Journal articles
Unveiling the gravitational universe at μ-Hz frequencies
Alberto Sesana
Natalia Korsakova
1
Manuel Sedda
Vishal Baibhav
Enrico Barausse
Simon Barke
Emanuele Berti
Matteo Bonetti
Pedro Capelo
Chiara Caprini
2
Juan Garcia-Bellido
Zoltan Haiman
Karan Jani
Oliver Jennrich
Peter Johansson
Fazeel Khan
Valeriya Korol
Astrid Lamberts
1
Alessandro Lupi
Alberto Mangiagli
Lucio Mayer
Germano Nardini
Fabio Pacucci
Antoine Petiteau
2
Alvise Raccanelli
Surjeet Rajendran
John Regan
Lijing Shao
Alessandro Spallicci
3
Nicola Tamanini
4
Marta Volonteri
5
Niels Warburton
Kaze Wong
Miguel Zumalacarregui
Valeriya Korol
Author
Astrid Lamberts 1
Author IdHAL : astridlamberts ORCID : https://orcid.org/0000-0001-8740-0127
Alessandro Lupi
Author
Alberto Mangiagli
Author
Alessandro Spallicci 3
Author
Nicola Tamanini 4
Author
Marta Volonteri 5
Author
Niels Warburton
Author
Kaze Wong
Author
Miguel Zumalacarregui
Author
1
OCA - Observatoire de la Côte d'Azur (B.P. 4229 06304 Nice Cedex 4 - France)
- INSU - CNRS - Institut national des sciences de l'Univers : UMS2202 (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- CNRS - Centre National de la Recherche Scientifique : UMS2202 (France)
2
APC (UMR_7164) - AstroParticule et Cosmologie (APC - UMR 7164, Université Paris Diderot, 10 rue Alice Domon et Léonie Duquet, case postale 7020, F-75205 Paris Cedex 13 - France)
- CEA - Commissariat à l'énergie atomique et aux énergies alternatives : DRF/IRFU (Centre de Saclay Centre de Grenoble Centre de Cadarache etc - France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
- Observatoire de Paris (61 Av de l'Observatoire 75014 PARIS - France)
- PSL - Université Paris sciences et lettres (60 rue Mazarine 75006 Paris - France)
- CNRS - Centre National de la Recherche Scientifique : UMR_7164 (France)
- UP - Université de Paris : UMR_7164 (85 boulevard Saint-Germain 75006 Paris - France)
3
LPC2E - Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (3A, Avenue de la Recherche Scientifique 45071 Orléans cedex 2 - France)
- OSUC - Observatoire des Sciences de l'Univers en région Centre : UMS3116 (Campus Géosciences, 1A rue de la Férollerie, 45071 Orléans - France)
- INSU - CNRS - Institut national des sciences de l'Univers (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- Observatoire de Paris (61 Av de l'Observatoire 75014 PARIS - France)
- PSL - Université Paris sciences et lettres (60 rue Mazarine 75006 Paris - France)
- UO - Université d'Orléans (Château de la Source - Avenue du Parc Floral - BP 6749 - 45067 Orléans cedex 2 - France)
- CNRS - Centre National de la Recherche Scientifique : UMS3116 (France)
- CNES - Centre National d’Études Spatiales [Paris] : UMR 7328 (Siège social : 2 place Maurice Quentin, 75039 Paris - France)
4
L2IT - Laboratoire des deux Infinis de Toulouse (Bâtiment 3R1B4
118 route de Narbonne
31062 TOULOUSE CEDEX 9 - France)
- UT3 - Université Toulouse III - Paul Sabatier (118 route de Narbonne - 31062 Toulouse - France)
- Université Fédérale Toulouse Midi-Pyrénées (41 Allée Jules Guesde, 31000 Toulouse - France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
- CNRS - Centre National de la Recherche Scientifique : UMR5033 (France)
5
IAP - Institut d'Astrophysique de Paris (98bis, bd Arago - 75014 Paris France - France)
- INSU - CNRS - Institut national des sciences de l'Univers (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- SU - Sorbonne Université (21 rue de l’École de médecine - 75006 Paris - France)
- CNRS - Centre National de la Recherche Scientifique : UMR7095 (France)
Abstract : We propose a space-based interferometer surveying the gravitational wave (GW) sky in the milli-Hz to μ-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.
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https://hal-insu.archives-ouvertes.fr/insu-03336222
Contributor : Nathalie Pothier Connect in order to contact the contributor
Submitted on : Tuesday, September 7, 2021 - 9:41:50 AM
Last modification on : Tuesday, October 12, 2021 - 5:20:36 PM
Contributor : Nathalie Pothier Connect in order to contact the contributor
Submitted on : Tuesday, September 7, 2021 - 9:41:50 AM
Last modification on : Tuesday, October 12, 2021 - 5:20:36 PM
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Distributed under a Creative Commons Attribution 4.0 International License
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- HAL Id : insu-03336222, version 1
- DOI : 10.1007/s10686-021-09709-9
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INSU | OSUC | UNIV-ORLEANS | LPC2E | UNIV-TLSE3 | OBSPM | UP-SCIENCES | PSL | IN2P3 | GALILEE | CEA | IAP | APC | UNIV-COTEDAZUR | SORBONNE-UNIVERSITE | CNRS | SU-SCIENCES | L2IT | SU-TI | OCA | UNIV-PARIS
Citation
Alberto Sesana, Natalia Korsakova, Manuel Sedda, Vishal Baibhav, Enrico Barausse, et al.. Unveiling the gravitational universe at μ-Hz frequencies. Experimental Astronomy, Springer Link, 2021, ⟨10.1007/s10686-021-09709-9⟩. ⟨insu-03336222⟩
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