A toy-model resolving the black hole information paradox

Abstract

This dissertation focuses on how considering a toy model that allows non-local gravitational interaction among the Hawking radiated pairs along with the chosen bell pair state gets closer to resolving the black hole information paradox. We begin by presenting some of the required background on Hawking radiation and the small correction to the leading order Hawking state before focusing on the non-local gravitational interaction prescription of the toy model for the entanglement entropy. We show how introducing two new parameters, which depend on mass depletion rate of a Black Hole and interactions between Hawking radiated pairs leads to the decrease of the leading order Hawking state entanglement entropy resulting in the recovery of information.