Numerical simulations in 4+1 dimensions show near-extremal Schwarzschild-de Sitter black holes forming from gravitational wave collapse with mass over 99% of the extremal limit, suggesting the third law may not apply in cosmological settings.
(2023) Equivalence principle, de-Sitter space, and cosmological twistors
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
gr-qc 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Near--extremal gravitational collapse in 4+1 dimensions: Schwarzschild--de--Sitter space
Numerical simulations in 4+1 dimensions show near-extremal Schwarzschild-de Sitter black holes forming from gravitational wave collapse with mass over 99% of the extremal limit, suggesting the third law may not apply in cosmological settings.