Dark matter self-interactions and small scale structure

Tulin, Sean; Yu, Hai-Bo

doi:10.1016/j.physrep.2017.11.004

Title: Dark matter self-interactions and small scale structure

Journal Article · Tue Dec 05 00:00:00 EST 2017 · Physics Reports

DOI:https://doi.org/10.1016/j.physrep.2017.11.004· OSTI ID:1538743

^[1]; Yu, Hai-Bo ^[2]

York University, Toronto, ON (Canada)
University of California, Riverside, CA (United States)

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.

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Research Organization:: Univ. of California, Riverside, CA (United States)

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: SC0008541; de-sc0008541 (HBY)

OSTI ID:: 1538743

Alternate ID(s):: OSTI ID: 1548928

Journal Information:: Physics Reports, Vol. 730, Issue C; ISSN 0370-1573

Publisher:: ElsevierCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 535 works

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