Kinetic recoupling of dark matter

Fuente: arXiv
Salvato in:
Dettagli Bibliografici
Autori principali: Lehmann, Benjamin V., Morrison, Logan, Profumo, Stefano, Smyth, Nolan
Natura: Preprint
Pubblicazione: 2023
Soggetti:
Accesso online:
Tags: Aggiungi Tag
Nessun Tag, puoi essere il primo ad aggiungerne!!
_version_ 1866909262581596160
author Lehmann, Benjamin V.
Morrison, Logan
Profumo, Stefano
Smyth, Nolan
author_facet Lehmann, Benjamin V.
Morrison, Logan
Profumo, Stefano
Smyth, Nolan
contents We study the possibility that dark matter re-enters kinetic equilibrium with a radiation bath after kinetic decoupling, a scenario we dub kinetic recoupling. This naturally occurs, for instance, with certain types of resonantly-enhanced interactions, or as the result of a phase transition. While late kinetic decoupling damps structure on small scales below a cutoff, kinetic recoupling produces more complex changes in the power spectrum that depend on the nature and extent of the recoupling period. We explore the features that kinetic recoupling imprints upon the matter power spectrum, and discuss how such features can be traced to dark matter microphysics with future observations.
format Preprint
id arxiv_https___arxiv_org_abs_2310_20513
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Kinetic recoupling of dark matter
Lehmann, Benjamin V.
Morrison, Logan
Profumo, Stefano
Smyth, Nolan
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
We study the possibility that dark matter re-enters kinetic equilibrium with a radiation bath after kinetic decoupling, a scenario we dub kinetic recoupling. This naturally occurs, for instance, with certain types of resonantly-enhanced interactions, or as the result of a phase transition. While late kinetic decoupling damps structure on small scales below a cutoff, kinetic recoupling produces more complex changes in the power spectrum that depend on the nature and extent of the recoupling period. We explore the features that kinetic recoupling imprints upon the matter power spectrum, and discuss how such features can be traced to dark matter microphysics with future observations.
title Kinetic recoupling of dark matter
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2310.20513