activity
20142024
most citedHeating up Neutron Stars with Inelastic Dark Matter

118 citations · 954 across the 28 of their papers we have counts for

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24 papers · 1 filter

hep-ph2024★ 10 cited

Heavy Dark Matter in White Dwarfs: Multiple-Scattering Capture and Thermalization

Nicole F. Bell, Giorgio Busoni, Sandra Robles +1

We present an improved treatment for the scattering of heavy dark matter from the ion constituents of a white dwarf. In the heavy dark matter regime, multiple collisions are requir…

hep-ph2023★ 31 cited

Thermalization and Annihilation of Dark Matter in Neutron Stars

Nicole F. Bell, Giorgio Busoni, Sandra Robles +1

The capture of dark matter, and its subsequent annihilation, can heat old, isolated neutron stars. In order for kinetic heating to be achieved, the captured dark matter must underg…

hep-ph2022★ 6 cited

Improved Treatment of Dark Matter Capture in Compact Stars

Sandra Robles

Compact stellar objects are promising cosmic laboratories to test the nature of dark matter (DM). DM captured by the strong gravitational field of these stellar remnants transfers…

hep-ph2022★ 2 cited

Disentangling Sub-GeV Dark Matter from the Diffuse Supernova Neutrino Background using Hyper-Kamiokande

Sandra Robles

The upcoming Hyper-Kamiokande (HyperK) experiment is expected to detect the Diffuse Supernova Neutrino Background (DSNB). This requires to ponder all possible sources of background…

hep-ph2022★ 9 cited

Dark Matter Pollution in the Diffuse Supernova Neutrino Background

Nicole F. Bell, Matthew J. Dolan, Sandra Robles

The Hyper-Kamiokande (HyperK) experiment is expected to precisely measure the Diffuse Supernova Neutrino Background (DSNB). This requires that the backgrounds in the relevant energ…

hep-ph2021★ 58 cited

Improved Treatment of Dark Matter Capture in Neutron Stars III: Nucleon and Exotic Targets

Filippo Anzuini, Nicole F. Bell, Giorgio Busoni +4

We consider the capture of dark matter (DM) in neutron stars via scattering on hadronic targets, including neutrons, protons and hyperons. We extend previous analyses by including…