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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 2025-3-21 16:46:40 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Cosmology in Scalar-Tensor Gravity
編輯Valerio Faraoni
視頻videohttp://file.papertrans.cn/239/238934/238934.mp4
叢書名稱Fundamental Theories of Physics
圖書封面Titlebook: Cosmology in Scalar-Tensor Gravity;  Valerio Faraoni Book 2004 Springer Science+Business Media Dordrecht 2004 Cosmology.Dust solution.EFE.G
描述.Cosmology in Scalar-Tensor Gravity. covers all aspects of cosmology in scalar-tensor theories of gravity. Considerable progress has been made in this exciting area of physics and this book is the first to provide a critical overview of the research. Among the topics treated are: .-Scalar-tensor gravity and its limit to general relativity, .-Effective energy-momentum tensors and conformal frames, .-Gravitational waves in scalar-tensor cosmology, .-Specific scalar-tensor theories, .-Exact cosmological solutions and cosmological perturbations, .-Scalar-tensor scenarios of the early universe and inflation, .-Scalar-tensor models of quintessence in the present universe and their far-reaching consequences for the ultimate fate of the cosmos. .
出版日期Book 2004
關(guān)鍵詞Cosmology; Dust solution; EFE; Gravity; Relativity; Universe; general relativity
版次1
doihttps://doi.org/10.1007/978-1-4020-1989-0
isbn_softcover978-90-481-6564-3
isbn_ebook978-1-4020-1989-0Series ISSN 0168-1222 Series E-ISSN 2365-6425
issn_series 0168-1222
copyrightSpringer Science+Business Media Dordrecht 2004
The information of publication is updating

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發(fā)表于 2025-3-21 21:40:06 | 只看該作者
Effective Energy-Momentum Tensors and Conformal Frames,eral 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
板凳
發(fā)表于 2025-3-22 02:51:59 | 只看該作者
Gravitational Waves in Scalar-Tensor Cosmology,gravity. 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
地板
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5#
發(fā)表于 2025-3-22 12:33:45 | 只看該作者
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發(fā)表于 2025-3-22 14:43:51 | 只看該作者
Nonminimal Coupling,exts that it deserves special treatment, although it can formally be reduced to a special case of a scalar-tensor theory. The action is .ξ where is a dimensionless coupling constant. Through most of this chapter, the action . describing other forms of matter is omitted, since we want to consider reg
7#
發(fā)表于 2025-3-22 20:50:56 | 只看該作者
The Present Universe,., . . > 0. This conclusion is based on observations of distant type Ia supernovae [738, 703], which have a characteristic light curve and constitute reasonable standard candles for cosmological studies [149, 438] . The systematic search for type Ia supernovae followed two decades of progress in the
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發(fā)表于 2025-3-23 00:54:51 | 只看該作者
Nonminimal Coupling,dimensionless coupling constant. Through most of this chapter, the action . describing other forms of matter is omitted, since we want to consider regimes in which the nonminimally coupled scalar dominates the cosmic dynamics, for example during inflation.
9#
發(fā)表于 2025-3-23 01:24:34 | 只看該作者
0168-1222 de in this exciting area of physics and this book is the first to provide a critical overview of the research. Among the topics treated are: .-Scalar-tensor gravity and its limit to general relativity, .-Effective energy-momentum tensors and conformal frames, .-Gravitational waves in scalar-tensor c
10#
發(fā)表于 2025-3-23 05:34:11 | 只看該作者
dimensionless coupling constant. Through most of this chapter, the action . describing other forms of matter is omitted, since we want to consider regimes in which the nonminimally coupled scalar dominates the cosmic dynamics, for example during inflation.
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