Origin and detection of nontopological soliton dark matter

Fuente: arXiv
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Auteur principal: Orlofsky, Nicholas
Format: Preprint
Publié: 2024
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author Orlofsky, Nicholas
author_facet Orlofsky, Nicholas
contents Macroscopic dark matter like nontopological solitons can form either via the fusion and accumulation of free particles or during cosmological phase transitions. Both mechanisms can create dark matter with large masses ranging from TeV to solar mass. This can lead to interesting targets in direct detection, astrophysical, and cosmological searches.
format Preprint
id arxiv_https___arxiv_org_abs_2405_09239
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Origin and detection of nontopological soliton dark matter
Orlofsky, Nicholas
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
High Energy Astrophysical Phenomena
Macroscopic dark matter like nontopological solitons can form either via the fusion and accumulation of free particles or during cosmological phase transitions. Both mechanisms can create dark matter with large masses ranging from TeV to solar mass. This can lead to interesting targets in direct detection, astrophysical, and cosmological searches.
title Origin and detection of nontopological soliton dark matter
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2405.09239