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  Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA

The KAGRA Collaboration, The LIGO Scientific Collaboration, The Virgo Collaboration, Abbott, B. P., Abbott, R., Abbott, T. D., et al. (2018). Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA. Living Reviews in Relativity, 21: 3. doi:10.1007/s41114-018-0012-9.

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The KAGRA Collaboration, Autor              
The LIGO Scientific Collaboration, Autor              
The Virgo Collaboration, Autor              
Abbott, B. P., Autor
Abbott, R., Autor
Abbott, T. D., Autor
Abernathy, M. R., Autor
Acernese, F., Autor
Ackley, K., Autor
Adams, C., Autor
Adams, T., Autor
Addesso, P., Autor
Adhikari, R. X., Autor
Adya, V. B.1, Autor
Affeldt, C.2, Autor           
Agathos, M., Autor
Agatsuma, K., Autor
Aggarwal, N., Autor
Aguiar, O. D., Autor
Aiello, L., Autor
mehr..
Affiliations:
1AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, Hannover, DE, ou_24009              
2Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24010              
3Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24011              
4Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_1933290              
5AEI-Golm, MPI for Gravitational Physics, Max Planck Society, Golm, DE, ou_24008              
6Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24013              

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Schlagwörter: General Relativity and Quantum Cosmology, gr-qc, Astrophysics, High Energy Astrophysical Phenomena, astro-ph.HE
 Zusammenfassung: We present possible observing scenarios for the Advanced LIGO, Advanced Virgo
and KAGRA gravitational-wave detectors over the next decade, with the intention
of providing information to the astronomy community to facilitate planning for
multi-messenger astronomy with gravitational waves. We estimate the sensitivity
of the network to transient gravitational-wave signals, and study the
capability of the network to determine the sky location of the source. We
report our findings for gravitational-wave transients, with particular focus on
gravitational-wave signals from the inspiral of binary neutron star systems,
which are the most promising targets for multi-messenger astronomy. The ability
to localize the sources of the detected signals depends on the geographical
distribution of the detectors and their relative sensitivity, and 90% credible
regions can be as large as thousands of square degrees when only two sensitive
detectors are operational. Determining the sky position of a significant
fraction of detected signals to areas of 5-20 square degrees requires at least
three detectors of sensitivity within a factor of ~2 of each other and with a
broad frequency bandwidth. When all detectors, including KAGRA and the third
LIGO detector in India, reach design sensitivity, a significant fraction of
gravitational-wave signals will be localized to a few square degrees by
gravitational-wave observations alone.

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 Datum: 2013-04-022018-04-262018
 Publikationsstatus: Online veröffentlicht
 Seiten: 54 pages, 8 figures, 3 tables. Updated to match version published in Living Reviews in Relativity. Sensitivity curves available from https://dcc.ligo.org/LIGO-P1200087-v47/public Science summary available from https://www.ligo.org/science/Publication-ObservingScenario-2/index.php
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Titel: Living Reviews in Relativity
Genre der Quelle: Zeitschrift
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Seiten: - Band / Heft: 21 Artikelnummer: 3 Start- / Endseite: - Identifikator: -