Fast Radio Bursts as probes of the late-time universe: A new insight on the Hubble tension

Fast Radio Bursts (FRBs) are bright radio transient events, a subset of which have been localized to their host galaxies. Their high dispersion measures offer valuable insights into the ionized plasma along their line of sight, enabling them to serve as probes of cosmological parameters . One of the major challenges in contemporary cosmology is the Hubble tension — an unresolved discrepancy between two independent methods of determining the Universe’s expansion rate, yielding differing values for the Hubble constant . In this study, we analyze a sample of 64 extragalactic, localized FRBs observed by various telescopes, employing Bayesian analysis with distinct likelihood functions. Our findings suggest that FRBs serve as tracers of the Hubble constant in the late-time Universe. Notably, our results exhibit smaller error bars compared to previous studies, and the derived Hubble constant with 1 σ error bars no longer overlap with those obtained from early-Universe measurements. These results underscore the continuing tension between early- and late-time measurements of the Hubble constant.

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Publication Details

Journal
Physics of the Dark Universe
Published
2025-04-18
DOI
https://doi.org/10.1016/j.dark.2025.101926
Citations
11
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
12.70

Funders

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article

Fast Radio Bursts as probes of the late-time universe: A new insight on the Hubble tension

Shruti Bhatporia, Amanda Weltman, Surajit Kalita
11 citations
Physics of the Dark Universe
Cosmology and Gravitation Theories
12.70
article

Fast Radio Bursts as probes of the late-time universe: A new insight on the Hubble tension

Shruti Bhatporia, Amanda Weltman, Surajit Kalita
article en
11 citations

Abstract

Fast Radio Bursts (FRBs) are bright radio transient events, a subset of which have been localized to their host galaxies. Their high dispersion measures offer valuable insights into the ionized plasma along their line of sight, enabling them to serve as probes of cosmological parameters . One of the major challenges in contemporary cosmology is the Hubble tension — an unresolved discrepancy between two independent methods of determining the Universe’s expansion rate, yielding differing values for the Hubble constant . In this study, we analyze a sample of 64 extragalactic, localized FRBs observed by various telescopes, employing Bayesian analysis with distinct likelihood functions. Our findings suggest that FRBs serve as tracers of the Hubble constant in the late-time Universe. Notably, our results exhibit smaller error bars compared to previous studies, and the derived Hubble constant with 1 σ error bars no longer overlap with those obtained from early-Universe measurements. These results underscore the continuing tension between early- and late-time measurements of the Hubble constant.

Physics of the Dark UniverseVol. 48
African Institute for Mathematical Sciences (ZA), University of Cape Town (ZA), Astronomical Observatory (RS), University of Warsaw (PL)
Simons Foundation, National Research Foundation, University of Capetown, Department of Science and Technology, Ministry of Science and Technology, India, Abdus Salam International Centre for Theoretical Physics, Narodowe Centrum Nauki
Climate action
Openalex Percentile: Top 1%
Cosmology and Gravitation Theories
12.70
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