Gravothermal collapse and the diversity of galactic rotation curves

The rotation curves of spiral galaxies exhibit a great diversity that challenges our understanding of galaxy formation and the nature of dark matter. Previous studies showed that in self-interacting dark matter (SIDM) models with a cross section per unit mass of $\ensuremath{\sigma}/m\ensuremath{\approx}\mathcal{O}(1)\text{ }\text{ }{\mathrm{cm}}^{2}/\mathrm{g}$, the predicted dark matter central densities are a good match to the observed densities in galaxies. In this work, we explore a regime with a larger cross section of $\ensuremath{\sigma}/m\ensuremath{\approx}20\ensuremath{-}40\text{ }\text{ }{\mathrm{cm}}^{2}/\mathrm{g}$ in dwarf galactic halos. We will show that such strong dark matter self-interactions can further amplify the diversity of halo densities inherited from their assembly history. High concentration halos can enter the gravothermal collapse phase within 10 Gyr, resulting in a high density, while low concentration ones remain in the expansion phase and have a low density. We fit the rotation curves of 14 representative low surface brightness galaxies and demonstrate how the large range of observed central densities is naturally accommodated in the strong SIDM regime of $\ensuremath{\sigma}/m\ensuremath{\approx}20--40\text{ }\text{ }{\mathrm{cm}}^{2}/\mathrm{g}$. Galaxies that are outliers in the previous studies, due to their high halo central densities, are no longer outliers in this SIDM regime as their halos would be in the collapse phase. For galaxies with a low density, the SIDM fits are robust to the variation of the cross section. Our findings open up a new window for testing gravothermal collapse, the unique signature of strong dark matter self-interactions, and exploring a broader SIDM model space. As an example, we illustrate how the larger cross sections favored by our fits, together with upper limits from strong lensing observations in clusters, pick out the preferred SIDM model space for a dark matter particle coupled to a light gauge boson in the Born regime.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-05-20
DOI
https://doi.org/10.1103/physrevd.111.103041
Citations
12
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
13.86

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article

Gravothermal collapse and the diversity of galactic rotation curves

M. Grant Roberts, Hai-Bo Yu, Mauro Valli, Manoj Kaplinghat
12 citations
Physical review. D/Physical review. D.
Stellar, planetary, and galactic studies
13.86
article

Gravothermal collapse and the diversity of galactic rotation curves

M. Grant Roberts, Hai-Bo Yu, Mauro Valli, Manoj Kaplinghat
article en
12 citations

Abstract

The rotation curves of spiral galaxies exhibit a great diversity that challenges our understanding of galaxy formation and the nature of dark matter. Previous studies showed that in self-interacting dark matter (SIDM) models with a cross section per unit mass of $\ensuremath{\sigma}/m\ensuremath{\approx}\mathcal{O}(1)\text{ }\text{ }{\mathrm{cm}}^{2}/\mathrm{g}$, the predicted dark matter central densities are a good match to the observed densities in galaxies. In this work, we explore a regime with a larger cross section of $\ensuremath{\sigma}/m\ensuremath{\approx}20\ensuremath{-}40\text{ }\text{ }{\mathrm{cm}}^{2}/\mathrm{g}$ in dwarf galactic halos. We will show that such strong dark matter self-interactions can further amplify the diversity of halo densities inherited from their assembly history. High concentration halos can enter the gravothermal collapse phase within 10 Gyr, resulting in a high density, while low concentration ones remain in the expansion phase and have a low density. We fit the rotation curves of 14 representative low surface brightness galaxies and demonstrate how the large range of observed central densities is naturally accommodated in the strong SIDM regime of $\ensuremath{\sigma}/m\ensuremath{\approx}20--40\text{ }\text{ }{\mathrm{cm}}^{2}/\mathrm{g}$. Galaxies that are outliers in the previous studies, due to their high halo central densities, are no longer outliers in this SIDM regime as their halos would be in the collapse phase. For galaxies with a low density, the SIDM fits are robust to the variation of the cross section. Our findings open up a new window for testing gravothermal collapse, the unique signature of strong dark matter self-interactions, and exploring a broader SIDM model space. As an example, we illustrate how the larger cross sections favored by our fits, together with upper limits from strong lensing observations in clusters, pick out the preferred SIDM model space for a dark matter particle coupled to a light gauge boson in the Born regime.

Physical review. D/Physical review. D.Vol. 111(10)
University of California, Riverside (US), University of California, Santa Cruz (US), University of California, Irvine (US), Institute of Particle Physics (CA), Istituto Nazionale di Fisica Nucleare, Sezione di Roma I (IT)
National Science Foundation, U.S. Department of Energy, John Templeton Foundation, Instituto Nazionale di Fisica Nucleare
Climate action
Openalex Percentile: Top 1%
Stellar, planetary, and galactic studies
13.86
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