Dark matter self-interactions and small scale structure
Abstract
We review theories of dark matter (DM) beyond the collisionless paradigm, known as self-interacting dark matter (SIDM), and their observable implications for astrophysical structure in the Universe. Self-interactions are motivated, in part, due to the potential to explain long-standing (and more recent) small scale structure observations that are in tension with collisionless cold DM (CDM) predictions. Simple particle physics models for SIDM can provide a universal explanation for these observations across a wide range of mass scales spanning dwarf galaxies, low and high surface brightness spiral galaxies, and clusters of galaxies. At the same time, SIDM leaves intact the success of $$Λ$$CDM cosmology on large scales. This report covers the following topics: (1) small scale structure issues, including the core–cusp problem, the diversity problem for rotation curves, the missing satellites problem, and the too-big-to-fail problem, as well as recent progress in hydrodynamical simulations of galaxy formation; (2) N-body simulations for SIDM, including implications for density profiles, halo shapes, substructure, and the interplay between baryons and self-interactions; (3) semi-analytic Jeans-based methods that provide a complementary approach for connecting particle models with observations; (4) merging systems, such as cluster mergers (e.g., the Bullet Cluster) and minor infalls, along with recent simulation results for mergers; (5) particle physics models, including light mediator models and composite DM models; and (6) complementary probes for SIDM, including indirect and direct detection experiments, particle collider searches, and cosmological observations. In conclusion, we provide a summary and critical look for all current constraints on DM self-interactions and an outline for future directions.
- Authors:
-
[1];
- York University, Toronto, ON (Canada)
- University of California, Riverside, CA (United States)
- Publication Date:
- Research Org.:
- Univ. of California, Riverside, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC)
- OSTI Identifier:
- 1538743
- Alternate Identifier(s):
- OSTI ID: 1548928
- Grant/Contract Number:
- SC0008541; de-sc0008541 (HBY)
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physics Reports
- Additional Journal Information:
- Journal Volume: 730; Journal Issue: C; Journal ID: ISSN 0370-1573
- Publisher:
- Elsevier
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Physics
Citation Formats
Tulin, Sean, and Yu, Hai-Bo. Dark matter self-interactions and small scale structure. United States: N. p., 2017.
Web. doi:10.1016/j.physrep.2017.11.004.
Tulin, Sean, & Yu, Hai-Bo. Dark matter self-interactions and small scale structure. United States. https://doi.org/10.1016/j.physrep.2017.11.004
Tulin, Sean, and Yu, Hai-Bo. Tue .
"Dark matter self-interactions and small scale structure". United States. https://doi.org/10.1016/j.physrep.2017.11.004. https://www.osti.gov/servlets/purl/1538743.
@article{osti_1538743,
title = {Dark matter self-interactions and small scale structure},
author = {Tulin, Sean and Yu, Hai-Bo},
abstractNote = {We review theories of dark matter (DM) beyond the collisionless paradigm, known as self-interacting dark matter (SIDM), and their observable implications for astrophysical structure in the Universe. Self-interactions are motivated, in part, due to the potential to explain long-standing (and more recent) small scale structure observations that are in tension with collisionless cold DM (CDM) predictions. Simple particle physics models for SIDM can provide a universal explanation for these observations across a wide range of mass scales spanning dwarf galaxies, low and high surface brightness spiral galaxies, and clusters of galaxies. At the same time, SIDM leaves intact the success of $Λ$CDM cosmology on large scales. This report covers the following topics: (1) small scale structure issues, including the core–cusp problem, the diversity problem for rotation curves, the missing satellites problem, and the too-big-to-fail problem, as well as recent progress in hydrodynamical simulations of galaxy formation; (2) N-body simulations for SIDM, including implications for density profiles, halo shapes, substructure, and the interplay between baryons and self-interactions; (3) semi-analytic Jeans-based methods that provide a complementary approach for connecting particle models with observations; (4) merging systems, such as cluster mergers (e.g., the Bullet Cluster) and minor infalls, along with recent simulation results for mergers; (5) particle physics models, including light mediator models and composite DM models; and (6) complementary probes for SIDM, including indirect and direct detection experiments, particle collider searches, and cosmological observations. In conclusion, we provide a summary and critical look for all current constraints on DM self-interactions and an outline for future directions.},
doi = {10.1016/j.physrep.2017.11.004},
journal = {Physics Reports},
number = C,
volume = 730,
place = {United States},
year = {Tue Dec 05 00:00:00 EST 2017},
month = {Tue Dec 05 00:00:00 EST 2017}
}
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Works referencing / citing this record:
A universal constant for dark matter-baryon interplay
journal, March 2019
- Chan, Man Ho
- Scientific Reports, Vol. 9, Issue 1