Ali, TibraKamal, Ahmed RakinDipro, Savin Shayok2025-05-192025-05-1920242024-12ID 19111001http://hdl.handle.net/10361/25918This thesis is submitted in partial fulfillment of the requirements for the degree of Bachelor of Science in Physics, 2024.Cataloged from PDF version of thesis.Includes bibliographical references (pages 54-58).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.66 pagesenBRAC University thesis reports are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission.Black hole information paradoxNon-local gravitational interactionQuantum mechanicsGravitationHawking radiationGravitation.Quantum field theory.Quantum gravity--Mathematical models.Black holes (Astronomy)--Mathematical models.Thesis