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Constraints on black hole charges in M87* and Sgr A* with the EHT observations
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Constraints on black hole charges in M87* and Sgr A* with the EHT observations
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In May 2022 ICRANet organized the Workshop dedicated to the 80th anniversary of Professor Ruffini. This paper is based on the talk delivered at the meeting. Professor Ruffini was well known for Soviet scientific community not only due to his publications in leading journals but also due Russian translations of his books where he was an author or a contributor in collection of articles. But only in 1988 I had an opportunity to watch and listen professor R. Ruffini at the Conference dedicated to the century since the birthday of Alexander Alexandrovich Friedmann. This conference was organized in Leningrad (Soviet Union) in June during a short magic period when there are white nights there. In June 2023 we celebrate the 135th anniversary of Friedmann's birth. Friedmann and his closed friend V. K. Frederics were the founders of Soviet school of general relativity and George Gamow was one of the brilliant representative of the school and he was the author of the hot Universe model which is the most popular now. In the USSR a development of general relativity and relativistic cosmology was not smooth and only in sixties of the last century these branches of science freed from the total control of representatives of the ideology of Marxism -- Leninism. I also discussed a Soviet contribution in a discovery of cosmic microwave background radiation done by T. Shmaonov in 1957 and reasons why his supervisors did not connect these results with the hot Universe models discussed by G. Gamow. Author's results about observational features of supemassive black holes (including the black hole in our Galactic Center) are also briefly discussed, it was considered an opportunity to evaluate a (tidal) charge of Reissner -- Nordstr\"om black hole from observational estimates of shadow size in the Galactic Center and M87* done by the EHT Collaboration based its observations in April 2017.
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Cited by 1 Pith paper
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Observational Limits on Einasto Dark Matter Parameters from Event Horizon Telescope Images of Sgr A$^{*}$ and M87$^{*}$
EHT dimensionless shadow diameters plus stellar-dynamical mass priors constrain Einasto central density to ρ₀ ≲ 10^{-11} M⊙/pc³ (1σ) for Sgr A*, with weaker bounds for M87*.
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