2026-06-28T20:28:44Zhttps://docta.ucm.es/rest/oai/request

oai:docta.ucm.es:20.500.14352/1350732026-04-24T23:49:06Zcom_20.500.14352_14col_20.500.14352_15

Sensitivity forecasts for gravitational-wave detectors to dark matter decaying into gravitons Ruiz Cembranos, José Alberto Cendal García, Álvaro © 2026 IOP Publishing Ltd and Sissa Medialab. CA21106, CA21136, CA22113, CA23130. FPU22/03222. 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. 2026-04-24T16:15:49Z 2026-04-24T16:15:49Z 2026-03-19 journal article Jose A.R. Cembranos and Álvaro Cendal JCAP03(2026)055 10.1088/1475-7516/2026/03/055 https://hdl.handle.net/20.500.14352/135073 1475-7516 https//doi.org/10.1088/1475-7516/2026/03/055 https://iopscience.iop.org/article/10.1088/1475-7516/2026/03/055 https://arxiv.org/abs/2510.18958 eng info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2022-139841NB-I00/CONSTRUYENDO EL UNIVERSO: DE LA INFLACION COSMOLOGICA A LA MATERIA OSCURA/ES embargoed access IOP Publishing