TY - GEN
T1 - Was it Really a Kerr Black Hole That EHT Imaged in 2019?
AU - Chakraborty, Chandrachur
N1 - Publisher Copyright:
© The Author(s), under exclusive license to Springer Nature Switzerland AG 2025.
PY - 2025
Y1 - 2025
N2 - By using the working hypothesis of a Kerr black hole (BH), the Event Horizon Telescope was able to map M87* to the Kerr BH, and it was shown that the observed image of M87* is generally consistent with what would be expected for a Kerr black hole’s shadow. Here, it is demonstrated that M87* is not certainly a Kerr BH, but rather that it might be a Kerr naked singularity, or a BH/naked singularity with a gravitomagnetic monopole, since the alternatives to the Kerr BH cannot be ruled out.
AB - By using the working hypothesis of a Kerr black hole (BH), the Event Horizon Telescope was able to map M87* to the Kerr BH, and it was shown that the observed image of M87* is generally consistent with what would be expected for a Kerr black hole’s shadow. Here, it is demonstrated that M87* is not certainly a Kerr BH, but rather that it might be a Kerr naked singularity, or a BH/naked singularity with a gravitomagnetic monopole, since the alternatives to the Kerr BH cannot be ruled out.
UR - https://www.scopus.com/pages/publications/105023432350
UR - https://www.scopus.com/pages/publications/105023432350#tab=citedBy
U2 - 10.1007/978-3-031-90186-7_29
DO - 10.1007/978-3-031-90186-7_29
M3 - Conference contribution
AN - SCOPUS:105023432350
SN - 9783031901850
T3 - Astrophysics and Space Science Proceedings
SP - 369
EP - 376
BT - The Relativistic Universe
A2 - Ghosh, Shubhrangshu
A2 - Rao, A.R.
PB - Springer Science and Business Media B.V.
T2 - 1st International Symposium on Recent Developments in Relativistic Astrophysics, ISRA 2023
Y2 - 11 December 2023 through 13 December 2023
ER -