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Testing Einstein's Equivalence Principle with Cosmological Fast Radio Bursts behind Clusters of Galaxies

2016/01/15 by Shuang-Nan Zhang, Shuang‐Nan Zhang, Zhang, Shuang-Nan · 2 citations
Mathematics · Physics and Astronomy · #Cosmology and Nongalactic Astrophysics (astro-ph.CO) #FOS: Physical sciences #Gamma-ray bursts and supernovae #General Relativity and Quantum Cosmology (gr-qc) #High Energy Astrophysical Phenomena (astro-ph.HE) #Pulsars and Gravitational Waves Research #Statistical and numerical algorithms #astro-ph.CO #astro-ph.HE #gr-qc

paper · pdf · doi:10.48550/arxiv.1601.04558

2 pages; submitted to A&A research note on Jan. 13th, 2016

arxiv created 2016/01/15 · openalex publication_date 2016/01/15 · arxiv updated 2016/01/19 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

Aims: Recently, cosmological fast radio bursts (FRBs) have been used to provide the most stringent limit up to date on Einstein's Equivalence Principle (EEP). We study how to further test EEP with FRBs. Methods: Future systematic radio surveys will certainly find abundant FRBs at cosmological distances and some of them will inevitably be located behind clusters of galaxies. Here we suggest to use those FRBs to further test EEP. Results: We find that the robustness and accuracy of testing EEP can be improved further by orders of magnitude with these FRBs. The same methodology can also be applied to any other types of fast and bright transients at cosmological distances.

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