The missing link in gravitational-wave astronomy: A summary of discoveries waiting in the decihertz range.

Binary evolution Black holes Decihertz observatories Gravitational waves Intermediate-mass black holes Multiband gravitational-wave astronomy Multimessenger astronomy Neutron stars Space-based detectors Stochastic backgrounds Tests of general relativity Voyage 2050 White dwarfs

Journal

Experimental astronomy
ISSN: 1572-9508
Titre abrégé: Exp Astron (Dordr)
Pays: Netherlands
ID NLM: 101769314

Informations de publication

Date de publication:
2021
Historique:
received: 03 08 2020
accepted: 09 02 2021
entrez: 1 11 2021
pubmed: 2 11 2021
medline: 2 11 2021
Statut: ppublish

Résumé

Since 2015 the gravitational-wave observations of LIGO and Virgo have transformed our understanding of compact-object binaries. In the years to come, ground-based gravitational-wave observatories such as LIGO, Virgo, and their successors will increase in sensitivity, discovering thousands of stellar-mass binaries. In the 2030s, the space-based

Identifiants

DOI: 10.1007/s10686-021-09713-z PMID: 34720416 PMC: PMC8536607
pubmed: 34720416
doi: 10.1007/s10686-021-09713-z
pii: 9713
pmc: PMC8536607
doi:

Types de publication

Journal Article

Langues

eng

Pagination

1427-1440

Informations de copyright

© The Author(s) 2021.

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Auteurs

Manuel Arca Sedda (MA)

Astronomisches Rechen-Institut, Zentrüm für Astronomie, Universität Heidelberg, Mönchofstr. 12-14, Heidelberg, Germany.

Christopher P L Berry (CPL)

Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), Department of Physics and Astronomy, Northwestern University, 2145 Sheridan Road, Evanston, IL 60208 USA.
SUPA, School of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ UK.
ORCID: 0000-0003-3870-7215

Karan Jani (K)

Department of Physics and Astronomy, Vanderbilt University, Nashville, TN 37212 USA.

Pau Amaro-Seoane (P)

Universitat Politècnica de València, IGIC, Valencia, Spain.
Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing, 100871 China.
Institute of Applied Mathematics, Academy of Mathematics and Systems Science, CAS, Beijing, 100190 China.
Zentrum für Astronomie und Astrophysik, TU Berlin, Hardenbergstraße 36, 10623 Berlin, Germany.

Pierre Auclair (P)

Laboratoire Astroparticule et Cosmologie, CNRS UMR 7164, Université Paris-Diderot, 10 rue Alice Domon et Léonie Duquet, 75013 Paris, France.

Jonathon Baird (J)

High Energy Physics Group, Physics Department, Imperial College London, Blackett Laboratory, Prince Consort Road, London, SW7 2BW UK.

Tessa Baker (T)

School of Physics and Astronomy, Queen Mary University of London, Mile End Road, London, E1 4NS UK.

Emanuele Berti (E)

Department of Physics and Astronomy, Johns Hopkins University, 3400 N. Charles Street, Baltimore, MD 21218 USA.

Katelyn Breivik (K)

Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St. George Street, Toronto, Ontario M5S 1A7 Canada.

Chiara Caprini (C)

Laboratoire Astroparticule et Cosmologie, CNRS UMR 7164, Université Paris-Diderot, 10 rue Alice Domon et Léonie Duquet, 75013 Paris, France.

Xian Chen (X)

Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing, 100871 China.
Astronomy Department, School of Physics, Peking University, Beijing, 100871 China.

Daniela Doneva (D)

Theoretical Astrophysics, Eberhard Karls University of Tübingen, Tübingen, 72076 Germany.

Jose M Ezquiaga (JM)

Kavli Institute for Cosmological Physics, Enrico Fermi Institute, The University of Chicago, Chicago, IL 60637 USA.

K E Saavik Ford (KES)

City University of New York-BMCC, Chambers St, New York, NY 10007 USA.
Department of Astrophysics, American Museum of Natural History, New York, NY 10028 USA.

Michael L Katz (ML)

Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), Department of Physics and Astronomy, Northwestern University, 2145 Sheridan Road, Evanston, IL 60208 USA.

Shimon Kolkowitz (S)

Department of Physics, University of Wisconsin - Madison, Madison, WI 53706 USA.

Barry McKernan (B)

City University of New York-BMCC, Chambers St, New York, NY 10007 USA.
Department of Astrophysics, American Museum of Natural History, New York, NY 10028 USA.

Guido Mueller (G)

Department of Physics, University of Florida, PO Box 118440, Gainesville, Florida 32611 USA.

Germano Nardini (G)

Faculty of Science and Technology, University of Stavanger, 4036 Stavanger, Norway.

Igor Pikovski (I)

Department of Physics, Stevens Institute of Technology, Hoboken, NJ 07030 USA.
Department of Physics, Stockholm University, SE-10691 Stockholm, Sweden.

Surjeet Rajendran (S)

Department of Physics and Astronomy, Johns Hopkins University, 3400 N. Charles Street, Baltimore, MD 21218 USA.

Alberto Sesana (A)

Università di Milano Bicocca, Dipartimento di Fisica G. Occhialini, Piazza della Scienza 3, I-20126 Milano, Italy.

Lijing Shao (L)

Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing, 100871 China.
National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012 China.

Nicola Tamanini (N)

Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Am Mühlenberg 1, 14476 Potsdam-Golm, Germany.

Niels Warburton (N)

School of Mathematics and Statistics, University College Dublin, Belfield, Dublin 4 Ireland.

Helvi Witek (H)

Department of Physics, King's College London, Strand, London WC2R 2LS UK.

Kaze Wong (K)

Department of Physics and Astronomy, Johns Hopkins University, 3400 N. Charles Street, Baltimore, MD 21218 USA.

Michael Zevin (M)

Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), Department of Physics and Astronomy, Northwestern University, 2145 Sheridan Road, Evanston, IL 60208 USA.

Classifications MeSH