The Effect of Dark Matter–Dark Radiation Interactions on Halo Abundance: A Press–Schechter Approach

Sameie, Omid; Benson, Andrew J.; Sales, Laura V.; Yu, Hai-bo; Moustakas, Leonidas A.; Creasey, Peter

doi:10.3847/1538-4357/ab0824

The Effect of Dark Matter–Dark Radiation Interactions on Halo Abundance: A Press–Schechter Approach

Journal Article · Wed Mar 20 04:00:00 EDT 2019 · The Astrophysical Journal (Online)

DOI:https://doi.org/10.3847/1538-4357/ab0824· OSTI ID:1611077

^[1]; ^[2]; Sales, Laura V. ^[3]; Yu, Hai-bo ^[3]; ^[4]; ^[3]

Univ. of California, Riverside, CA (United States). Dept. of Physics and Astronomy; DOE/OSTI
Carnegie Observatories, Pasadena, CA (United States)
Univ. of California, Riverside, CA (United States). Dept. of Physics and Astronomy
California Institute of Technology (CalTech), Pasadena, CA (United States). Jet Propulsion Lab. (JPL)

We study halo mass functions with the Press–Schechter formalism for interacting dark matter models, where matter power spectra are damped due to dark acoustic oscillations in the early universe. After adopting a smooth window function, we calibrate the analytical model with numerical simulations from the "effective theory of structure formation" (ETHOS) project and fix the model parameters in the high-mass regime, M_h ≳ 3 × $${10}^{10}\ {M}_{\odot }$$. We also perform high-resolution cosmological simulations with halo masses down to M_h ~ 10⁸ M_⊙ to cover a wide mass range for comparison. Although the model is calibrated with ETHOS1 and cold dark matter simulations for high halo masses at redshift z = 0, it successfully reproduces simulations for two other ETHOS models in the low-mass regime at low and high redshifts. As an application, we compare the cumulative number density of halos to that of observed galaxies at z = 6, and find that the interacting dark matter models with a kinetic decoupling temperature below 0.5 keV is disfavored. We also perform the abundance-matching analysis and derive the stellar–halo mass relation for these models at z = 4. Suppression in halo abundance leads to less massive halos that host observed galaxies in the stellar mass range $${M}_{* }\simeq {10}^{5}-{10}^{7}\ {M}_{\odot }$$.

View Accepted Manuscript (DOE)

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

Sponsoring Organization:: USDOE Office of Science (SC); National Aeronautics and Space Administration (NASA); National Science Foundation (NSF); Hellman Fellows Foundation

Grant/Contract Number:: SC0008541

OSTI ID:: 1611077

Journal Information:: The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 1 Vol. 874; ISSN 1538-4357

