[HTML][HTML] String cosmology: from the early universe to today

M Cicoli, JP Conlon, A Maharana, S Parameswaran… - Physics Reports, 2024 - Elsevier
We review applications of string theory to cosmology, from primordial times to the present-
day accelerated expansion. Starting with a brief overview of cosmology and string …

Cosmology with the laser interferometer space antenna

P Auclair, D Bacon, T Baker, T Barreiro… - Living Reviews in …, 2023 - Springer
Abstract The Laser Interferometer Space Antenna (LISA) has two scientific objectives of
cosmological focus: to probe the expansion rate of the universe, and to understand …

Constraints on primordial black holes

B Carr, K Kohri, Y Sendouda… - Reports on Progress in …, 2021 - iopscience.iop.org
We update the constraints on the fraction of the Universe that may have gone into primordial
black holes (PBHs) over the mass range 10− 5 to 10 50 g. Those smaller than∼ 10 15 g …

Constraints on cosmic strings using data from the third advanced LIGO–virgo observing run

R Abbott, TD Abbott, S Abraham, F Acernese, K Ackley… - Physical review …, 2021 - APS
We search for gravitational-wave signals produced by cosmic strings in the Advanced LIGO
and Virgo full O3 dataset. Search results are presented for gravitational waves produced by …

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 …

Stochastic gravitational wave backgrounds

N Christensen - Reports on Progress in Physics, 2018 - iopscience.iop.org
A stochastic background of gravitational waves could be created by the superposition of a
large number of independent sources. The physical processes occurring at the earliest …

Stochastic gravitational-wave backgrounds: Current detection efforts and future prospects

AI Renzini, B Goncharov, AC Jenkins, PM Meyers - Galaxies, 2022 - mdpi.com
The collection of individually resolvable gravitational wave (GW) events makes up a tiny
fraction of all GW signals that reach our detectors, while most lie below the confusion limit …

European pulsar timing array limits on an isotropic stochastic gravitational-wave background

L Lentati, SR Taylor, CMF Mingarelli… - Monthly Notices of …, 2015 - academic.oup.com
We present new limits on an isotropic stochastic gravitational-wave background (GWB)
using a six pulsar data set spanning 18 yr of observations from the 2015 European Pulsar …

Cosmology and fundamental physics with the Euclid satellite

L Amendola, S Appleby, A Avgoustidis, D Bacon… - Living reviews in …, 2018 - Springer
Abstract Euclid is a European Space Agency medium-class mission selected for launch in
2020 within the cosmic vision 2015–2025 program. The main goal of Euclid is to understand …

[HTML][HTML] Encyclopædia inflationaris

J Martin, C Ringeval, V Vennin - Physics of the Dark Universe, 2014 - Elsevier
The current flow of high accuracy astrophysical data, among which are the Cosmic
Microwave Background (CMB) measurements by the Planck satellite, offers an …