Filtered Dark Matter at a First Order Phase Transition
Abstract
We describe a new mechanism of dark matter production. If dark matter particles acquire mass during a first order phase transition, it is energetically unfavorable for them to enter the expanding bubbles. Instead, most of them are reflected and quickly annihilate away. The bubbles eventually merge as the phase transition completes and only the dark matter particles that have entered the bubbles survive to constitute the observed dark matter today. This mechanism can produce dark matter with masses from the TeV scale to above the PeV scale, surpassing the Griest-Kamionkowski bound.
- Authors:
- Publication Date:
- Research Org.:
- Univ. of Michigan, Ann Arbor, MI (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP); Swiss National Science Foundation (SNF); European Research Council (ERC); German Research Foundation (DFG)
- OSTI Identifier:
- 1671365
- Alternate Identifier(s):
- OSTI ID: 1684627
- Grant/Contract Number:
- SC0007859; 200021-159720; 637506; 4820/4
- Resource Type:
- Published Article
- Journal Name:
- Physical Review Letters
- Additional Journal Information:
- Journal Name: Physical Review Letters Journal Volume: 125 Journal Issue: 15; Journal ID: ISSN 0031-9007
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; First order phase transitions; particle dark matter
Citation Formats
Baker, Michael J., Kopp, Joachim, and Long, Andrew J. Filtered Dark Matter at a First Order Phase Transition. United States: N. p., 2020.
Web. doi:10.1103/PhysRevLett.125.151102.
Baker, Michael J., Kopp, Joachim, & Long, Andrew J. Filtered Dark Matter at a First Order Phase Transition. United States. https://doi.org/10.1103/PhysRevLett.125.151102
Baker, Michael J., Kopp, Joachim, and Long, Andrew J. Fri .
"Filtered Dark Matter at a First Order Phase Transition". United States. https://doi.org/10.1103/PhysRevLett.125.151102.
@article{osti_1671365,
title = {Filtered Dark Matter at a First Order Phase Transition},
author = {Baker, Michael J. and Kopp, Joachim and Long, Andrew J.},
abstractNote = {We describe a new mechanism of dark matter production. If dark matter particles acquire mass during a first order phase transition, it is energetically unfavorable for them to enter the expanding bubbles. Instead, most of them are reflected and quickly annihilate away. The bubbles eventually merge as the phase transition completes and only the dark matter particles that have entered the bubbles survive to constitute the observed dark matter today. This mechanism can produce dark matter with masses from the TeV scale to above the PeV scale, surpassing the Griest-Kamionkowski bound.},
doi = {10.1103/PhysRevLett.125.151102},
journal = {Physical Review Letters},
number = 15,
volume = 125,
place = {United States},
year = {Fri Oct 09 00:00:00 EDT 2020},
month = {Fri Oct 09 00:00:00 EDT 2020}
}
Free Publicly Available Full Text
Publisher's Version of Record
https://doi.org/10.1103/PhysRevLett.125.151102
https://doi.org/10.1103/PhysRevLett.125.151102
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Figures / Tables:
FIG. 1: “Filtered DM”: only DM particles $χ$ with kinetic energy $E$ ≳ $m^{in}_{χ}$ can penetrate the bubble; slower particles are reflected. In front of the bubble wall (pink region), DM is kept in thermal equilibrium through $χ\bar{χ}$ ↔ $ϕϕ$, but this reaction is put abruptly out of equilibrium atmore »
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