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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A Baryonic Solution to the Missing Satellites Problem Brooks, Alyson M.; Kuhlen, Michael; Zolotov, Adi arXiv https://doi.org/10.48550/arxiv.1209.5394	text	January 2012
Constraining Self-Interacting Dark Matter with the Milky Way's dwarf spheroidals Zavala, Jesus; Vogelsberger, Mark; Walker, Matthew G. arXiv https://doi.org/10.48550/arxiv.1211.6426	text	January 2012
A new multi-field determination of the galaxy luminosity function at z=7-9 incorporating the 2012 Hubble Ultra Deep Field imaging McLure, R. J.; Dunlop, J. S.; Bowler, R. A. A. arXiv https://doi.org/10.48550/arxiv.1212.5222	text	January 2012
Halo Mass Function and the Free Streaming Scale Schneider, Aurel; Smith, Robert E.; Reed, Darren arXiv https://doi.org/10.48550/arxiv.1303.0839	text	January 2013
The properties of warm dark matter haloes Lovell, Mark R.; Frenk, Carlos S.; Eke, Vincent R. arXiv https://doi.org/10.48550/arxiv.1308.1399	text	January 2013
Tying Dark Matter to Baryons with Self-interactions Kaplinghat, Manoj; Keeley, Ryan E.; Linden, Tim arXiv https://doi.org/10.48550/arxiv.1311.6524	text	January 2013
Using the Milky Way satellites to study interactions between cold dark matter and radiation Boehm, C.; Schewtschenko, J. A.; Wilkinson, R. J. arXiv https://doi.org/10.48550/arxiv.1404.7012	text	January 2014
Scattering, Damping, and Acoustic Oscillations: Simulating the Structure of Dark Matter Halos with Relativistic Force Carriers Buckley, Matthew R.; Zavala, Jesús; Cyr-Racine, Francis-Yan arXiv https://doi.org/10.48550/arxiv.1405.2075	text	January 2014
Cosmic Discordance: Are Planck CMB and CFHTLenS weak lensing measurements out of tune? MacCrann, Niall; Zuntz, Joe; Bridle, Sarah arXiv https://doi.org/10.48550/arxiv.1408.4742	preprint	January 2014
Structure formation with suppressed small-scale perturbations Schneider, Aurel arXiv https://doi.org/10.48550/arxiv.1412.2133	preprint	January 2014
Planck 2015 results. XIII. Cosmological parameters Collaboration, Planck; Ade, P. A. R.; Aghanim, N. arXiv https://doi.org/10.48550/arxiv.1502.01589	text	January 2015
The unexpected diversity of dwarf galaxy rotation curves Oman, Kyle A.; Navarro, Julio F.; Fattahi, Azadeh arXiv https://doi.org/10.48550/arxiv.1504.01437	text	January 2015
The universality of the virial halo mass function and models for non-universality of other halo definitions Despali, Giulia; Giocoli, Carlo; Angulo, Raul E. arXiv https://doi.org/10.48550/arxiv.1507.05627	text	January 2015
The Evolution of the Galaxy Stellar Mass Function at z= 4-8: A Steepening Low-mass-end Slope with Increasing Redshift Song, Mimi; Finkelstein, Steven L.; Ashby, Matthew L. N. arXiv https://doi.org/10.48550/arxiv.1507.05636	text	January 2015
ETHOS - An Effective Theory of Structure Formation: From dark particle physics to the matter distribution of the Universe Cyr-Racine, Francis-Yan; Sigurdson, Kris; Zavala, Jesus arXiv https://doi.org/10.48550/arxiv.1512.05344	text	January 2015
CFHTLenS revisited: assessing concordance with Planck including astrophysical systematics Joudaki, Shahab; Blake, Chris; Heymans, Catherine arXiv https://doi.org/10.48550/arxiv.1601.05786	text	January 2016
A 2.4% Determination of the Local Value of the Hubble Constant Riess, Adam G.; Macri, Lucas M.; Hoffmann, Samantha L. arXiv https://doi.org/10.48550/arxiv.1604.01424	text	January 2016
A Testable Conspiracy: Simulating Baryonic Effects on Self-Interacting Dark Matter Halos Elbert, Oliver D.; Bullock, James S.; Kaplinghat, Manoj arXiv https://doi.org/10.48550/arxiv.1609.08626	text	January 2016
Cosmological Constraints on Interacting Light Particles Brust, Christopher; Cui, Yanou; Sigurdson, Kris arXiv https://doi.org/10.48550/arxiv.1703.10732	text	January 2017
"Non-cold" dark matter at small scales: a general approach Murgia, Riccardo; Merle, Alexander; Viel, Matteo arXiv https://doi.org/10.48550/arxiv.1704.07838	text	January 2017
NIHAO XIV: Reproducing the observed diversity of dwarf galaxy rotation curve shapes in LCDM Santos-Santos, Isabel M.; Di Cintio, Arianna; Brook, Chris B. arXiv https://doi.org/10.48550/arxiv.1706.04202	text	January 2017
Signatures of Self-Interacting Dark Matter in the Matter Power Spectrum and the CMB Huo, Ran; Kaplinghat, Manoj; Pan, Zhen arXiv https://doi.org/10.48550/arxiv.1709.09717	text	January 2017
The diverse density profiles of galaxy clusters with self-interacting dark matter plus baryons Robertson, Andrew; Massey, Richard; Eke, Vincent arXiv https://doi.org/10.48550/arxiv.1711.09096	text	January 2017
Gravitational Lensing and the Power Spectrum of Dark Matter Substructure: Insights from the ETHOS N-body Simulations Rivero, Ana Díaz; Dvorkin, Cora; Cyr-Racine, Francis-Yan arXiv https://doi.org/10.48550/arxiv.1809.00004	text	January 2018
Cosmological parameters from CMB and other data: a Monte-Carlo approach Lewis, Antony; Bridle, Sarah arXiv https://doi.org/10.48550/arxiv.astro-ph/0205436	text	January 2002
The Non-Parametric Model for Linking Galaxy Luminosity with Halo/Subhalo Mass Vale, A.; Ostriker, J. P. arXiv https://doi.org/10.48550/arxiv.astro-ph/0511816	text	January 2005
Observational and Theoretical Constraints on Singular Dark Matter Halos Flores, Ricardo A.; Primack, Joel R. arXiv https://doi.org/10.48550/arxiv.astro-ph/9402004	text	January 1994
Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons Bryan, G. L.; Norman, M. L. arXiv https://doi.org/10.48550/arxiv.astro-ph/9710107	text	January 1997
Where are the missing galactic satellites? Klypin, Anatoly A.; Kravtsov, Andrey V.; Valenzuela, Octavio arXiv https://doi.org/10.48550/arxiv.astro-ph/9901240	text	January 1999
Structure formation with suppressed small-scale perturbations Schneider, Aurel Oxford University Press https://doi.org/10.5167/uzh-122014	text	January 2015
Cosmic Dawn (CoDa): the first radiation-hydrodynamics simulation of reionization and galaxy formation in the Local Universe Ocvirk, Pierre; Gillet, Nicolas; Shapiro, Paul R. Oxford University Press https://doi.org/10.5167/uzh-129969	text	January 2016
Hints against the cold and collisionless nature of dark matter from the galaxy velocity function Aurel, Schneider,; Sebastian, Trujillo-Gomez,; Emmanouil, Papastergis, Oxford University Press https://doi.org/10.5167/uzh-142895	text	January 2017

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Dark matter haloes and subhaloes Zavala, Jesús; Frenk, Carlos S. arXiv https://doi.org/10.48550/arxiv.1907.11775	preprint	January 2019
Double dark matter vision: twice the number of compact-source lenses with narrow-line lensing and the WFC3 grism Nierenberg, A. M.; Gilman, D.; Treu, T. Monthly Notices of the Royal Astronomical Society, Vol. 492, Issue 4 https://doi.org/10.1093/mnras/stz3588	journal	December 2019
The halo mass function in alternative dark matter models Lovell, M. R. Monthly Notices of the Royal Astronomical Society: Letters, Vol. 493, Issue 1 https://doi.org/10.1093/mnrasl/slaa005	journal	January 2020
Dark Matter Haloes and Subhaloes Zavala, Jesús; Frenk, Carlos S. Galaxies, Vol. 7, Issue 4 https://doi.org/10.3390/galaxies7040081	journal	September 2019

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