activity
20242026
collaborators

18 papers

astro-ph.CO2026

Sensitivity of Next-Generation CMB Surveys to Neutrinos and Other Light Relics

Cynthia Trendafilova, Srinivasan Raghunathan, Benjamin Wallisch +33

Neutrinos and other light relics leave characteristic imprints in the cosmic microwave background anisotropies, making their observation a sensitive probe of the particle content a…

astro-ph.CO2026

Correlated signals of ultralight scalar dark matter in pulsar timing

Joshua W. Foster, Kimberly K. Boddy, Jeff A. Dror +5

Pulsar timing arrays (PTAs) are sensitive to ultralight dark matter (ULDM) in the - mass range, with existing datasets already probing otherwise op…

astro-ph.CO2026

CMB Limits on the Absorption of Light Vector and Axial-Vector Dark Matter

Gabriele Montefalcone, Nicola Bellomo, Kimberly K. Boddy

Leptophilic sub-MeV spin-1 dark matter (DM) can be converted into a photon via inelastic scattering with a free electron or absorption by a neutral hydrogen atom in the primordial…

astro-ph.CO2026

CMB constraints on dark matter-proton scattering: investigating prior-volume effects using profile likelihoods

Maria C. Straight, Tanvi Karwal, José Luis Bernal +1

We present profile-likelihood constraints on velocity-independent dark matter-proton scattering, including cases in which only a fraction of dark matter has such non-gravitational…

astro-ph.GA2026

Survival of the most compact: the life and death of satellite halos in self-interacting dark matter

David Klemmer, Moritz S. Fischer, Kimberly K. Boddy +2

Self-interacting dark matter (SIDM) models feature short-range interactions between dark matter (DM) particles that lead to larger diversity in the inner parts of galactic rotation…

astro-ph.CO2026

First galaxy ultraviolet luminosity function limits on dark matter-proton scattering

Hovav Lazare, Ely D. Kovetz, Kimberly K. Boddy +1

Scattering between dark matter (DM) and protons leads to suppressed small-scale fluctuations, with implications for a variety of cosmological observables. In this work, we search f…