Gravitational waves from dark matter isocurvature

DOI10.1088/1475-7516/2022/03/023zbMath1504.83003arXiv2112.10163OpenAlexW4221071248WikidataQ114824739 ScholiaQ114824739MaRDI QIDQ5099192

Guillem Domènech, Samuel Passaglia, Sébastien Renaux-Petel

Publication date: 31 August 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2112.10163

zbMATH Keywords

cosmological perturbation theoryprimordial gravitational waves (theory)

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Asymptotic expansions of solutions to PDEs (35C20) Constrained dynamics, Dirac's theory of constraints (70H45) Methods of global Riemannian geometry, including PDE methods; curvature restrictions (53C21) Gravitational waves (83C35) Statistical thermodynamics (82B30) Traveling wave solutions (35C07)

Related Items (5)

The interplay between the dark matter axion and primordial black holes ⋮ Primordial stochastic gravitational wave backgrounds from a sharp feature in three-field inflation. Part I. The radiation era ⋮ Primordial black holes and gravitational waves from non-canonical inflation ⋮ Primordial black holes and gravitational waves induced by exponential-tailed perturbations ⋮ Primordial gravitational waves from excited states

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