Correlated gravitational wave and microlensing signals of macroscopic dark matter
Abstract Fermion dark matter particles can aggregate to form extended dark matter structures via a first-order phase transition in which the particles get trapped in the false vacuum. We study Fermi balls created in a phase transition induced by a generic quartic thermal effective potential. We show...
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2021
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oai:doaj.org-article:f291bcca85c74dc6afd0024839abfcc92021-11-14T12:41:17ZCorrelated gravitational wave and microlensing signals of macroscopic dark matter10.1007/JHEP11(2021)0681029-8479https://doaj.org/article/f291bcca85c74dc6afd0024839abfcc92021-11-01T00:00:00Zhttps://doi.org/10.1007/JHEP11(2021)068https://doaj.org/toc/1029-8479Abstract Fermion dark matter particles can aggregate to form extended dark matter structures via a first-order phase transition in which the particles get trapped in the false vacuum. We study Fermi balls created in a phase transition induced by a generic quartic thermal effective potential. We show that for Fermi balls of mass, 3 × 10 −12 M ⊙ ≲ M FB ≲ 10 −5 M ⊙, correlated observations of gravitational waves produced during the phase transition (at SKA/THEIA/μAres), and gravitational microlensing caused by Fermi balls (at Subaru-HSC), can be made.Danny MarfatiaPo-Yan TsengSpringerOpenarticleDark matterPhase transitionsOther experimentsNuclear and particle physics. Atomic energy. RadioactivityQC770-798ENJournal of High Energy Physics, Vol 2021, Iss 11, Pp 1-16 (2021) |
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Dark matter Phase transitions Other experiments Nuclear and particle physics. Atomic energy. Radioactivity QC770-798 |
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Dark matter Phase transitions Other experiments Nuclear and particle physics. Atomic energy. Radioactivity QC770-798 Danny Marfatia Po-Yan Tseng Correlated gravitational wave and microlensing signals of macroscopic dark matter |
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Abstract Fermion dark matter particles can aggregate to form extended dark matter structures via a first-order phase transition in which the particles get trapped in the false vacuum. We study Fermi balls created in a phase transition induced by a generic quartic thermal effective potential. We show that for Fermi balls of mass, 3 × 10 −12 M ⊙ ≲ M FB ≲ 10 −5 M ⊙, correlated observations of gravitational waves produced during the phase transition (at SKA/THEIA/μAres), and gravitational microlensing caused by Fermi balls (at Subaru-HSC), can be made. |
format |
article |
author |
Danny Marfatia Po-Yan Tseng |
author_facet |
Danny Marfatia Po-Yan Tseng |
author_sort |
Danny Marfatia |
title |
Correlated gravitational wave and microlensing signals of macroscopic dark matter |
title_short |
Correlated gravitational wave and microlensing signals of macroscopic dark matter |
title_full |
Correlated gravitational wave and microlensing signals of macroscopic dark matter |
title_fullStr |
Correlated gravitational wave and microlensing signals of macroscopic dark matter |
title_full_unstemmed |
Correlated gravitational wave and microlensing signals of macroscopic dark matter |
title_sort |
correlated gravitational wave and microlensing signals of macroscopic dark matter |
publisher |
SpringerOpen |
publishDate |
2021 |
url |
https://doaj.org/article/f291bcca85c74dc6afd0024839abfcc9 |
work_keys_str_mv |
AT dannymarfatia correlatedgravitationalwaveandmicrolensingsignalsofmacroscopicdarkmatter AT poyantseng correlatedgravitationalwaveandmicrolensingsignalsofmacroscopicdarkmatter |
_version_ |
1718429082937458688 |