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Unveiling the gravitational universe at $\mu$-Hz frequencies

We propose a space-based interferometer surveying the gravitational wave (GW) sky in the milli-Hz to $\mu$-Hz frequency range. By the 2040s, the μ-Hz frequency band, bracketed in between the Laser Interferometer Space Antenna (LISA) and pulsar timing arrays, will constitute the largest gap in the co...

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Autores principales: Sesana, Alberto, Korsakova, Natalia, Sedda, Manuel Arca, Baibhav, Vishal, Barausse, Enrico, Barke, Simon, Berti, Emanuele, Bonetti, Matteo, Capelo, Pedro R., Caprini, Chiara, Garcia-Bellido, Juan, Haiman, Zoltan, Jani, Karan, Jennrich, Oliver, Johansson, Peter H., Khan, Fazeel Mahmood, Korol, Valeriya, Lamberts, Astrid, Lupi, Alessandro, Mangiagli, Alberto, Mayer, Lucio, Nardini, Germano, Pacucci, Fabio, Petiteau, Antoine, Raccanelli, Alvise, Rajendran, Surjeet, Regan, John, Shao, Lijing, Spallicci, Alessandro, Tamanini, Nicola, Volonteri, Marta, Warburton, Niels, Wong, Kaze, Zumalacarregui, Miguel
Lenguaje:eng
Publicado: 2019
Materias:
Acceso en línea:https://dx.doi.org/10.1007/s10686-021-09709-9
http://cds.cern.ch/record/2790828
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author Sesana, Alberto
Korsakova, Natalia
Sedda, Manuel Arca
Baibhav, Vishal
Barausse, Enrico
Barke, Simon
Berti, Emanuele
Bonetti, Matteo
Capelo, Pedro R.
Caprini, Chiara
Garcia-Bellido, Juan
Haiman, Zoltan
Jani, Karan
Jennrich, Oliver
Johansson, Peter H.
Khan, Fazeel Mahmood
Korol, Valeriya
Lamberts, Astrid
Lupi, Alessandro
Mangiagli, Alberto
Mayer, Lucio
Nardini, Germano
Pacucci, Fabio
Petiteau, Antoine
Raccanelli, Alvise
Rajendran, Surjeet
Regan, John
Shao, Lijing
Spallicci, Alessandro
Tamanini, Nicola
Volonteri, Marta
Warburton, Niels
Wong, Kaze
Zumalacarregui, Miguel
author_facet Sesana, Alberto
Korsakova, Natalia
Sedda, Manuel Arca
Baibhav, Vishal
Barausse, Enrico
Barke, Simon
Berti, Emanuele
Bonetti, Matteo
Capelo, Pedro R.
Caprini, Chiara
Garcia-Bellido, Juan
Haiman, Zoltan
Jani, Karan
Jennrich, Oliver
Johansson, Peter H.
Khan, Fazeel Mahmood
Korol, Valeriya
Lamberts, Astrid
Lupi, Alessandro
Mangiagli, Alberto
Mayer, Lucio
Nardini, Germano
Pacucci, Fabio
Petiteau, Antoine
Raccanelli, Alvise
Rajendran, Surjeet
Regan, John
Shao, Lijing
Spallicci, Alessandro
Tamanini, Nicola
Volonteri, Marta
Warburton, Niels
Wong, Kaze
Zumalacarregui, Miguel
author_sort Sesana, Alberto
collection CERN
description We propose a space-based interferometer surveying the gravitational wave (GW) sky in the milli-Hz to $\mu$-Hz frequency range. By the 2040s, the μ-Hz frequency band, bracketed in between the Laser Interferometer Space Antenna (LISA) and pulsar timing arrays, will constitute the largest gap in the coverage of the astrophysically relevant GW spectrum. Yet many outstanding questions related to astrophysics and cosmology are best answered by GW observations in this band. We show that a μ-Hz GW detector will be a truly overarching observatory for the scientific community at large, greatly extending the potential of LISA. Conceived to detect massive black hole binaries from their early inspiral with high signal-to-noise ratio, and low-frequency stellar binaries in the Galaxy, this instrument will be a cornerstone for multimessenger astronomy from the solar neighbourhood to the high-redshift Universe.
