On the instability of Reissner-Nordstrom black holes in de Sitter backgrounds
Vitor Cardoso, Madalena Lemos, Miguel Marques

TL;DR
This paper analytically proves the instability of higher-dimensional Reissner-Nordstrom-de Sitter black holes, providing insights into their instability mechanisms and confirming previous numerical findings.
Contribution
It offers an analytical proof of black hole instability in higher dimensions and calculates the instability timescale, complementing prior numerical studies.
Findings
Reissner-Nordstrom-de Sitter black holes are unstable in dimensions greater than 6.
Analytical computation of the instability timescale in the near-extremal limit.
Strong agreement between analytical results and previous numerical investigations.
Abstract
Recent numerical investigations have uncovered a surprising result: Reissner-Nordstrom-de Sitter black holes are unstable for spacetime dimensions larger than 6. Here we prove the existence of such instability analytically, and we compute the timescale in the near-extremal limit. We find very good agreement with the previous numerical results. Our results may me helpful in shedding some light on the nature of the instability.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
