Dark matter haloes in the multicomponent model. III. From dwarfs to galaxy clusters

Todoroki, Keita; Medvedev, Mikhail V.

doi:10.1093/mnras/stab3764

Title: Dark matter haloes in the multicomponent model. III. From dwarfs to galaxy clusters

Journal Article · 27 December 2021 · Monthly Notices of the Royal Astronomical Society

DOI: https://doi.org/10.1093/mnras/stab3764 · OSTI ID:1979532

Todoroki, Keita ^[1]; Medvedev, Mikhail V. ^[2]

University of Kansas, Lawrence, KS (United States); Univ. of Kansas, Lawrence, KS (United States)
University of Kansas, Lawrence, KS (United States); Massachusetts Institute of Technology (MIT), Cambridge, MA (United States)

A possibility of DM being multicomponent has a strong implication on resolving decades-long known cosmological problems on small scale. In addition to elastic scattering, the model allows for inelastic interactions, which can be characterized by a ‘velocity kick’ parameter. The simplest 2cDM model with cross-section 0.01 ≲ σ/m < 1cm²g^-1 and the kick velocity V_k≃100kms^-1 have been shown to robustly resolve the missing satellites, core-cusp, and too-big-to-fail problems in N-body cosmological simulations tested on Milky Way (MW)-like haloes of a virial mass ~5 × 10¹¹M_⊙ (Papers I & II). With the aim of further constraining the parameter space available for the 2cDM model, we extend our analysis to dwarf and galaxy cluster haloes with their virial mass of ~10⁷-10⁸ and ~10¹³-10¹⁴M_⊙ ⁠, respectively. We find that σ₀/m ≳ 0.1 cm²g^-1 is preferentially disfavoured for both dwarfs and galaxy cluster haloes in comparison with observations, while σ₀/m = 0.001 cm²g^-1 causes little perceptible difference from that of the CDM counterpart for most of the cross-section’s velocity dependence studied in this work. Our main result is that within the reasonable set of parameters, the 2cDM model can successfully explain the observational trends seen in dwarf galaxy and galaxy cluster haloes, and the model leaves us an open window for other possible alternative DM models.

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Research Organization:: University of Kansas, Lawrence, KS (United States)

Sponsoring Organization:: USDOE Office of Science (SC); National Science Foundation (NSF)

Grant/Contract Number:: SC0016368; SC0019474

OSTI ID:: 1979532

Journal Information:: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 3 Vol. 510; ISSN 0035-8711

Publisher:: Oxford University PressCopyright Statement

Country of Publication:: United States

Language:: English

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