Physical Foundations of Cosmology: Gravitational instability in General Relativity

By V. Mukhanov. 2005

1,857 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/723ed2b687df7b49c48707b6d7c7a8d9644cf2e8

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In Astronomy and Astrophysics

1. Xingang Chen
2. D. Baumann
3. L. Senatore
4. M. Zaldarriaga
5. Yi Wang
6. Andrei Linde
7. Liam McAllister
8. E. Komatsu

In Nuclear and High Energy Physics

1. D. Baumann
2. Xingang Chen
3. Andrei Linde
4. Liam McAllister
5. L. Senatore
6. Yi Wang
7. M. Zaldarriaga
8. E. Pajer

Citations in the corpus

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• Gravitational waves from a universe filled with primordial black holes (2020, background): “In a spatially flat background, in the absence of anisotropic stress (Φ = Ψ) and of entropic perturbations, the Einstein equations take the form [55]”
• Non-Abelian Gauge Field Inflation (2011, background): “The metric perturbations may be parameterized in the standard form [2, 3] ds(2) = −(1 + 2A)dt(2) + 2a(∂iB − Si)dxdt + a(2) ( (1− 2C)δij + 2∂ijE + 2∂(iWj) + hij ) dxdx , (V.”
• The pre-inflationary dynamics of loop quantum cosmology: confronting quantum gravity with observations (2012, neutral): “[3] V.”
• Inflationary schism after Planck2013 (2014, background): “One is the inflationary paradigm described in textbooks [4, 5], which we will call classic inflation.”
• Extension of the quantum theory of cosmological perturbations to the Planck era (2012, methodology): “, [3–6].”
• Inflation, Cosmic Perturbations and Non-Gaussianities (2013, background): “[14] V.”
• Inflation and String Theory (2014, background): “This calculation has become textbook material [57, 58] and can also be found in many reviews (e.”
• Gravitational waves induced by scalar perturbations during a gradual transition from an early matter era to the radiation era (2019, background): “e and denote the energy density perturbation and the velocity divergence [36,38], respectively, and we have neglected the anisotropic stress of radiation. In addition, the derivative of is given by [39], 0= k2 + 3 H2 + 3 2H 2 ˆm ˆtot m + ˆr ˆtot r 3H ; (3.7) where ˆ tot = ˆ m + ˆ r. Figure1shows”
• The Effective Field Theorist's Approach to Gravitational Dynamics (2016, background): “Finally, the EFT of LSS is stochastic in nature, since we only have a statistical description of the initial conditions, plausibly originating from an early phase of accelerated expansion [320].”
• Axions and the Strong CP Problem (2008, background): “…angle at Tc.] In most regions of the phase transition space, a time scale ∆t is needed for the sound wave of quark bilinears to propagate to a large distance, which releases the latent heat to keep the constant temperature during the first order phase transition in [277, Mukhanov (2005), p.149].”
• Primordial Non-Gaussianities from Inflation Models (2010, background): “The introductions to inflation and density perturbations can be found in many textbooks [15–20] and reviews [21–25].”