Self-interacting dark matter and small-scale gravitational lenses in galaxy clusters

Recently, Meneghetti et al. reported an excess of small-scale gravitational lenses in galaxy clusters. We study its implications for self-interacting dark matter (SIDM) compared with standard cold dark matter (CDM). We design controlled N-body simulations that incorporate observational constraints....

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Vydáno v:Physical review. D Ročník 104; číslo 10
Hlavní autoři: Yang, Daneng, Yu, Hai-Bo
Médium: Journal Article
Jazyk:angličtina
Vydáno: United States American Physical Society (APS) 01.11.2021
Témata:
ASTRONOMY AND ASTROPHYSICS
ATOMIC AND MOLECULAR PHYSICS
Dark matter
ISSN:2470-0010, 2470-0029
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Abstract Recently, Meneghetti et al. reported an excess of small-scale gravitational lenses in galaxy clusters. We study its implications for self-interacting dark matter (SIDM) compared with standard cold dark matter (CDM). We design controlled N-body simulations that incorporate observational constraints. The presence of early-type galaxies in cluster substructures can deepen gravitational potential and reduce tidal mass loss. Both scenarios require a relatively high baryon concentration in the substructure to accommodate the lensing measurements, and their tangential caustics are similar. The SIDM substructure can experience gravothermal collapse and produce a steeper density profile than its CDM counterpart, leading to a larger radial galaxy-galaxy strong-lensing cross section, although this effect is hard to observe. Our results indicate that SIDM can provide a unified explanation to small-scale lenses in galaxy clusters and stellar motion in dwarf galaxies.
AbstractList Recently, Meneghetti et al. reported an excess of small-scale gravitational lenses in galaxy clusters. We study its implications for self-interacting dark matter (SIDM) compared with standard cold dark matter (CDM). We design controlled N-body simulations that incorporate observational constraints. The presence of early-type galaxies in cluster substructures can deepen gravitational potential and reduce tidal mass loss. Both scenarios require a relatively high baryon concentration in the substructure to accommodate the lensing measurements, and their tangential caustics are similar. The SIDM substructure can experience gravothermal collapse and produce a steeper density profile than its CDM counterpart, leading to a larger radial galaxy-galaxy strong-lensing cross section, although this effect is hard to observe. Our results indicate that SIDM can provide a unified explanation to small-scale lenses in galaxy clusters and stellar motion in dwarf galaxies.
ArticleNumber 103031
Author Yu, Hai-Bo
Yang, Daneng
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  surname: Yu
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BackLink https://www.osti.gov/servlets/purl/1979953$$D View this record in Osti.gov
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Snippet Recently, Meneghetti et al. reported an excess of small-scale gravitational lenses in galaxy clusters. We study its implications for self-interacting dark...
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SubjectTerms ASTRONOMY AND ASTROPHYSICS
ATOMIC AND MOLECULAR PHYSICS
Dark matter
Title Self-interacting dark matter and small-scale gravitational lenses in galaxy clusters
URI https://www.osti.gov/servlets/purl/1979953
Volume 104
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