The Lunar Gravitational-wave Antenna: mission studies and science case

Parameswaran Ajith et al.

Detalles Bibliográficos
Autores: Ajith, Parameswaran, Giustini, Margherita, Kavanagh, Bradley J., Miniutti, Giovanni
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2025
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/392124
Acceso en línea:http://hdl.handle.net/10261/392124
Access Level:acceso abierto
Palabra clave:Gravitational wave detectors
Gravitational waves / sources
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dc.title.none.fl_str_mv The Lunar Gravitational-wave Antenna: mission studies and science case
title The Lunar Gravitational-wave Antenna: mission studies and science case
spellingShingle The Lunar Gravitational-wave Antenna: mission studies and science case
Ajith, Parameswaran
Gravitational wave detectors
Gravitational waves / sources
title_short The Lunar Gravitational-wave Antenna: mission studies and science case
title_full The Lunar Gravitational-wave Antenna: mission studies and science case
title_fullStr The Lunar Gravitational-wave Antenna: mission studies and science case
title_full_unstemmed The Lunar Gravitational-wave Antenna: mission studies and science case
title_sort The Lunar Gravitational-wave Antenna: mission studies and science case
dc.creator.none.fl_str_mv Ajith, Parameswaran
Giustini, Margherita
Kavanagh, Bradley J.
Miniutti, Giovanni
author Ajith, Parameswaran
author_facet Ajith, Parameswaran
Giustini, Margherita
Kavanagh, Bradley J.
Miniutti, Giovanni
author_role author
author2 Giustini, Margherita
Kavanagh, Bradley J.
Miniutti, Giovanni
author2_role author
author
author
dc.contributor.none.fl_str_mv European Commission
European Research Council
Agencia Estatal de Investigación (España)
Ministerio de Ciencia, Innovación y Universidades (España)
Comunidad de Madrid
NASA
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Gravitational wave detectors
Gravitational waves / sources
topic Gravitational wave detectors
Gravitational waves / sources
description Parameswaran Ajith et al.
publishDate 2025
dc.date.none.fl_str_mv 2025
2025
2025
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dc.publisher.none.fl_str_mv IOP Publishing
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spelling The Lunar Gravitational-wave Antenna: mission studies and science caseAjith, ParameswaranGiustini, MargheritaKavanagh, Bradley J.Miniutti, GiovanniGravitational wave detectorsGravitational waves / sourcesParameswaran Ajith et al.ArXiv ePrint: 2404.09181The Lunar Gravitational-wave Antenna (LGWA) is a proposed array of next-generation inertial sensors to monitor the response of the Moon to gravitational waves (GWs). Given the size of the Moon and the expected noise produced by the lunar seismic background, the LGWA would be able to observe GWs from about 1 mHz to 1 Hz. This would make the LGWA the missing link between space-borne detectors like LISA with peak sensitivities around a few millihertz and proposed future terrestrial detectors like Einstein Telescope or Cosmic Explorer. In this article, we provide a first comprehensive analysis of the LGWA science case including its multi-messenger aspects and lunar science with LGWA data. We also describe the scientific analyses of the Moon required to plan the LGWA mission.This article has benefited from the program Lunar Gravitational-Wave Detection (ICTS / LGWD2023/04) organised by the International Centre for Theoretical Sciences (ICTS), Bengaluru, India. AS acknowledges the financial support provided under the European Union’s H2020 ERC Consolidator Grant “Binary Massive Black Hole Astrophysics” (B Massive, Grant Agreement: 818691). GM is supported by grant No. PID2020-115325GB-C31 funded by MCIN/AEI/10.13039/50110001103. MManc is supported by ERC Starting Grant No. 945155GWmining, Cariplo Foundation Grant No. 2021-0555, MUR PRIN Grant No. 2022-Z9X4XS, and the ICSC National Research Centre funded by NextGenerationEU. The work of MManc received support from the French government under the France 2030 investment plan, as part of the Initiative d’Excellence d’Aix-Marseille Université — A*MIDEX AMX-22-CEI-02. TP’s work is supported by an advanced ERC grant MultiJets. The work of MMagg is supported by the Swiss National Science Foundation (SNSF) grants 200020_191957 and CRSII5_213497; SF, FI and NM are supported by the SNSF grant 200020_191957; EB is supported by the SNSF grant CRSII5_213497. ARP is supported by the Swiss National Science Foundation (SNSF Ambizione grant no. 182044). RA was supported by NASA through the NASA Hubble Fellowship grant #HST-HF2-51499.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555. MWC acknowledges support from the National Science Foundation (NSF) with grant numbers PHY-2010970 and PHY2117997. AM acknowledges financial support from MUR PRIN Grant No. 2022-Z9X4XS, funded by the European Union — Next Generation EU. CC acknowledges the support of P Sreekumar and the LGWA discussion meeting hosted by the International Centre for Theoretical Sciences (ICTS), Tata Institute of Fundamental Research, India, in April 2023. MAS acknowledges funding from the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No. 101025436 (project GRACE-BH, PI: Manuel Arca Sedda). MAS acknowledge financial support from the MERAC Foundation. OG is funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany’s Excellence Strategy — EXC 2121 “Quantum Universe” — 390833306. SCS is funded by the Deutsches Zentrum für Luft- und Raumfahrt (DLR) with funding from the Bundesministerium für Wirtschaft und Klimaschutz under project reference 50OQ2302. RS acknowledges support from the agreement ASI-INAF eXTP Fase B — 2020-3-HH.1-2021 and the INAF-PRIN grant “A systematic Study of the largest reservoir of baryons and metals in the Universe: the circumgalactic medium of galaxies” (No. 1.05.01.85.10). FO acknowledges support from MIUR, PRIN 2020 (grant 2020KB33TP) “Multimessenger astronomy in the Einstein Telescope Era (METE)”. PS, RDC, RS, CV, ADR, VB acknowledge a financial contribution from the Bando Ricerca Fondamentale INAF 2022 Large Grant, ‘Dual and binary supermassive black holes in the multi-messenger era: from galaxy mergers to gravitational waves’. MG is supported by the “Programa de Atracción de Talento” of the Comunidad de Madrid, grant number 2022-5A/TIC-24235. The work of SM is a part of the ⟨data|theory⟩ Universe-Lab which is supported by the TIFR and the Department of Atomic Energy, Government of India. MZ is funded by the Fonds National de la Recherche Scientifique (FNRS) under projet de recherche STELLAR (T.0022.22). AB acknowledges support for this project from the European Union’s Horizon 2020 research and innovation program under grant agreement No 865932-ERC-SNeX. PA, NVK, PK, RP and VP were supported by the Department of Atomic Energy, Government of India, under Project No. RTI4001. AMB acknowledges funding from the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No 895174. DV acknowledges support from the NASA Hubble Fellowship Program grant HST-HF2-51520. M.T. acknowledges support from MUR through the FARE 2020 scheme, project ‘B Massive-LISA’, code: R203NMYZJ5.Peer reviewedIOP PublishingEuropean CommissionEuropean Research CouncilAgencia Estatal de Investigación (España)Ministerio de Ciencia, Innovación y Universidades (España)Comunidad de MadridNASAConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202520252025info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://hdl.handle.net/10261/392124reponame:DIGITAL.CSIC. 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