Theory of cosmological perturbations
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 …
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 …
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 …
particularly to the early history of the Universe. Subjects covered include primordial …
Cosmology of the invisible axion
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 …
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
The creation and evolution of energy-density perturbations are analyzed for the" new
inflationary universe" scenario proposed by Linde, and Albrecht and Steinhardt. According …
inflationary universe" scenario proposed by Linde, and Albrecht and Steinhardt. According …
Towards the theory of reheating after inflation
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 …
this paper we briefly describe the perturbative approach to reheating, and then concentrate …
Reheating after inflation
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 …
typically at the first stage of reheating the classical inflation field φ rapidly decays into φ …
Cosmological perturbation theory
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 …
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 …
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 …
quarks and leptons of a supersymmetric GUT may have large expectation values. The …