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The effect of mission duration on LISA science objectives

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The effect of mission duration on LISA science objectives

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dc.contributor.author Amaro-Seoane, Pau es_ES
dc.contributor.author Arca Sedda, Manuel es_ES
dc.contributor.author Babak, Stanislav es_ES
dc.contributor.author Berry, Christopher P. L. es_ES
dc.contributor.author Berti, Emanuele es_ES
dc.contributor.author Bertone, Gianfranco es_ES
dc.contributor.author Blas, Diego es_ES
dc.contributor.author Bogdanovic, Tamara es_ES
dc.contributor.author Bonetti, Matteo es_ES
dc.contributor.author Breivik, Katelyn es_ES
dc.contributor.author Brito, Richard es_ES
dc.contributor.author Caldwell, Robert es_ES
dc.contributor.author Capelo, Pedro R. es_ES
dc.contributor.author Caprini, Chiara es_ES
dc.contributor.author Cardoso, Vitor es_ES
dc.date.accessioned 2023-09-21T18:06:38Z
dc.date.available 2023-09-21T18:06:38Z
dc.date.issued 2022-01 es_ES
dc.identifier.issn 0001-7701 es_ES
dc.identifier.uri http://hdl.handle.net/10251/196939
dc.description.abstract [EN] The science objectives of the LISA mission have been defined under the implicit assumption of a 4-years continuous data stream. Based on the performance of LISA Pathfinder, it is now expected that LISA will have a duty cycle of ¿0.75, which would reduce the effective span of usable data to 3 years. This paper reports the results of a study by the LISA Science Group, which was charged with assessing the additional science return of increasing the mission lifetime. We explore various observational scenarios to assess the impact of mission duration on the main science objectives of the mission. We find that the science investigations most affected by mission duration concern the search for seed black holes at cosmic dawn, as well as the study of stellar-origin black holes and of their formation channels via multi-band and multi-messenger observations. We conclude that an extension to 6 years of mission operations is recommended. es_ES
dc.description.sponsorship We thank Danny Laghi and Walter Del Pozzo for help with Fig. 8. C.P.L. Berry is supported by the CIERA Board of Visitors Professorship. E. Berti is supported by NSF Grants No. PHY1912550 and AST-2006538, NASA ATP Grants No. 17-ATP17-0225 and 19-ATP19-0051, NSF-XSEDE Grant No. PHY-090003, and NSF Grant PHY-20043. D. Blas acknowledges support from the Fundacion Jesus Serra and the Instituto de Astrofisica de Canarias under the Visiting Researcher Programme 2021 agreed between both institutions. T. Bogdanovi ' c acknowledges the support by the National Aeronautics and Space Administration (NASA) under award No. 80NSSC19K0319 and by the National Science Foundation (NSF) under Award No. 1908042. V. Cardoso acknowledges financial support provided under the European Union's H2020 ERC Consolidator Grant "Matter and strong-field gravity: New frontiers in Einstein's theory" Grant Agreement No. MaGRaTh-646597. This project has received funding from the European Union's Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant agreement No 101007855. We thank FCT for financial support through Projects No. UIDB/00099/2020 and through grants PTDC/MAT-APL/30043/2017 and PTDC/FIS-AST/7002/2020. H.-Y. Chen is supported by NASA through NASA Hubble Fellowship Grants No. HST-HF2-51452.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. Z. Haiman acknowledges support by NASA Grant NNX15AB19G and NSF Grants AST-2006176 and AST-1715661. G. Nardini is partly supported by the ROMFORSK Grant Project. No. 302640 "Gravitational Wave Signals From Early Universe Phase Transitions". P. Pani acknowledges financial support provided under the European Union's H2020 ERC, Starting Grant Agreement No. DarkGRA-757480. He also acknowledges support under the MIUR PRIN and FARE programmes (GW-NEXT, CUP: B84I20000100001), and by the Amaldi Research Center funded by the MIUR program "Dipartimento di Eccellenza" (CUP: B81I18001170001). A. Sesana acknowledges financial support provided under the European Union's H2020 ERC Consolidator Grant "Binary Massive Black Hole Astrophysics" (BMassive, Grant Agreement: 818691). K. Yagi acknowledges support from NSF Grant PHY-1806776, NASA Grant 80NSSC20K0523, a Sloan Foundation Research Fellowship and the Owens Family Foundation. D. J. Weirwas supported by a Science and Technology Facilities Council Ernest Rutherford Fellowship, Grant no. ST/R003904/1, and by the Academy of Finland, Grants 324882 and 328958. A. Zimmerman is supported by NSF Grant No. PHY-1912578. The authors would like to acknowledge networking support by the GWverse COST Action CA16104, "Black holes, gravitational waves and fundamental physics." The Flatiron Institute is supported by the Simons Foundation. This research has made use of data, software and web tools obtained from the Gravitational Wave Open Science Center (www.gw-openscience.org/), a service of LIGO Laboratory, the LIGO Scientific Collaboration and the Virgo Collaboration. LIGO Laboratory and Advanced LIGO are funded by the United States National Science Foundation (NSF) as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, theMax-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. Virgo is funded, through the European Gravitational Observatory (EGO), by the French Centre National de Recherche Scientifique (CNRS), the Italian Istituto Nazionale di Fisica Nucleare (INFN) and the Dutch Nikhef, with contributions by institutions from Belgium, Germany, Greece, Hungary, Ireland, Japan, Monaco, Poland, Portugal, Spain. es_ES
