Forecast for cosmological parameter estimation with gravitational-wave standard sirens from the LISA-Taiji network
TLDR
In this paper, the cosmological parameter estimation with the standard siren observations from the LISA-Taiji network was analyzed and it was shown that the standard Siren data from LISA and Taiji can provide much tighter constraints on cosmology parameters, e.g., the constraint precision of w reaches about 4%.Abstract:
LISA and Taiji are expected to form a space-based gravitational-wave (GW) detection network in the future. In this work, we make a forecast for the cosmological parameter estimation with the standard siren observation from the LISA-Taiji network. We simulate the standard siren data based on a scenario with configuration angle of 40° between LISA and Taiji. Three models for the population of massive black hole binary (MBHB), i.e., pop III, Q3d, and Q3nod, are considered to predict the events of MBHB mergers. We find that, based on the LISA-Taiji network, the number of electromagnetic (EM) counterparts detected is almost doubled compared with the case of single Taiji mission. Therefore, the LISA-Taiji network’s standard siren observation could provide much tighter constraints on cosmological parameters. For example, solely using the standard sirens from the LISA-Taiji network, the constraint precision of H0 could reach 1.3%. Moreover, combined with the CMB data, the GW-EM observation based on the LISA-Taiji network could also tightly constrain the equation of state of dark energy, e.g., the constraint precision of w reaches about 4%, which is comparable with the result of CMB+BAO+SN. It is concluded that the GW standard sirens from the LISA-Taiji network will become a useful cosmological probe in understanding the nature of dark energy in the future.read more
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The Gravitational-Wave Physics II: Progress
Ligong Bian,Rong-Gen Cai,Shuo Cao,Zhoujian Cao,He Gao,Zong-Kuan Guo,Kejia Lee,Di Li,Jing Liu,Youjun Lu,Shi Pi,Jian-Min Wang,Shao-Jiang Wang,Yan Wang,Tao Yang,Xing-Yu Yang,Shenghua Yu,Xin Zhang +17 more
TL;DR: In this article, the authors summarize the recent progress over the past five years, but with a special focus on some of their own works for the Key Project ''Physics associated with the gravitational waves'' supported by the National Natural Science Foundation of China.
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How can gravitational-wave standard sirens and 21 cm intensity mapping jointly provide a precise late-universe cosmological probe?
TL;DR: In this article, a forecast for cosmological parameter estimation with the synergy between the GW standard siren observations and the neutral hydrogen 21 cm IM surveys was made, and the results showed that the magnificent prospects for non-optical precision cosmology are worth expecting.
Journal ArticleDOI
The Gravitational-wave physics II: Progress
Ligong Bian,Rong-Gen Cai,Shuo Cao,Zhoujian Cao,He Gao,Zong-Kuan Guo,Kejia Lee,Kejia Lee,Di Li,Jing Liu,Youjun Lu,Shi Pi,Jian-Min Wang,Shao-Jiang Wang,Yan Wang,Tao Yang,Xing-Yu Yang,Shenghua Yu,Xin Zhang,Xin Zhang +19 more
TL;DR: In this paper, the authors presented the mechanism of the gravitational-wave production during some physical processes of the early Universe, such as inflation, preheating and phase transition, and the cosmological implications of the measurements.
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TL;DR: The association of GRB 170817A, detected by Fermi-GBM 1.7 s after the coalescence, corroborates the hypothesis of a neutron star merger and provides the first direct evidence of a link between these mergers and short γ-ray bursts.
Journal ArticleDOI
The Cosmological Constant Problem
TL;DR: In this article, five different approaches to the cosmological constant problem are described, and a brief review of the history of this problem is given. But none of the approaches are considered in this paper.
Journal ArticleDOI
First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Preliminary maps and basic results
Charles L. Bennett,Mark Halpern,Gary Hinshaw,N. Jarosik,Alan J. Kogut,Michele Limon,Michele Limon,S. S. Meyer,Lyman A. Page,David N. Spergel,Gregory S. Tucker,Gregory S. Tucker,Gregory S. Tucker,Edward J. Wollack,Edward L. Wright,Cris W. Barnes,M. R. Greason,Robert S. Hill,Eiichiro Komatsu,M. R. Nolta,N. Odegard,Hiranya V. Peiris,Licia Verde,Janet Weiland +23 more
TL;DR: In this paper, the authors present full sky microwave maps in five frequency bands (23 to 94 GHz) from the WMAP first year sky survey, which are consistent with the 7 in. full-width at half-maximum (FWHM) Cosmic Background Explorer (COBE) maps.