Astrophysical constraints on dark-matter -balls in the presence of baryon-violating operators
Abstract
Supersymmetric extensions of the standard model predict the existence of non-topological solitons, Q-balls. Assuming the standard cosmological history preceded by inflation, Q-balls can form in the early universe and can make up the dark matter. The relatively large masses of such dark-matter particles imply a low number density, making direct detection very challenging. The strongest limits come from the existence of neutron stars because, if a baryonic Q-ball is captured by a neutron star, the Q-ball can absorb the baryon number releasing energy and eventually destroying a neutron star. Yet, in the presence of baryon number violating higher-dimension operators, the growth of a Q-ball inside a neutron star is hampered once the Q-ball reaches a certain size. We re-examine the limits and identify some classes of higher-dimensional operators for which supersymmetric Q-balls can account for dark matter. The current limits leave a wide range of parameters available for dark matter in the form of supersymmetric Q-balls.
- Authors:
-
- Univ. of California, Los Angeles, CA (United States)
- Univ. of California, Los Angeles, CA (United States); Univ. of Tokyo (Japan). Kavli Institute for the Physics and Mathematics of the Universe (WPI)
- Publication Date:
- Research Org.:
- Univ. of California, Los Angeles, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF)
- OSTI Identifier:
- 1609079
- Alternate Identifier(s):
- OSTI ID: 1335191
- Grant/Contract Number:
- SC0009937; PHY-1066293
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review D
- Additional Journal Information:
- Journal Volume: 94; Journal Issue: 12; Journal ID: ISSN 2470-0010
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
Citation Formats
Cotner, Eric, and Kusenko, Alexander. Astrophysical constraints on dark-matter Q -balls in the presence of baryon-violating operators. United States: N. p., 2016.
Web. doi:10.1103/PhysRevD.94.123006.
Cotner, Eric, & Kusenko, Alexander. Astrophysical constraints on dark-matter Q -balls in the presence of baryon-violating operators. United States. https://doi.org/10.1103/PhysRevD.94.123006
Cotner, Eric, and Kusenko, Alexander. Mon .
"Astrophysical constraints on dark-matter Q -balls in the presence of baryon-violating operators". United States. https://doi.org/10.1103/PhysRevD.94.123006. https://www.osti.gov/servlets/purl/1609079.
@article{osti_1609079,
title = {Astrophysical constraints on dark-matter Q -balls in the presence of baryon-violating operators},
author = {Cotner, Eric and Kusenko, Alexander},
abstractNote = {Supersymmetric extensions of the standard model predict the existence of non-topological solitons, Q-balls. Assuming the standard cosmological history preceded by inflation, Q-balls can form in the early universe and can make up the dark matter. The relatively large masses of such dark-matter particles imply a low number density, making direct detection very challenging. The strongest limits come from the existence of neutron stars because, if a baryonic Q-ball is captured by a neutron star, the Q-ball can absorb the baryon number releasing energy and eventually destroying a neutron star. Yet, in the presence of baryon number violating higher-dimension operators, the growth of a Q-ball inside a neutron star is hampered once the Q-ball reaches a certain size. We re-examine the limits and identify some classes of higher-dimensional operators for which supersymmetric Q-balls can account for dark matter. The current limits leave a wide range of parameters available for dark matter in the form of supersymmetric Q-balls.},
doi = {10.1103/PhysRevD.94.123006},
journal = {Physical Review D},
number = 12,
volume = 94,
place = {United States},
year = {Mon Dec 12 00:00:00 EST 2016},
month = {Mon Dec 12 00:00:00 EST 2016}
}
Web of Science
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Works referencing / citing this record:
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