標(biāo)題: Titlebook: Generalized Perturbations in Modified Gravity and Dark Energy; Jonathan Pearson Book 2014 Springer International Publishing Switzerland 20 [打印本頁(yè)] 作者: magnify 時(shí)間: 2025-3-21 20:04
書目名稱Generalized Perturbations in Modified Gravity and Dark Energy影響因子(影響力)
書目名稱Generalized Perturbations in Modified Gravity and Dark Energy影響因子(影響力)學(xué)科排名
書目名稱Generalized Perturbations in Modified Gravity and Dark Energy網(wǎng)絡(luò)公開度
書目名稱Generalized Perturbations in Modified Gravity and Dark Energy網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Generalized Perturbations in Modified Gravity and Dark Energy被引頻次
書目名稱Generalized Perturbations in Modified Gravity and Dark Energy被引頻次學(xué)科排名
書目名稱Generalized Perturbations in Modified Gravity and Dark Energy年度引用
書目名稱Generalized Perturbations in Modified Gravity and Dark Energy年度引用學(xué)科排名
書目名稱Generalized Perturbations in Modified Gravity and Dark Energy讀者反饋
書目名稱Generalized Perturbations in Modified Gravity and Dark Energy讀者反饋學(xué)科排名
作者: CYN 時(shí)間: 2025-3-21 20:35
(Re)Presenting Sherlock Holmes,for parameters which have a “l(fā)arge” effect on observables on “small” scales. It is rather unfortunate, however, that it is most natural for dark sector theories to induce modifications on large scales, since it is only at late times when the dark sector dominates when those large scale modes cross the horizon.作者: Kinetic 時(shí)間: 2025-3-22 01:38 作者: EXUDE 時(shí)間: 2025-3-22 06:50
Observational Signatures of Generalized Cosmological Perturbations,for parameters which have a “l(fā)arge” effect on observables on “small” scales. It is rather unfortunate, however, that it is most natural for dark sector theories to induce modifications on large scales, since it is only at late times when the dark sector dominates when those large scale modes cross the horizon.作者: 食草 時(shí)間: 2025-3-22 10:45 作者: 紡織品 時(shí)間: 2025-3-22 15:26 作者: 紡織品 時(shí)間: 2025-3-22 17:37
https://doi.org/10.1007/978-3-319-72523-9urbations. However, the formalism can be applied in much more diverse systems where relativistic field theories play a central role, such as massive gravities, inflation and even effective theories for quantum gravity.作者: 嬰兒 時(shí)間: 2025-3-22 23:19 作者: 草率男 時(shí)間: 2025-3-23 03:19 作者: 放逐 時(shí)間: 2025-3-23 06:46
The Effective Action Formalism for Cosmological Perturbations,, supernovae, baryon acoustic oscillations, gravitational lensing and structure formation point to the existence of an additional component dubbed “dark energy”, or a modification to gravity, which needs to be introduced to explain the the observed acceleration [1–5].作者: profligate 時(shí)間: 2025-3-23 10:54
High Derivative Theories,urbations. However, the formalism can be applied in much more diverse systems where relativistic field theories play a central role, such as massive gravities, inflation and even effective theories for quantum gravity.作者: Muffle 時(shí)間: 2025-3-23 14:30 作者: FIN 時(shí)間: 2025-3-23 20:55 作者: Trabeculoplasty 時(shí)間: 2025-3-24 02:12
Book 2014is thesis the author constructs a unifying framework for understanding the observational impact of general classes of dark sector theories, by formulating equations of state for the dark sector perturbations.作者: acheon 時(shí)間: 2025-3-24 04:20 作者: sinoatrial-node 時(shí)間: 2025-3-24 08:35
Introduction to Gravitational Theories and Cosmology,eps objects firmly planted on the surface of the earth. Whilst gravity is the weakest of the fundamental forces, it is gravity which dictates the structure and shape of the universe on a vast range of scales.作者: hankering 時(shí)間: 2025-3-24 13:31
The Effective Action Formalism for Cosmological Perturbations,he geometry and matter content of cold dark matter (CDM)/photons/baryons to describe its constituents. Observations of the cosmic microwave background, supernovae, baryon acoustic oscillations, gravitational lensing and structure formation point to the existence of an additional component dubbed “da作者: Ibd810 時(shí)間: 2025-3-24 18:40 作者: 控訴 時(shí)間: 2025-3-24 22:52
