Low-redshift constraints on the Hubble constant from the baryon acoustic oscillation “standard rulers” and the gravitational wave “standard sirens”
Abstract The multi-messenger observations of GW170817 indicated a new independent measurement of the Hubble constant ($$H_0$$ H0 ). We obtain the low-redshift cosmological constraints on $$H_0$$ H0 by combining this gravitational wave measurement with the observations of distance scales in baryon ac...
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2019-02-01
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Series: | European Physical Journal C: Particles and Fields |
Online Access: | http://link.springer.com/article/10.1140/epjc/s10052-019-6664-0 |
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doaj-0d78b9c426514e69b2ee8d8e1a093c9a2020-11-25T02:38:26ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522019-02-0179211310.1140/epjc/s10052-019-6664-0Low-redshift constraints on the Hubble constant from the baryon acoustic oscillation “standard rulers” and the gravitational wave “standard sirens”Zhe Chang0Qing-Guo Huang1Sai Wang2Zhi-Chao Zhao3Institute of High Energy Physics, Chinese Academy of SciencesSchool of Physical Sciences, University of Chinese Academy of SciencesDepartment of Physics, The Chinese University of Hong KongInstitute of High Energy Physics, Chinese Academy of SciencesAbstract The multi-messenger observations of GW170817 indicated a new independent measurement of the Hubble constant ($$H_0$$ H0 ). We obtain the low-redshift cosmological constraints on $$H_0$$ H0 by combining this gravitational wave measurement with the observations of distance scales in baryon acoustic oscillations. Using Fisher information matrix, we estimate the projected constraints on $$H_0$$ H0 from Einstein Telescope. Simulating $$10^3$$ 103 gravitational-wave standard sirens from binary neutron star coalescences, we find that Einstein Telescope alone can constrain $$H_0$$ H0 almost as tightly as Planck final data release in the cosmological constant plus cold dark matter model. This constraint can be further improved by combining Einstein Telescope with Dark Energy Spectroscopic Instrument. The Hubble constant tension can thus be checked by observing the standard sirens with Einstein Telescope in the future.http://link.springer.com/article/10.1140/epjc/s10052-019-6664-0 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Zhe Chang Qing-Guo Huang Sai Wang Zhi-Chao Zhao |
spellingShingle |
Zhe Chang Qing-Guo Huang Sai Wang Zhi-Chao Zhao Low-redshift constraints on the Hubble constant from the baryon acoustic oscillation “standard rulers” and the gravitational wave “standard sirens” European Physical Journal C: Particles and Fields |
author_facet |
Zhe Chang Qing-Guo Huang Sai Wang Zhi-Chao Zhao |
author_sort |
Zhe Chang |
title |
Low-redshift constraints on the Hubble constant from the baryon acoustic oscillation “standard rulers” and the gravitational wave “standard sirens” |
title_short |
Low-redshift constraints on the Hubble constant from the baryon acoustic oscillation “standard rulers” and the gravitational wave “standard sirens” |
title_full |
Low-redshift constraints on the Hubble constant from the baryon acoustic oscillation “standard rulers” and the gravitational wave “standard sirens” |
title_fullStr |
Low-redshift constraints on the Hubble constant from the baryon acoustic oscillation “standard rulers” and the gravitational wave “standard sirens” |
title_full_unstemmed |
Low-redshift constraints on the Hubble constant from the baryon acoustic oscillation “standard rulers” and the gravitational wave “standard sirens” |
title_sort |
low-redshift constraints on the hubble constant from the baryon acoustic oscillation “standard rulers” and the gravitational wave “standard sirens” |
publisher |
SpringerOpen |
series |
European Physical Journal C: Particles and Fields |
issn |
1434-6044 1434-6052 |
publishDate |
2019-02-01 |
description |
Abstract The multi-messenger observations of GW170817 indicated a new independent measurement of the Hubble constant ($$H_0$$ H0 ). We obtain the low-redshift cosmological constraints on $$H_0$$ H0 by combining this gravitational wave measurement with the observations of distance scales in baryon acoustic oscillations. Using Fisher information matrix, we estimate the projected constraints on $$H_0$$ H0 from Einstein Telescope. Simulating $$10^3$$ 103 gravitational-wave standard sirens from binary neutron star coalescences, we find that Einstein Telescope alone can constrain $$H_0$$ H0 almost as tightly as Planck final data release in the cosmological constant plus cold dark matter model. This constraint can be further improved by combining Einstein Telescope with Dark Energy Spectroscopic Instrument. The Hubble constant tension can thus be checked by observing the standard sirens with Einstein Telescope in the future. |
url |
http://link.springer.com/article/10.1140/epjc/s10052-019-6664-0 |
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