collaborators

11 papers

hep-ph2026

Astrophysical Neutrino Sources as Colliders

Carlos A. Argüelles, P. S. Bhupal Dev, Bhaskar Dutta +6

High-energy neutrinos arise from processes at large center-of-mass energies, offering a window to test physics at comparable scales or beyond those accessible in collider experimen…

hep-ph2026

Dark matter energy exchange in stars orbiting supermassive black holes

Stephan A. Meighen-Berger, R. Andrew Gustafson, Nicole F. Bell +3

Stars on tight orbits around the supermassive black hole at the Galactic Center pass through regions where the dark matter~(DM) density may be strongly enhanced. We compute the orb…

hep-ph2026

The Cosmic Neutrino Background is within Reach of Future Neutrino Telescopes

Gonzalo Herrera, Shunsaku Horiuchi, Xiaolin Qi +1

The cosmic neutrino background (CB) can be boosted to high energies due to scatterings with energetic cosmic rays (CRs) across cosmological scales. Previous calculations focuse…

hep-ph2026

Cosmic-ray boosted inelastic dark matter from neutrino-emitting active galactic nuclei

R. Andrew Gustafson, Gonzalo Herrera, Mainak Mukhopadhyay +2

Cosmic rays may scatter off dark matter particles in active galactic nuclei, where both the densities of cosmic rays and dark matter are expected to be very large. These scattering…

hep-ph2026

The Dark Matter Diffused Supernova Neutrino Background

Garv Chauhan, R. Andrew Gustafson, Gonzalo Herrera +2

We consider neutrinos scattering off Milky Way dark matter and the impact of this scattering on supernovae neutrinos. This can take the form of attenuation on the initial flux of n…

hep-ph2025

Probing Dark Matter Interactions with Stellar Motion near Sagittarius A*

R. Andrew Gustafson, Ian M. Shoemaker, Volodymyr Takhistov

Stars orbiting Sgr A* at the Milky Way's center provide a unique laboratory to test gravity and dark matter (DM). We demonstrate that DM interactions in stellar interiors induce a…