Details
| Originalsprache | Englisch |
|---|---|
| Aufsatznummer | 76 |
| Fachzeitschrift | Astrophysical Journal |
| Jahrgang | 949 |
| Ausgabenummer | 2 |
| Publikationsstatus | Veröffentlicht - 7 Juni 2023 |
Abstract
ASJC Scopus Sachgebiete
- Physik und Astronomie (insg.)
- Astronomie und Astrophysik
- Erdkunde und Planetologie (insg.)
- Astronomie und Planetologie
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in: Astrophysical Journal, Jahrgang 949, Nr. 2, 76, 07.06.2023.
Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review
}
TY - JOUR
T1 - Constraints on the cosmic expansion history from GWTC-3
AU - The LIGO Scientific Collaboration
AU - The Virgo Collaboration
AU - the KAGRA Collaboration
AU - Adya, V. B.
AU - Bose, S.
AU - Brown, D. D.
AU - Carlassara, M.
AU - Chatterjee, C.
AU - Chen, X.
AU - Chen, Y.-B.
AU - Chen, Y.-R.
AU - Cheng, H.
AU - Choudhary, R. K.
AU - Danilishin, S.
AU - Danzmann, K.
AU - Guo, H.-K.
AU - Hansen, H.
AU - Hennig, J.
AU - Heurs, M.
AU - Hreibi, A.
AU - Hübner, M. T.
AU - Isleif, K.
AU - Knust, N.
AU - Lang, R. N.
AU - Lee, H. M.
AU - Lee, H. W.
AU - Lehmann, J.
AU - Li, J.
AU - Li, X.
AU - Lück, H.
AU - More, A.
AU - Nguyen, T.
AU - Richardson, L.
AU - Rose, C. A.
AU - Roy, S.
AU - Sanders, J. R.
AU - Schmidt, P.
AU - Schmidt, S.
AU - Sun, L.
AU - Wilken, D.
AU - Willke, B.
AU - Wu, D. S.
AU - Wu, H.
AU - Yamamoto, K.
AU - Zhang, H.
AU - Zhang, L.
AU - Zhang, R.
AU - Zhang, Y.
AU - Zhou, Z.
AU - Zhu, X. J.
AU - Klinger, T.
AU - Li, P.
AU - Pham, H.
AU - Affeldt, C.
AU - Bergamin, F.
AU - Bisht, A.
AU - Bode, N.
AU - Booker, P.
AU - Brinkmann, M.
AU - Gohlke, N.
AU - Heidt, A.
AU - Heinze, J.
AU - Hochheim, S.
AU - Kastaun, W.
AU - Kirchhoff, R.
AU - Koch, P.
AU - Koper, N.
AU - Kringel, V.
AU - Kuehn, G.
AU - Leavey, S.
AU - Lough, J. D.
AU - Matiushechkina, M.
AU - Mehmet, M.
AU - Meylahn, F.
AU - Mukund, N.
AU - Nadji, S. L.
AU - Nery, M.
AU - Ohme, F.
AU - Schneewind, M.
AU - Schulte, B. W.
AU - Schutz, B. F.
AU - Setyawati, Y.
AU - Venneberg, J.
AU - von Wrangel, J.
AU - Weinert, M.
AU - Wellmann, F.
AU - Weßels, Peter
AU - Woehler, J.
AU - Junker, Jonas
PY - 2023/6/7
Y1 - 2023/6/7
N2 - We use 47 gravitational-wave sources from the Third LIGO-Virgo-KAGRA Gravitational-Wave Transient Catalog (GWTC-3) to estimate the Hubble parameter \(H(z)\), including its current value, the Hubble constant \(H_0\). Each gravitational-wave (GW) signal provides the luminosity distance to the source and we estimate the corresponding redshift using two methods: the redshifted masses and a galaxy catalog. Using the binary black hole (BBH) redshifted masses, we simultaneously infer the source mass distribution and \(H(z)\). The source mass distribution displays a peak around \(34\, {\rm M_\odot}\), followed by a drop-off. Assuming this mass scale does not evolve with redshift results in a \(H(z)\) measurement, yielding \(H_0=68^{+12}_{-7} {\rm km\,s^{-1}\,Mpc^{-1}}\) (\(68\%\) credible interval) when combined with the \(H_0\) measurement from GW170817 and its electromagnetic counterpart. This represents an improvement of 17% with respect to the \(H_0\) estimate from GWTC-1. The second method associates each GW event with its probable host galaxy in the catalog GLADE+, statistically marginalizing over the redshifts of each event's potential hosts. Assuming a fixed BBH population, we estimate a value of \(H_0=68^{+8}_{-6} {\rm km\,s^{-1}\,Mpc^{-1}}\) with the galaxy catalog method, an improvement of 42% with respect to our GWTC-1 result and 20% with respect to recent \(H_0\) studies using GWTC-2 events. However, we show that this result is strongly impacted by assumptions about the BBH source mass distribution; the only event which is not strongly impacted by such assumptions (and is thus informative about \(H_0\)) is the well-localized event GW190814.
AB - We use 47 gravitational-wave sources from the Third LIGO-Virgo-KAGRA Gravitational-Wave Transient Catalog (GWTC-3) to estimate the Hubble parameter \(H(z)\), including its current value, the Hubble constant \(H_0\). Each gravitational-wave (GW) signal provides the luminosity distance to the source and we estimate the corresponding redshift using two methods: the redshifted masses and a galaxy catalog. Using the binary black hole (BBH) redshifted masses, we simultaneously infer the source mass distribution and \(H(z)\). The source mass distribution displays a peak around \(34\, {\rm M_\odot}\), followed by a drop-off. Assuming this mass scale does not evolve with redshift results in a \(H(z)\) measurement, yielding \(H_0=68^{+12}_{-7} {\rm km\,s^{-1}\,Mpc^{-1}}\) (\(68\%\) credible interval) when combined with the \(H_0\) measurement from GW170817 and its electromagnetic counterpart. This represents an improvement of 17% with respect to the \(H_0\) estimate from GWTC-1. The second method associates each GW event with its probable host galaxy in the catalog GLADE+, statistically marginalizing over the redshifts of each event's potential hosts. Assuming a fixed BBH population, we estimate a value of \(H_0=68^{+8}_{-6} {\rm km\,s^{-1}\,Mpc^{-1}}\) with the galaxy catalog method, an improvement of 42% with respect to our GWTC-1 result and 20% with respect to recent \(H_0\) studies using GWTC-2 events. However, we show that this result is strongly impacted by assumptions about the BBH source mass distribution; the only event which is not strongly impacted by such assumptions (and is thus informative about \(H_0\)) is the well-localized event GW190814.
KW - astro-ph.CO
KW - gr-qc
KW - Gravitational wave astronomy
KW - Gravitational waves
KW - Gravitational wave sources
UR - http://www.scopus.com/inward/record.url?scp=85163895637&partnerID=8YFLogxK
U2 - 10.3847/1538-4357/ac74bb
DO - 10.3847/1538-4357/ac74bb
M3 - Article
VL - 949
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0004-637X
IS - 2
M1 - 76
ER -