Baryon-Interacting Dark Matter: heating dark matter and the emergence of galaxy scaling relations

Famaey, Benoit; Khoury, Justin; Penco, Riccardo; Sharma, Anushrut

doi:10.1088/1475-7516/2020/06/025

Baryon-Interacting Dark Matter: heating dark matter and the emergence of galaxy scaling relations

Journal Article · Fri Jun 12 00:00:00 EDT 2020 · Journal of Cosmology and Astroparticle Physics

DOI:https://doi.org/10.1088/1475-7516/2020/06/025· OSTI ID:1802503

Famaey, Benoit ^[1]; Khoury, Justin ^[2]; Penco, Riccardo ^[3]; Sharma, Anushrut ^[2]

Universite de Strasbourg (France). Centre National de la Recherche Scientifique (CNRS). Observatorie astronomique de Strasbourg; OSTI
Univ. of Pennsylvania, Philadelphia, PA (United States). Center for particle Cosmology
Carnegie Mellon Univ., Pittsburgh, PA (United States). Dept. of Physics. McWilliams Center for Cosmology

The empirical scaling relations observed in disk galaxies remain challenging for models of galaxy formation. The most striking among these is the Mass Discrepancy-Acceleration Relation (MDAR), which encodes both a tight baryonic Tully-Fisher relation (BTFR) and the observed diversity of galaxy rotation curves through the central surface density relation (CSDR). Building on our earlier work [1], we propose here that the MDAR is the result of interactions between baryons and ‘Baryon-Interacting Dark Matter’ (BIDM), which heat up the dark matter. Following a bottom-up, hydrodynamical approach, we find that the MDAR follows if: i) the BIDM equation of state approximates that of an ideal gas; ii) the BIDM relaxation time is order the Jeans time; iii) the heating rate is inversely proportional to the BIDM density. Remarkably, under these assumptions the set of hydrodynamical equations together with Poisson’s equation enjoy an anisotropic scaling symmetry. In the BIDM-dominated regime, this gives rise to an enhanced symmetry which fully captures the low-acceleration limit of the MDAR. We then show that, assuming a cored pseudo-isothermal profile at equilibrium, this set of equations gives rise to parameters reproducing the MDAR. Specifically, in the flat part of the rotation curve the asymptotic rotational velocity matches the parametric dependence of the BTFR. Moreover, in the central region of high-surface brightness galaxies, the profile reproduces the CSDR. Finally, by studying the time-dependent approach to equilibrium, we derive a global combination of the BTFR and CSDR, which matches the expectations in low surface-brightness galaxies. The form of the heating rate also makes model-independent predictions for various cosmological observables. We argue that our scenario satisfies existing observational constraints, and, intriguingly, offers a possible explanation to the EDGES anomaly.

View Accepted Manuscript (DOE)

Research Organization:: Univ. of Pennsylvania, Philadelphia, PA (United States)

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: SC0013528

OSTI ID:: 1802503

Alternate ID(s):: OSTI ID: 23041208

Journal Information:: Journal of Cosmology and Astroparticle Physics, Journal Name: Journal of Cosmology and Astroparticle Physics Journal Issue: 06 Vol. 2020; ISSN 1475-7516

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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The Relation Between Stellar and Dynamical Surface Densities in the Central Regions of disk Galaxies Lelli, Federico; McGaugh, Stacy S.; Schombert, James M. The Astrophysical Journal, Vol. 827, Issue 1 https://doi.org/10.3847/2041-8205/827/1/L19	journal	August 2016
Λ CDM is Consistent with SPARC Radial Acceleration Relation Keller, B. W.; Wadsley, J. W. The Astrophysical Journal, Vol. 835, Issue 1 https://doi.org/10.3847/2041-8213/835/1/L17	journal	January 2017
Off the Baryonic Tully–Fisher Relation: A Population of Baryon-dominated Ultra-diffuse Galaxies Mancera Piña, Pavel E.; Fraternali, Filippo; Adams, Elizabeth A. K. The Astrophysical Journal, Vol. 883, Issue 2 https://doi.org/10.3847/2041-8213/ab40c7	journal	September 2019

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