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

Simple item page
dc.contributor.authorRuiz Cembranos, José Alberto
dc.contributor.authorCendal García, Álvaro
dc.date.accessioned2026-04-24T16:15:49Z
dc.date.available2026-04-24T16:15:49Z
dc.date.issued2026-03-19
dc.description© 2026 IOP Publishing Ltd and Sissa Medialab. CA21106, CA21136, CA22113, CA23130. FPU22/03222.
dc.description.abstractDark 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.
dc.description.departmentDepto. de Física Teórica
dc.description.facultyFac. de Ciencias Físicas
dc.description.facultyInstituto de Física de Partículas y del Cosmos (IPARCOS)
dc.description.refereedTRUE
dc.description.sponsorshipMinisterio de Ciencia, Innovación y Universidades (España)
dc.description.sponsorshipAgencia Estatal de Investigación (España)
dc.description.sponsorshipEuropean Commission
dc.description.statuspub
dc.identifier.citationJose A.R. Cembranos and Álvaro Cendal JCAP03(2026)055
dc.identifier.doi10.1088/1475-7516/2026/03/055
dc.identifier.essn1475-7516
dc.identifier.officialurlhttps//doi.org/10.1088/1475-7516/2026/03/055
dc.identifier.relatedurlhttps://iopscience.iop.org/article/10.1088/1475-7516/2026/03/055
dc.identifier.relatedurlhttps://arxiv.org/abs/2510.18958
dc.identifier.urihttps://hdl.handle.net/20.500.14352/135073
dc.issue.number3
dc.journal.titleJournal of Cosmology and Astroparticle Physics
dc.language.isoeng
dc.page.final055-16
dc.page.initial055-1
dc.publisherIOP Publishing
dc.relation.projectIDinfo: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
dc.rights.accessRightsembargoed access
dc.subject.cdu539.1
dc.subject.keywordGravitational waves
dc.subject.keywordSources
dc.subject.keywordDark matter detectors
dc.subject.ucmPartículas
dc.subject.unesco2212 Física Teórica
dc.subject.unesco2212.02 Partículas Elementales
dc.titleSensitivity forecasts for gravitational-wave detectors to dark matter decaying into gravitons
dc.typejournal article
dc.type.hasVersionAM
dc.volume.number2026
dspace.entity.typePublication
relation.isAuthorOfPublicationc5a4cc87-ceba-494d-95ab-d54b9b1a35e3
relation.isAuthorOfPublication.latestForDiscoveryc5a4cc87-ceba-494d-95ab-d54b9b1a35e3

Download

Original bundle

Now showing 1 - 1 of 1
Thumbnail Image
Name:
2510.18958v3.pdf
Size:
1.26 MB
Format:
Adobe Portable Document Format
(Restricted until: 2027-03-19) Download

Collections

Artículos