2021/12/31 by Guillem Domènech, Samuel Passaglia, Sébastien Renaux‐Petel +1 · 69 citations
Physics and Astronomy · #Adiabatic process #Advanced Thermodynamics and Statistical Mechanics #Astrophysics #Classical mechanics #Cold dark matter #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark matter #Gravitation #Gravitational wave #Observable #Particle physics #Physics #Quantum mechanics #Spectral density #astro-ph.CO #gr-qc
paper · pdf · doi:10.1088/1475-7516/2022/03/023
published in Journal of Cosmology and Astroparticle Physics 2022(03), 023 (Institute of Physics) · 46 page, 9 figures; matches published version
openalex publication_date 2022/03/01 · arxiv created 2022/03/21 · arxiv updated 2022/03/22 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
The primordial fluctuations on large scales are adiabatic, but on smaller scales this need not be the case. Here we derive the general analytical framework to compute the stochastic gravitational wave background induced by primordial cold dark matter isocurvature fluctuations on small scales. We find that large isocurvature fluctuations can yield an observable gravitational wave signal, with a spectrum distinct from the one induced by adiabatic perturbations, and we provide for the first time the exact analytic expression of the kernel necessary to compute this signal. We then forecast the constraining power of future gravitational wave detectors on dark matter isocurvature on small scales and find they will dramatically improve on existing constraints.