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25 April 2024
 
  » arxiv » 2006.1450

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Cosmological parameter estimation for dynamical dark energy models with future fast radio burst observations
Ze-Wei Zhao ; Zheng-Xiang Li ; Jing-Zhao Qi ; He Gao ; Jing-Fei Zhang ; Xin Zhang ;
Date 2 Jun 2020
AbstractFast radio bursts (FRBs) are a mysterious astrophysical phenomenon of bright pulses emitted at radio frequencies, and it is expected for them to be frequently detected in the future. The dispersion measures of FRBs are related to cosmological parameters, and thus FRBs have a potential to be developed into a new cosmological probe if their data can be largely accumulated in the future. In this work, we study the capability of future FRB data for improving cosmological parameter estimation in two dynamical dark energy models. We find that the simulated FRB data can break the parameter degeneracies inherent in the current cosmic microwave background (CMB) data. Therefore, the combination of the CMB and FRB data can significantly improve the constraints on the Hubble constant and dark energy parameters, compared to those using CMB or FRB alone. If ten thousand events of FRBs with known redshifts are detected in the future, they would behave better than the baryon acoustic oscillation (BAO) data in breaking the parameter degeneracies inherent in the CMB data. We also find that the combination of FRB and gravitational wave (GW) standard siren data provides an independent low-redshift probe to verify the results from CMB and BAO data. For the data combination of CMB, GW, and FRB, it is found that the main contribution to the constraints comes from the CMB and GW data, but the inclusion of FRB data still can evidently improve the constraint on the baryon density.
Source arXiv, 2006.1450
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