activity
20102024
most citedThe properties of warm dark matter haloes

483 citations · 3.1k across the 49 of their papers we have counts for

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Showing 2022Show all

7 papers · 1 filter

astro-ph.CO2022★ 34 cited

Sensitivity of strong lensing observations to dark matter substructure: a case study with Euclid

Conor M. O'Riordan, Giulia Despali, Simona Vegetti +2

We introduce a machine learning method for estimating the sensitivity of strong lens observations to dark matter subhaloes in the lens. Our training data include elliptical power-l…

astro-ph.GA2022★ 19 cited

Gravothermal collapse of Self-Interacting Dark Matter halos as the Origin of Intermediate Mass Black Holes in Milky Way satellites

Tamar Meshveliani, Jesús Zavala, Mark R. Lovell

Milky Way (MW) satellites exhibit a diverse range of internal kinematics, reflecting in turn a diverse set of subhalo density profiles. These profiles include large cores and dense…

astro-ph.CO2022★ 12 cited

Matching the mass function of Milky Way satellites in competing dark matter models

Mark R. Lovell, Jesús Zavala

Any successful model of dark matter must explain the diversity of observed Milky Way (MW) satellite density profiles, from very dense ultrafaints to large, low density satellites s…

astro-ph.IM2022★ 7 cited

Differentiating small-scale subhalo distributions in CDM and WDM models using persistent homology

Jessi Cisewski-Kehe, Brittany Terese Fasy, Wojciech Hellwing +3

The spatial distribution of galaxies at sufficiently small scales will encode information about the identity of the dark matter. We develop a novel description of the halo distribu…

astro-ph.CO2022

Could fresh lava be (warm) dark matter?

Mark R. Lovell

Dark matter models can be classified according to their impact on the properties of galaxies, including cold dark matter (CDM), warm dark matter (WDM), self-interacting dark matter…

hep-ph2022★ 20 cited

Snowmass2021 Cosmic Frontier White Paper: Dark Matter Physics from Halo Measurements

Keith Bechtol, Simon Birrer, Francis-Yan Cyr-Racine +41

The non-linear process of cosmic structure formation produces gravitationally bound overdensities of dark matter known as halos. The abundances, density profiles, ellipticities, an…

astro-ph.GA2022★ 7 cited

The feasibility of constraining DM interactions with high-redshift observations by JWST

Ali Kurmus, Sownak Bose, Mark Lovell +4

Observations of the high redshift universe provide a promising avenue for constraining the nature of the dark matter (DM). This will be even more true with the advent of the James…