activity
20242026
collaborators

12 papers

hep-ph2026

Combined constraints on dark photons from high-energy collisions, cosmology, and astrophysics

A. W. Romero Jorge, L. Sagunski, Guan-Wen Yuan +2

We investigate a dark sector coupled to the Standard Model (SM) through a kinetically mixed dark photon associated with a new gauge symmetry. Kinetic mixing $\varepsilo…

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

Illuminating the dark universe in the multi-messenger era

Philippe Brax, Anne-Christine Davis, Md Riajul Haque +8

The precision era of multi-messenger astronomy, together with modern astrophysical, cosmological, and gravitational wave observations, increasingly points toward the existence of a…

gr-qc2026

Fundamental oscillations as a tool to distinguish boson stars from neutron stars and black holes

Swarnim Shirke, Bikram Keshari Pradhan, Debarati Chatterjee +2

Massive boson stars are self-gravitating configurations of self-interacting scalar fields and can be modeled by a massive scalar field with a quartic self-interaction potential. It…

astro-ph.HE2026

Inference on inner galaxy structure via gravitational waves from supermassive binaries

Yifan Chen, Matthias Daniel, Daniel J. D'Orazio +107

The detection of a stochastic gravitational wave background by pulsar-timing arrays indicates the presence of a population of supermassive black hole binaries. Although the observe…

astro-ph.HE2025

Forecasted Detection Limits on the (Dark) Matter Density in Supermassive Black Hole Binaries for LISA

Matthias Daniel, Kris Pardo, Laura Sagunski

Supermassive black hole binaries (SMBHBs) are among the most powerful known sources of gravitational waves (GWs). Accordingly, these systems could dominate GW emission in the micro…