Sensitivity forecasts for gravitational-wave detectors to dark matter decaying into gravitons

Read full text
Authors: José A. R. Cembranos, Álvaro Cendal
Cited by: 2
References: 66

Abstract

Abstract Dark matter may not be perfectly stable, and its decay could generate distinctive gravitational-wave signatures. In this work, we present model-independent predictions for the stochastic gravitational-wave background arising from the decay of ultralight dark matter into gravitons. Within this framework, we forecast the sensitivity reach of current and forthcoming gravitational-wave detectors to such signals.

Fields of Study & Subjects

Dark Matter and Cosmic Phenomena Pulsars and Gravitational Waves Research Atomic and Subatomic Physics Research

Publication details

Journal / source
Journal of Cosmology and Astroparticle Physics
Publisher
IOP Publishing
Volume
2026
Issue
03
Pages
055–055
Publication date
1 March 2026