RT Journal Article
T1 Sensitivity forecasts for gravitational-wave detectors to dark matter decaying into gravitons
A1 García Cendal, Álvaro
A1 Ruiz Cembranos, José Alberto
AB 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.
PB IOP Publishing Ltd and Sissa Medialab
YR 2026
FD 2026-03-19
LK https://hdl.handle.net/20.500.14352/136778
UL https://hdl.handle.net/20.500.14352/136778
LA eng
NO Jose A.R. Cembranos and Álvaro Cendal JCAP03(2026)055
NO © 2026 IOP Publishing Ltd and Sissa Medialab.CA21106, CA21136, CA22113, CA23130.FPU22/03222
NO European Commission
NO Ministerio de Ciencia, Innovación y Universidades (España)
NO Agencia Estatal de Investigación (España)
DS Docta Complutense
RD 10 jun 2026