Black hole horizon fluctuations
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Cited by (45)
Non-trivial quantum fluctuations in asymptotically non-flat black-hole space–times
2022, Annals of PhysicsCitation Excerpt :Hawking’s original derivation ignores the radiation’s interaction with matter and requires the incoming vacuum modes with frequencies far above the Planck scale. One way to address both these assumptions is not to make the horizon a fixed surface, but a dynamical one that changes due to the backreaction of the quantum modes [16,37]. Such an approach is also consistent within the framework of effective field theory [11,13].
Quantum black hole wave packet: Average area entropy and temperature dependent width
2014, Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy PhysicsEnhanced geometry fluctuations in Minkowski and black hole spacetimes
2008, Classical and Quantum GravityStochastic gravity: A primer with applications
2003, Classical and Quantum GravityElectroweak Phase Transition Near the Event Horizon of a Schwarzschild Black Hole
2024, International Journal of Theoretical Physics
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