dc.language Inglés es_ES
dc.publisher Springer-Verlag es_ES
dc.relation.ispartof General Relativity and Gravitation es_ES
dc.rights Reconocimiento (by) es_ES
dc.subject General relativity es_ES
dc.subject Gravitational waves es_ES
dc.subject Black holes es_ES
dc.subject.classification MATEMATICA APLICADA es_ES
dc.title The effect of mission duration on LISA science objectives es_ES
dc.type Artículo es_ES
dc.identifier.doi 10.1007/s10714-021-02889-x es_ES
dc.relation.projectID info:eu-repo/grantAgreement/EC/FP7/302640/EU es_ES
dc.relation.projectID info:eu-repo/grantAgreement/NSF//1908042/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/EC/H2020/101007855/EU es_ES
dc.relation.projectID info:eu-repo/grantAgreement/STFC//ST%2FR003904%2F1/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/EC/H2020/646597/EU es_ES
dc.relation.projectID info:eu-repo/grantAgreement/AKA//324882/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/EC/H2020/757480/EU es_ES
dc.relation.projectID info:eu-repo/grantAgreement/AKA//328958/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/EC/H2020/818691/EU es_ES
dc.relation.projectID info:eu-repo/grantAgreement/MIUR//CUP: B84I20000100001/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/FCT/3599-PPCDT/PTDC%2FFIS-AST%2F7002%2F2020/PT es_ES
dc.relation.projectID info:eu-repo/grantAgreement/MIUR//CUP: B81I18001170001/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/FCT/3599-PPCDT/PTDC%2FMAT-APL%2F30043%2F2017/PT es_ES
dc.relation.projectID info:eu-repo/grantAgreement/NASA//PHY-1806776//NSF/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/FCT/6817 - DCRRNI ID/UIDB%2F00099%2F2020/PT es_ES
dc.relation.projectID info:eu-repo/grantAgreement/NASA//NAS5-26555/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/NASA//80NSSC20K0523/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/NASA//PHY-1912578//NSF/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/NASA//HST-HF2-51452.001-A//NASA Hubble Fellowship/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/NASA//17-ATP17-0225//ATP/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/NASA//19-ATP19-0051//ATP/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/NASA//PHY-090003//NSF-XSEDE/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/NASA//PHY-20043//NSF/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/NASA//80NSSC19K0319/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/NASA//AST-2006176//NSF/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/NASA//AST-1715661/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/NASA//NNX15AB19G/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/COST//CA16104//COST Action/ es_ES
dc.rights.accessRights Abierto es_ES
dc.contributor.affiliation Universitat Politècnica de València. Escuela Técnica Superior de Ingeniería del Diseño - Escola Tècnica Superior d'Enginyeria del Disseny es_ES
dc.description.bibliographicCitation Amaro-Seoane, P.; Arca Sedda, M.; Babak, S.; Berry, CPL.; Berti, E.; Bertone, G.; Blas, D.... (2022). The effect of mission duration on LISA science objectives. General Relativity and Gravitation. 54(1):1-47. https://doi.org/10.1007/s10714-021-02889-x es_ES
dc.description.accrualMethod S es_ES
dc.relation.publisherversion https://doi.org/10.1007/s10714-021-02889-x es_ES
dc.description.upvformatpinicio 1 es_ES
dc.description.upvformatpfin 47 es_ES
dc.type.version info:eu-repo/semantics/publishedVersion es_ES
dc.description.volume 54 es_ES
dc.description.issue 1 es_ES
dc.identifier.pmid 35221342 es_ES
dc.identifier.pmcid PMC8827205 es_ES
dc.relation.pasarela S\487083 es_ES
dc.contributor.funder Academy of Finland es_ES
dc.contributor.funder European Commission es_ES
dc.contributor.funder Owens Family Foundation es_ES
dc.contributor.funder Alfred P. Sloan Foundation es_ES
dc.contributor.funder National Science Foundation, EEUU es_ES
dc.contributor.funder European Cooperation in Science and Technology es_ES
dc.contributor.funder Fundação para a Ciência e a Tecnologia, Portugal es_ES
dc.contributor.funder National Aeronautics and Space Administration, EEUU es_ES
dc.contributor.funder Science and Technology Facilities Council, Reino Unido es_ES
dc.contributor.funder Ministero dell'Istruzione, dell'Università e della Ricerca es_ES
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