High Derivative Theories,sistent modifications to the gravitational field equations at perturbed order for modified gravity and dark energy theories from a Lagrangian for perturbations. However, the formalism can be applied in much more diverse systems where relativistic field theories play a central role, such as massive g作者: FISC 時(shí)間: 2025-3-25 00:15
Connections to Massive Gravity,or what has become called .. In this paper we will focus on what is the simplest subset of such theories, in which the dark sector Lagrangian is only a function of the metric (and no extra derivatives thereof) following the approach discussed in [.]作者: enchant 時(shí)間: 2025-3-25 06:46 作者: 胎兒 時(shí)間: 2025-3-25 10:52 作者: 魔鬼在游行 時(shí)間: 2025-3-25 11:54 作者: Thyroiditis 時(shí)間: 2025-3-25 19:06 作者: 搖擺 時(shí)間: 2025-3-25 20:15
Generalized Perturbations in Modified Gravity and Dark Energy978-3-319-01210-0Series ISSN 2190-5053 Series E-ISSN 2190-5061 作者: 持續(xù) 時(shí)間: 2025-3-26 00:25 作者: beta-cells 時(shí)間: 2025-3-26 05:38
Explicit Theories,In this chapter we will provide expressions for the coupling coefficients in the Lagrangian for perturbations for explicit theories, as well as the values of the functions which appear in the (.) decomposition of the coupling coefficients. This will show the existence of a mapping between generalized and explicit theories.作者: Recessive 時(shí)間: 2025-3-26 10:20
Jonathan PearsonNominated as an outstanding Ph.D. thesis by the University of Manchester, UK.Offers a clear and pedagogical introduction to General Relativity, Cosmology and Modified Gravity.Presents physical interpr作者: 強(qiáng)有力 時(shí)間: 2025-3-26 16:14 作者: Sedative 時(shí)間: 2025-3-26 20:49 作者: BRIDE 時(shí)間: 2025-3-26 21:14 作者: CANE 時(shí)間: 2025-3-27 03:53 作者: BET 時(shí)間: 2025-3-27 07:45 作者: extinct 時(shí)間: 2025-3-27 09:39
Connections to Massive Gravity,or what has become called .. In this paper we will focus on what is the simplest subset of such theories, in which the dark sector Lagrangian is only a function of the metric (and no extra derivatives thereof) following the approach discussed in [.]作者: Incumbent 時(shí)間: 2025-3-27 17:38 作者: 完全 時(shí)間: 2025-3-27 20:34
Relation to Dialects and to the Foreigner,eps objects firmly planted on the surface of the earth. Whilst gravity is the weakest of the fundamental forces, it is gravity which dictates the structure and shape of the universe on a vast range of scales.作者: 手段 時(shí)間: 2025-3-27 22:34 作者: 臥虎藏龍 時(shí)間: 2025-3-28 04:16 作者: Palpitation 時(shí)間: 2025-3-28 08:12 作者: Herbivorous 時(shí)間: 2025-3-28 11:18
Ben P. White,Lindy Willmott,Eliana Closeor what has become called .. In this paper we will focus on what is the simplest subset of such theories, in which the dark sector Lagrangian is only a function of the metric (and no extra derivatives thereof) following the approach discussed in [.]作者: 誘拐 時(shí)間: 2025-3-28 16:36
Peter Winker,Jianbin Chen,Dennis K. J. Linar field contents of the dark sector. All modifications to the equations governing perturbations are contained within . and the perturbed fluid equations. In this chapter we rewrite some of these results to obtain what we call .. As the name suggests, these equations of state for perturbations play 作者: Vsd168 時(shí)間: 2025-3-28 21:23 作者: Muscularis 時(shí)間: 2025-3-28 23:56
Fascinated Disgust in Richard Powers,ul theories. The approach requires a field content, but does not require a particular Lagrangian to be presented for calculations to be performed. Once the field content has been specified we have shown how to write down an effective action for linearized perturbations, and from that how to compute 作者: Enrage 時(shí)間: 2025-3-29 06:18
https://doi.org/10.1007/978-3-322-83579-6Gesellschaft; Ideologie; Individuum; Institution; Macht; Struktur; Umwelt; Verschiedenheit; Vertrauen作者: RAGE 時(shí)間: 2025-3-29 09:19
