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PreprintCC BY-NC-SA 4.0arXiv

Reissner-Nordstrom in the Bertotti-Robinson-Bonnor-Melvin electromagnetic field

Abstract

The magnetic Reissner-Nordstrom black hole embedded into the Bertotti-Robinson magnetic field is presented. Then it is used, as a seed, to generate, through the Harrison transformation of the Ersnt's equations, the Reissner-Nordstrom metric in the Bertotti-Robinson-Bonnor-Melvin magnetic field. Special cases generalising, the vacuum hairy type I Schwarzschild solution is discussed. The local equivalence between various forms of the Schwarzschild-Bertotti-Robinson is shown by exhibiting the explicit diffeomorphism.

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BibTeX
@misc{astorino2026reissnernordstrom,
  title = {{Reissner-Nordstrom in the Bertotti-Robinson-Bonnor-Melvin electromagnetic field}},
  author = {Marco Astorino},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2609.00882},
  eprint = {2609.00882},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.00882},
  note = {CC BY-NC-SA 4.0},
}
RIS
TY  - UNPB
TI  - Reissner-Nordstrom in the Bertotti-Robinson-Bonnor-Melvin electromagnetic field
AU  - Marco Astorino
PY  - 2026
DA  - 2026/10/20
PB  - arXiv
DO  - 10.48550/arxiv.2609.00882
UR  - https://arxiv.org/abs/2609.00882
AB  - The magnetic Reissner-Nordstrom black hole embedded into the Bertotti-Robinson magnetic field is presented. Then it is used, as a seed, to generate, through the Harrison transformation of the Ersnt's equations, the Reissner-Nordstrom metric in the Bertotti-Robinson-Bonnor-Melvin magnetic field. Special cases generalising, the vacuum hairy type I Schwarzschild solution is discussed. The local equivalence between various forms of the Schwarzschild-Bertotti-Robinson is shown by exhibiting the explicit diffeomorphism.
ER  -