Email this article Sagnac effect in the spacetime of tidal black holes
- Authors: Karimov R.K.1, Izmailov R.N.1,2, Yusupova R.M.1,2, Bhattacharya A.3
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Affiliations:
- M. Akmullah Bashkir State Pedagogical University
- Institute of Molecule and Crystal Physics, Ufa Federal Research Centre of the Russian Academy of Sciences
- Kidderpore College
- Issue: Vol 89, No 3 (2025)
- Pages: 482–487
- Section: Electronic, Spin and Quantum Processes in Molecular and Crystalline Systems
- URL: https://journal-vniispk.ru/0367-6765/article/view/301663
- DOI: https://doi.org/10.31857/S0367676525030253
- EDN: https://elibrary.ru/FTXMHZ
- ID: 301663
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Abstract
We study the Sagnac effect in the space-time of a spinning black hole with a tidal charge ?. It is shown that the greatest influence of the tidal (electric) charge is occured at close distances to the black hole. An increase in the tidal charge leads to an increase in the Sagnac delay. Numerical estimates have shown that for the Earth, the Sagnac delay is determined in the range from –63.8 to –1.5 ns.
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About the authors
R. Kh. Karimov
M. Akmullah Bashkir State Pedagogical University
Email: karimov_ramis_92@mail.ru
Ufa, 450077 Russia
R. N. Izmailov
M. Akmullah Bashkir State Pedagogical University; Institute of Molecule and Crystal Physics, Ufa Federal Research Centre of the Russian Academy of SciencesUfa, 450077 Russia; Ufa, 450075 Russia
R. M. Yusupova
M. Akmullah Bashkir State Pedagogical University; Institute of Molecule and Crystal Physics, Ufa Federal Research Centre of the Russian Academy of SciencesUfa, 450077 Russia; Ufa, 450075 Russia
A. Bhattacharya
Kidderpore CollegeKolkata, 700023 India
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