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

Arca Sedda, Manuel (author)
Berry, Christopher P. L. (author)
Jani, Karan (author)
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Amaro-Seoane, Pau (author)
Auclair, Pierre (author)
Baird, Jonathon (author)
Baker, Tessa (author)
Berti, Emanuele (author)
Breivik, Katelyn (author)
Caprini, Chiara (author)
Chen, Xian (author)
Doneva, Daniela (author)
Ezquiaga, Jose M. (author)
Ford, K. E. Saavik (author)
Katz, Michael L. (author)
Kolkowitz, Shimon (author)
McKernan, Barry (author)
Mueller, Guido (author)
Nardini, Germano (author)
Pikovski, Igor (author)
Stockholms universitet,Fysikum,Stevens Institute of Technology, USA
Rajendran, Surjeet (author)
Sesana, Alberto (author)
Shao, Lijing (author)
Tamanini, Nicola (author)
Warburton, Niels (author)
Witek, Helvi (author)
Wong, Kaze (author)
Zevin, Michael (author)
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 (creator_code:org_t)
2021-04-29
2021
English.
In: Experimental astronomy. - : Springer Science and Business Media LLC. - 0922-6435 .- 1572-9508. ; 51, s. 1427-1440
Related links:
https://doi.org/10.1...
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  • Journal article (peer-reviewed)
Abstract Subject headings
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  • 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 LISA will provide gravitational-wave observations of massive black holes binaries. Between the similar to 10-10(3) Hz band of ground-based observatories and the similar to 10(-4)-10(- 1) Hz band of LISA lies the uncharted decihertz gravitational-wave band. We propose a Decihertz Observatory to study this frequency range, and to complement observations made by other detectors. Decihertz observatories are well suited to observation of intermediate-mass (similar to 10(2)-10(4)M(circle dot)) black holes; they will be able to detect stellar-mass binaries days to years before they merge, providing early warning of nearby binary neutron star mergers and measurements of the eccentricity of binary black holes, and they will enable new tests of general relativity and the Standard Model of particle physics. Here we summarise how a Decihertz Observatory could provide unique insights into how black holes form and evolve across cosmic time, improve prospects for both multimessenger astronomy and multiband gravitational-wave astronomy, and enable new probes of gravity, particle physics and cosmology.

Subject headings

NATURVETENSKAP  -- Fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences (hsv//eng)

Keyword

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

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ref (subject category)
art (subject category)

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