Ruiz Cembranos, José AlbertoCendal García, Álvaro2026-04-242026-04-242026-03-19Jose A.R. Cembranos and Álvaro Cendal JCAP03(2026)05510.1088/1475-7516/2026/03/055https://hdl.handle.net/20.500.14352/135073© 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.engjournal article1475-7516https//doi.org/10.1088/1475-7516/2026/03/055https://iopscience.iop.org/article/10.1088/1475-7516/2026/03/055https://arxiv.org/abs/2510.18958embargoed access539.1Gravitational wavesSourcesDark matter detectorsPartículas2212 Física Teórica2212.02 Partículas Elementales