Theory of cosmological perturbations

VF Mukhanov, HA Feldman, RH Brandenberger - Physics reports, 1992 - Elsevier
We present in a manifestly gauge-invariant form the theory of classical linear gravitational
perturbations in part I, and a quantum theory of cosmological perturbations in part II. Part I …

Cosmological backgrounds of gravitational waves

C Caprini, DG Figueroa - Classical and Quantum Gravity, 2018 - iopscience.iop.org
Gravitational waves (GWs) have a great potential to probe cosmology. We review early
universe sources that can lead to cosmological backgrounds of GWs. We begin by …

[BOOK][B] The early universe

E Kolb - 2018 - taylorfrancis.com
The Early Universe has become the standard reference on forefront topics in cosmology,
particularly to the early history of the Universe. Subjects covered include primordial …

Cosmology of the invisible axion

J Preskill, MB Wise, F Wilczek - Physics Letters B, 1983 - Elsevier
We identify a new cosmological problem for models which solve the strong CP puzzle with
an invisible axion, unrelated to the domain wall problem. Because the axion is very weakly …

Spontaneous creation of almost scale-free density perturbations in an inflationary universe

JM Bardeen, PJ Steinhardt, MS Turner - Physical Review D, 1983 - APS
The creation and evolution of energy-density perturbations are analyzed for the" new
inflationary universe" scenario proposed by Linde, and Albrecht and Steinhardt. According …

Towards the theory of reheating after inflation

L Kofman, A Linde, AA Starobinsky - Physical Review D, 1997 - APS
Reheating after inflation occurs due to particle production by the oscillating inflaton field. In
this paper we briefly describe the perturbative approach to reheating, and then concentrate …

Reheating after inflation

L Kofman, A Linde, AA Starobinsky - Physical Review Letters, 1994 - APS
The theory of reheating of the Universe after inflation is developed. We have found that
typically at the first stage of reheating the classical inflation field φ rapidly decays into φ …

Cosmological perturbation theory

H Kodama, M Sasaki - Progress of Theoretical Physics …, 1984 - academic.oup.com
The linear perturbation theory of spatially homogeneous and isotropic universes is reviewed
and reformulated extensively. In the first half of the article, a gauge-invariant formulation of …

Taiji program: Gravitational-wave sources

WH Ruan, ZK Guo, RG Cai, YZ Zhang - International Journal of …, 2020 - World Scientific
We review potential low-frequency gravitational-wave sources, which are expected to be
detected by Taiji, a Chinese space-based gravitational-wave detector, estimate the detection …

A new mechanism for baryogenesis

I Affleck, M Dine - Nuclear Physics B, 1985 - Elsevier
A new mechanism for baryogenesis is proposed. It is argued that, after inflation, the scalar
quarks and leptons of a supersymmetric GUT may have large expectation values. The …