Roosevelt
发表于 2025-3-21 18:58:26
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管理员
发表于 2025-3-21 23:44:08
Gravity Beyond General Relativity,ical solutions, culminating in a discussion of two key aspects of the cosmological standard model: .CDM at late times and inflation at early times. In this chapter, we extend that discussion to theories of gravity beyond general relativity, and in particular the theories which will receive our atten
暴行
发表于 2025-3-22 03:49:37
Cosmological Stability of Massive Bigravity, is given a small mass. In particular, by specialising to the dRGT interaction potentials (.) we ensure that the notorious Boulware-Deser ghost mode is absent, and by allowing both metrics to be dynamical and taking the graviton mass to be of the order of the present-day Hubble rate, we can obtain
organism
发表于 2025-3-22 05:03:50
Linear Structure Growth in Massive Bigravitysolutions in Chap. .. In addition to introducing the formalism for cosmological perturbation theory in bigravity, the specific aim of the previous chapter was to identify which models are stable at the linear level and which are not. The natural next step is to use perturbation theory to derive obse
CON
发表于 2025-3-22 08:56:15
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安抚
发表于 2025-3-22 15:30:39
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安抚
发表于 2025-3-22 19:36:20
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国家明智
发表于 2025-3-22 22:14:41
Discussion and Conclusions and cosmological implications of endowing the graviton with a finite mass, leading to theories either of ., in which there is a single, massive graviton, or ., in which two gravitons, one massless and the other massive, interact with each other.
MAIZE
发表于 2025-3-23 03:39:59
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小溪
发表于 2025-3-23 08:44:04
Soziodemographische Struktur der Stichproben this chapter, we extend that discussion to theories of gravity beyond general relativity, and in particular the theories which will receive our attention in this thesis: massive gravity, massive bigravity, and Einstein-aether theory.