Black Hole Information Problem and Wave Bursts

Abstract

By reexamination of the boundary conditions of wave equation on a black hole horizon it is found not harmonic, but real-valued exponentially time-dependent solutions. This means that quantum particles probably do not cross the Schwarzschild horizon, but are absorbed and some are reflected by it, what potentially can solve the famous black hole information paradox. To study this strong gravitational lensing we are introducing an effective negative cosmological constant between the Schwarzschild and photon spheres. It is shown that the reflected particles can obtain their additional energy in this effective AdS space and could explain properties of some unusually strong signals, like LIGO events, gamma ray and fast radio bursts.

The version accepted by Int. J. Theor. Phys

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Cited by in corpus (7)

• Can Quantum Particles Cross a Horizon?
• Quantum Back Flow Across a Black Hole Horizon in a Toy Model Approach
• Probing the Information-Probabilistic Description
• Einstein's hole argument and Schwarzschild singularities
• Hawking radiation as quantum mechanical reflection
• On the singular coordinate transformations of the Schwarzschild metric
• Black Holes and Baryon Number Violation: Unveiling the Origins of Early Galaxies and the Low-Mass Gap