id cern-2790828
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2019
record_format invenio
spelling cern-27908282022-08-20T06:00:30Zdoi:10.1007/s10686-021-09709-9http://cds.cern.ch/record/2790828engSesana, AlbertoKorsakova, NataliaSedda, Manuel ArcaBaibhav, VishalBarausse, EnricoBarke, SimonBerti, EmanueleBonetti, MatteoCapelo, Pedro R.Caprini, ChiaraGarcia-Bellido, JuanHaiman, ZoltanJani, KaranJennrich, OliverJohansson, Peter H.Khan, Fazeel MahmoodKorol, ValeriyaLamberts, AstridLupi, AlessandroMangiagli, AlbertoMayer, LucioNardini, GermanoPacucci, FabioPetiteau, AntoineRaccanelli, AlviseRajendran, SurjeetRegan, JohnShao, LijingSpallicci, AlessandroTamanini, NicolaVolonteri, MartaWarburton, NielsWong, KazeZumalacarregui, MiguelUnveiling the gravitational universe at $\mu$-Hz frequenciesgr-qcGeneral Relativity and Cosmologyastro-ph.HEAstrophysics and Astronomyastro-ph.IMAstrophysics and AstronomyWe propose a space-based interferometer surveying the gravitational wave (GW) sky in the milli-Hz to $\mu$-Hz frequency range. By the 2040s, the μ-Hz frequency band, bracketed in between the Laser Interferometer Space Antenna (LISA) and pulsar timing arrays, will constitute the largest gap in the coverage of the astrophysically relevant GW spectrum. Yet many outstanding questions related to astrophysics and cosmology are best answered by GW observations in this band. We show that a μ-Hz GW detector will be a truly overarching observatory for the scientific community at large, greatly extending the potential of LISA. Conceived to detect massive black hole binaries from their early inspiral with high signal-to-noise ratio, and low-frequency stellar binaries in the Galaxy, this instrument will be a cornerstone for multimessenger astronomy from the solar neighbourhood to the high-redshift Universe.We propose a space-based interferometer surveying the gravitational wave (GW) sky in the milli-Hz to $\mu$-Hz frequency range. By the 2040s', the $\mu$-Hz frequency band, bracketed in between the Laser Interferometer Space Antenna (LISA) and pulsar timing arrays, will constitute the largest gap in the coverage of the astrophysically relevant GW spectrum. Yet many outstanding questions related to astrophysics and cosmology are best answered by GW observations in this band. We show that a $\mu$-Hz GW detector will be a truly overarching observatory for the scientific community at large, greatly extending the potential of LISA. Conceived to detect massive black hole binaries from their early inspiral with high signal-to-noise ratio, and low-frequency stellar binaries in the Galaxy, this instrument will be a cornerstone for multimessenger astronomy from the solar neighbourhood to the high-redshift Universe.arXiv:1908.11391oai:cds.cern.ch:27908282019-08-29
spellingShingle gr-qc
General Relativity and Cosmology
astro-ph.HE
Astrophysics and Astronomy
astro-ph.IM
Astrophysics and Astronomy
Sesana, Alberto
Korsakova, Natalia
Sedda, Manuel Arca
Baibhav, Vishal
Barausse, Enrico
Barke, Simon
Berti, Emanuele
Bonetti, Matteo
Capelo, Pedro R.
Caprini, Chiara
Garcia-Bellido, Juan
Haiman, Zoltan
Jani, Karan
Jennrich, Oliver
Johansson, Peter H.
Khan, Fazeel Mahmood
Korol, Valeriya
Lamberts, Astrid
Lupi, Alessandro
Mangiagli, Alberto
Mayer, Lucio
Nardini, Germano
Pacucci, Fabio
Petiteau, Antoine
Raccanelli, Alvise
Rajendran, Surjeet
Regan, John
Shao, Lijing
Spallicci, Alessandro
Tamanini, Nicola
Volonteri, Marta
Warburton, Niels
Wong, Kaze
Zumalacarregui, Miguel
Unveiling the gravitational universe at $\mu$-Hz frequencies
title Unveiling the gravitational universe at $\mu$-Hz frequencies
title_full Unveiling the gravitational universe at $\mu$-Hz frequencies
title_fullStr Unveiling the gravitational universe at $\mu$-Hz frequencies
title_full_unstemmed Unveiling the gravitational universe at $\mu$-Hz frequencies
title_short Unveiling the gravitational universe at $\mu$-Hz frequencies
title_sort unveiling the gravitational universe at $\mu$-hz frequencies
topic gr-qc
General Relativity and Cosmology
astro-ph.HE
Astrophysics and Astronomy
astro-ph.IM
Astrophysics and Astronomy
url https://dx.doi.org/10.1007/s10686-021-09709-9
http://cds.cern.ch/record/2790828
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