PreprintCC BY 4.0arXiv
On the Extended Kerr-Newman-Bertotti-Robinson Spacetime: Two Black Holes and a Naked Singularity in Bertotti-Robinson Universe
Abstract
We introduce new coordinates that extend the Kerr--Newman--Bertotti--Robinson spacetime consistently with the previous reciprocal continuation. In these coordinates, the two points at Ω=0 are resolved into complete Bertotti--Robinson null infinities. The extended spacetime describes two black holes sharing a common exterior of nontrivial topology, together with a naked ring singularity. In the regular static limit, the new coordinates globally identify the spacetime with the balanced Alekseev--García geometry.
Related
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BibTeX
@misc{zhou2026extended,
title = {{On the Extended Kerr-Newman-Bertotti-Robinson Spacetime: Two Black Holes and a Naked Singularity in Bertotti-Robinson Universe}},
author = {Yu-Sen Zhou and Wen-Tao Fu and Li-Ming Cao and Rong-Gen Cai},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.20626},
eprint = {2609.20626},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.20626},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - On the Extended Kerr-Newman-Bertotti-Robinson Spacetime: Two Black Holes and a Naked Singularity in Bertotti-Robinson Universe
AU - Yu-Sen Zhou
AU - Wen-Tao Fu
AU - Li-Ming Cao
AU - Rong-Gen Cai
PY - 2026
DA - 2026/09/17
PB - arXiv
DO - 10.48550/arxiv.2609.20626
UR - https://arxiv.org/abs/2609.20626
AB - We introduce new coordinates that extend the Kerr--Newman--Bertotti--Robinson spacetime consistently with the previous reciprocal continuation. In these coordinates, the two points at Ω=0 are resolved into complete Bertotti--Robinson null infinities. The extended spacetime describes two black holes sharing a common exterior of nontrivial topology, together with a naked ring singularity. In the regular static limit, the new coordinates globally identify the spacetime with the balanced Alekseev--García geometry.
ER -