Finite-Size Dark Matter and its Effect on Small-Scale Structure
Abstract
If dark matter has a finite size that is larger than its Compton wavelength, the corresponding self-interaction cross section decreases with the velocity. We investigate the implications of this puffy dark matter for addressing the small-scale problems of the Λ cold dark matter model and show that the way the nonrelativistic cross section varies with the velocity is largely independent of the dark matter internal structure. Even in the presence of a light particle mediating self-interactions, we find that the finite-size effect may dominate the velocity dependence. We present an explicit example in the context of a QCD-like theory and discuss possible ways to differentiate puffy dark matter from the usual light-mediator scenarios. Particularly relevant for this are low-threshold direct-detection experiments and indirect signatures associated with the internal structure of dark matter.
- Authors:
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- OSTI Identifier:
- 1595515
- Alternate Identifier(s):
- OSTI ID: 1737595
- Grant/Contract Number:
- AC02-05CH11231
- Resource Type:
- Published Article
- Journal Name:
- Physical Review Letters
- Additional Journal Information:
- Journal Name: Physical Review Letters Journal Volume: 124 Journal Issue: 4; Journal ID: ISSN 0031-9007
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Bound states; evolution of the universe; particle astrophysics; particle dark matter
Citation Formats
Chu, Xiaoyong, Garcia-Cely, Camilo, and Murayama, Hitoshi. Finite-Size Dark Matter and its Effect on Small-Scale Structure. United States: N. p., 2020.
Web. doi:10.1103/PhysRevLett.124.041101.
Chu, Xiaoyong, Garcia-Cely, Camilo, & Murayama, Hitoshi. Finite-Size Dark Matter and its Effect on Small-Scale Structure. United States. https://doi.org/10.1103/PhysRevLett.124.041101
Chu, Xiaoyong, Garcia-Cely, Camilo, and Murayama, Hitoshi. Tue .
"Finite-Size Dark Matter and its Effect on Small-Scale Structure". United States. https://doi.org/10.1103/PhysRevLett.124.041101.
@article{osti_1595515,
title = {Finite-Size Dark Matter and its Effect on Small-Scale Structure},
author = {Chu, Xiaoyong and Garcia-Cely, Camilo and Murayama, Hitoshi},
abstractNote = {If dark matter has a finite size that is larger than its Compton wavelength, the corresponding self-interaction cross section decreases with the velocity. We investigate the implications of this puffy dark matter for addressing the small-scale problems of the Λ cold dark matter model and show that the way the nonrelativistic cross section varies with the velocity is largely independent of the dark matter internal structure. Even in the presence of a light particle mediating self-interactions, we find that the finite-size effect may dominate the velocity dependence. We present an explicit example in the context of a QCD-like theory and discuss possible ways to differentiate puffy dark matter from the usual light-mediator scenarios. Particularly relevant for this are low-threshold direct-detection experiments and indirect signatures associated with the internal structure of dark matter.},
doi = {10.1103/PhysRevLett.124.041101},
journal = {Physical Review Letters},
number = 4,
volume = 124,
place = {United States},
year = {Tue Jan 28 00:00:00 EST 2020},
month = {Tue Jan 28 00:00:00 EST 2020}
}
https://doi.org/10.1103/PhysRevLett.124.041101
Web of Science
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