## Detalles de publicación

PP 023063

## Revisiting constraints on the photon rest mass with cosmological fast radio bursts

(1) Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023, China; (2) School of Astronomy and Space Sciences, University of Science and Technology of China, Hefei 230026, China; (3) Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain; (4) PIFI-Visiting Scientist 2023 of China Academy of Sciences at Purple Mountain Observatory, Nanjing 210023 and National Astronomical Observatories, Beijing 100012, China; (5) Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain

Fast radio bursts (FRBs) have been suggested as an excellent celestial laboratory for testing the zero-mass hypothesis of the photon. In this work, we use the dispersion measure (DM)–redshift measurements of 23 localized FRBs to revisit the photon rest mass mγ. As an improvement over previous studies, here we take into account the more realistic probability distributions of DMs contributed by the FRB host galaxy and intergalactic medium (IGM)from the IllustrisTNG simulation. To better account for the systematic uncertainty induced by the choices of priors of cosmological parameters, we also combine the FRB data with the cosmic microwave background data, the baryon acoustic oscillation data, and type Ia supernova data to constrain the cosmological parameters and mγ simultaneously. We derive a new upper limit of mγ ≤ 3.8 × 10−51 kg, or equivalently mγ ≤ 2.1 × 10−15 eV/c2 (mγ ≤ 7.2×10−51 kg, or equivalently mγ ≤ 4.0×10−15 eV/c2 ) at 1σ (2σ) confidence level. Meanwhile,

our analysis can also lead to a reasonable estimation for the IGM baryon fraction fIGM =0.873+0.061−0.050. With the number increment of localized FRBs, the constraints on both mγ and fIGM will be further improved. A caveat of constraining mγ within the context of the standard ΛCDM cosmological model is also discussed.

our analysis can also lead to a reasonable estimation for the IGM baryon fraction fIGM =0.873+0.061−0.050. With the number increment of localized FRBs, the constraints on both mγ and fIGM will be further improved. A caveat of constraining mγ within the context of the standard ΛCDM cosmological model is also discussed.