collaborators

6 papers

astro-ph.CO2026

Pulsar Timing Sensitivity to Dark Matter Substructure in the Presence of a Stochastic Gravitational-Wave Background

Abhiram Cherukupalli, Vincent S. H. Lee, Kim Berghaus +1

Pulsar timing arrays (PTAs) can detect dark matter (DM) substructure through the small shifts a transiting DM subhalo imprints on pulse arrival times. Recently found evidence for a…

hep-ph2026

Classical equipartition dynamics between axions and non-Abelian gauge fields

Kim V. Berghaus, Adrien Florio, M. Laine +1

Motivated by axion-like inflation and its warm embedding within the Standard Model, we study the early stages of the energy transfer between an axion condensate and an SU(2) gauge…

hep-ph2026

The Migdal effect in Semiconductors for the Effective Field Theory of Dark Matter Direct Detection

Kim V. Berghaus, Rouven Essig, Megan H. McDuffie

The Migdal effect in semiconductors, prompt ionization from a primary nuclear scattering event, can be described across all kinematic regimes using an effective field theory that e…

hep-ph2026

Physics beyond the Standard Model with the DSA-2000

Kim V. Berghaus, Yufeng Du, Vincent S. H. Lee +4

The upcoming Deep Synoptic Array 2000 (DSA-2000) will map the radio sky at GHz (eV) with unprecedented sensitivity. This will enable searches for dark matt…

hep-ph2025

Warm Inflation with the Standard Model

Kim V. Berghaus, Marco Drewes, Sebastian Zell

We show for the first time that warm inflation is feasible with Standard Model (SM) gauge interactions alone. Our model consists of a minimal extension of the SM by a single scalar…

hep-ph2025

Searching For Superheavy Decaying Particles With Ultra-High-Energy Neutrino Observatories

Kim V. Berghaus, Dan Hooper, Emily R. Simon

If there exist unstable but long-lived relics of the early universe, their decays could produce detectable fluxes of gamma rays and neutrinos. In this paper, we point out that the…