activity
20182022
most citedETHOS - an effective theory of structure formation: formation of the first haloes and their stars

19 citations · 36 across the 5 of their papers we have counts for

collaborators

15 papers

astro-ph.CO2020

Constraints on the properties of warm dark matter using the satellite galaxies of the Milky Way

Oliver Newton, Matteo Leo, Marius Cautun +5

The satellite galaxies of the Milky Way (MW) are effective probes of the underlying dark matter (DM) substructure, which is sensitive to the nature of the DM particle. In particula…

astro-ph.CO2020

Joint constraints on thermal relic dark matter from strong gravitational lensing, the Lyman- forest, and Milky Way satellites

Wolfgang Enzi, Riccardo Murgia, Oliver Newton +10

We derive joint constraints on the warm dark matter (WDM) half-mode scale by combining the analyses of a selection of astrophysical probes: strong gravitational lensing with extend…

astro-ph.GA2020

The Onset of Gravothermal Core Collapse in Velocity Dependent Self-Interacting Dark Matter Subhaloes

Hannah C. Turner, Mark R. Lovell, Jesús Zavala +1

It has been proposed that gravothermal collapse due to dark matter self-interactions (i.e. self-interacting dark matter, SIDM) can explain the observed diversity of the Milky Way (…

astro-ph.CO20201 cited

Cosmological Dark Matter: a Review (the April Fool Edition)

M. R. Lovell

Evidence has continued to accumulate over the last few decades as to the existence and nature of dark matter. Depending on the particle candidate, the dark matter can exhibit one o…

astro-ph.CO2020

Towards a general parametrization of the warm dark matter halo mass function

Mark R. Lovell

Studies of flux anomalies statistics and perturbations in stellar streams have the potential to constrain models of warm dark matter (WDM), including sterile neutrinos. Producing t…

astro-ph.GA2020

Local Group star formation in warm and self-interacting dark matter cosmologies

Mark R. Lovell, Wojciech Hellwing, Aaron Ludlow +5

The nature of the dark matter can affect the collapse time of dark matter haloes, and can therefore be imprinted in observables such as the stellar population ages and star formati…