標題: Titlebook: Cosmology in Scalar-Tensor Gravity; Valerio Faraoni Book 2004 Springer Science+Business Media Dordrecht 2004 Cosmology.Dust solution.EFE.G [打印本頁] 作者: cessation 時間: 2025-3-21 16:46
書目名稱Cosmology in Scalar-Tensor Gravity影響因子(影響力)
書目名稱Cosmology in Scalar-Tensor Gravity影響因子(影響力)學科排名
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書目名稱Cosmology in Scalar-Tensor Gravity網(wǎng)絡公開度學科排名
書目名稱Cosmology in Scalar-Tensor Gravity被引頻次
書目名稱Cosmology in Scalar-Tensor Gravity被引頻次學科排名
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書目名稱Cosmology in Scalar-Tensor Gravity年度引用學科排名
書目名稱Cosmology in Scalar-Tensor Gravity讀者反饋
書目名稱Cosmology in Scalar-Tensor Gravity讀者反饋學科排名
作者: Toxoid-Vaccines 時間: 2025-3-21 21:40
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作者: 致敬 時間: 2025-3-22 02:51
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作者: Prosaic 時間: 2025-3-22 07:01 作者: 切掉 時間: 2025-3-22 12:33 作者: Malcontent 時間: 2025-3-22 14:43
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作者: Malcontent 時間: 2025-3-22 20:50
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作者: BET 時間: 2025-3-23 00:54
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.作者: Eructation 時間: 2025-3-23 01:24
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作者: Outshine 時間: 2025-3-23 05:34
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.作者: TIA742 時間: 2025-3-23 09:49
0168-1222 verse and inflation, .-Scalar-tensor models of quintessence in the present universe and their far-reaching consequences for the ultimate fate of the cosmos. .978-90-481-6564-3978-1-4020-1989-0Series ISSN 0168-1222 Series E-ISSN 2365-6425 作者: 枯萎將要 時間: 2025-3-23 14:53
Rogier Crijns,Nina D?rner,Philip Langn use eqs. (1.141) and (1.169) and integrate eq. (1.199) to obtain the corresponding Einstein frame solutions. In practice the reverse path is sometimes followed, i.e., exact solutions of general relativity are mapped back into the Jordan frame to obtain exact solutions in this representation.作者: VOC 時間: 2025-3-23 21:03 作者: 陳腐的人 時間: 2025-3-24 00:25
Book 2004 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, 作者: 熄滅 時間: 2025-3-24 04:04 作者: ANTI 時間: 2025-3-24 08:14 作者: anesthesia 時間: 2025-3-24 14:38 作者: fetter 時間: 2025-3-24 16:50 作者: notice 時間: 2025-3-24 21:15 作者: 松馳 時間: 2025-3-25 01:21
Perturbations,ed density perturbations. Their physical wavelengths λ. = aλ (where A is the comoving wavelength) scale as the scale factor a, while the horizon size . stays almost constant during inflation. As a consequence, perturbations cross outside the horizon during inflation. The spectrum of density perturba作者: 貴族 時間: 2025-3-25 04:28 作者: 脆弱帶來 時間: 2025-3-25 08:37
Regina H?nchen,Johannes Schnitzer the gravitational coupling G become time-dependent, while keeping the other fundamental constants fixed [295] . Next, the development of this idea by P. Jordan in the following decade took the form of a complete gravitational theory in which G was promoted to the role of a gravitational scalar fiel作者: 進取心 時間: 2025-3-25 14:14 作者: Aromatic 時間: 2025-3-25 16:58 作者: calorie 時間: 2025-3-25 22:54 作者: Genistein 時間: 2025-3-26 00:47
https://doi.org/10.1007/978-1-4020-1989-0Cosmology; Dust solution; EFE; Gravity; Relativity; Universe; general relativity作者: Detonate 時間: 2025-3-26 04:44
978-90-481-6564-3Springer Science+Business Media Dordrecht 2004作者: Prologue 時間: 2025-3-26 09:02
Cosmology in Scalar-Tensor Gravity978-1-4020-1989-0Series ISSN 0168-1222 Series E-ISSN 2365-6425 作者: 啪心兒跳動 時間: 2025-3-26 15:29 作者: 濕潤 時間: 2025-3-26 19:48 作者: 后天習得 時間: 2025-3-26 21:55 作者: chiropractor 時間: 2025-3-27 01:55
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作者: 眉毛 時間: 2025-3-27 05:27
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作者: 是剝皮 時間: 2025-3-27 10:13 作者: 阻塞 時間: 2025-3-27 15:36
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作者: Pulmonary-Veins 時間: 2025-3-27 20:53 作者: 出沒 時間: 2025-3-28 00:29 作者: Genistein 時間: 2025-3-28 02:47
Fundamental Theories of Physicshttp://image.papertrans.cn/c/image/238934.jpg作者: Amplify 時間: 2025-3-28 08:24 作者: alabaster 時間: 2025-3-28 13:38
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作者: Gerontology 時間: 2025-3-28 15:30
,überblick: Bildungskatastrophe und PISA-Schock – eine , zwischen Selbstvergewisserung und Ausnahmezen, dass immer einige Begriffe aufscheinen, die für einen gewissen Zeitraum zu Schlagw?rtern avancieren und gleichsam die Funktion einer Maxime übernehmen. Innerhalb eines gewissen Zeitraums organisieren sich die unterschiedlichen Str?nge einer Debatte um diese Begriffe herum und verleihen ihnen som作者: gimmick 時間: 2025-3-28 22:17
results of enterprise architecting.Questions standard approaThis book is positioned as a rst in a series of books on enterprise architecture needed for a Master of Enterprise Architecture program, and is targeted both at university students and practitioners with a drive to increase their understand作者: Benzodiazepines 時間: 2025-3-29 02:22