表于 2025-3-27 10:13:51 | 只看該作者
35#
發(fā)表于 2025-3-27 15:36:45 | 只看該作者
Rogier Crijns,Nina D?rner,Philip Langund, which have been detected by the . mission in 1992 [809]. These perturbations are the subject of intense experimental study. Hence, density and gravitational wave fluctuations around the FLRW background provide the means to test the predictions of theories of the early universe. Soon after the i
36#
發(fā)表于 2025-3-27 20:53:15 | 只看該作者
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發(fā)表于 2025-3-28 00:29:55 | 只看該作者
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發(fā)表于 2025-3-28 02:47:43 | 只看該作者
Fundamental Theories of Physicshttp://image.papertrans.cn/c/image/238934.jpg
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發(fā)表于 2025-3-28 08:24:37 | 只看該作者
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發(fā)表于 2025-3-28 13:38:11 | 只看該作者
Conference proceedings 2003 pairs which may form at equilibrium. The Workshop was targeted both to clarify the pending questions and, as far as feasible, to trace the path to possible answers since the underlying phenomena are yet incompletely understood and since a reliable theory is often not available. On the other hand, t
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