Neutrino self-interactions: A white paper

JM Berryman, N Blinov, V Brdar, T Brinckmann… - Physics of the Dark …, 2023 - Elsevier
Abstract Neutrinos are the Standard Model (SM) particles which we understand the least,
often due to how weakly they interact with the other SM particles. Beyond this, very little is …

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 …

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 …

Gravitational waves from inflation

MC Guzzetti, N Bartolo, M Liguori… - La Rivista del Nuovo …, 2016 - Springer
The production of a stochastic background of gravitational waves is a fundamental
prediction of any cosmological inflationary model. The features of such a signal encode …

[KÖNYV][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 …

Dynamics of phase transition in the new inflationary universe scenario and generation of perturbations

AA Starobinsky - Physics Letters B, 1982 - Elsevier
Dynamics of non-equilibrium phase transition in the early universe is investigated. The
transition is triggered by vacuum fluctuations of a Higgs scalar field which determine the …

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 …

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 …

The development of irregularities in a single bubble inflationary universe

SW Hawking - Physics Letters B, 1982 - Elsevier
The horizon, flatness and monopole problems can be solved if the universe underwent an
exponentially expanding stage which ended with a Higgs scalar field running slowly down …

Dark quark nuggets

Y Bai, AJ Long, S Lu - Physical Review D, 2019 - APS
“Dark quark nuggets,” a lump of dark quark matter, can be produced in the early universe for
a wide range of confining gauge theories and serve as a macroscopic dark matter …