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- W3122207551 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 $40^{circ}$ 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 $H_0$ 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." @default.
- W3122207551 created "2021-02-01" @default.
- W3122207551 creator A5006651636 @default.
- W3122207551 creator A5009825889 @default.
- W3122207551 creator A5041943317 @default.
- W3122207551 creator A5052211605 @default.
- W3122207551 date "2021-10-08" @default.
- W3122207551 modified "2023-09-29" @default.
- W3122207551 title "Forecast for cosmological parameter estimation with gravitational-wave standard sirens from the LISA-Taiji network" @default.
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