Analysis of quantum evaporation process of black holes in the model of Expansive Nondecelerative Universe

TL;DR

This paper examines black hole quantum evaporation within the Expansive Nondecelerative Universe model, concluding that black holes cannot fully evaporate and may reach a thermodynamic equilibrium, aligning with the second law.

Contribution

It introduces a new perspective on black hole evaporation in the ENU model, showing the possibility of equilibrium states contrary to traditional Hawking evaporation.

Findings

Black holes cannot fully evaporate in the ENU model

An equilibrium between gravitation creation and evaporation can occur

Black hole horizon surface remains constant at equilibrium

Abstract

In the model of Expansive Nondecelerative Universe, black hole cannot totally evaporate via quantum evaporation process proposed by Hawking. In a limiting case, an equilibrium of gravitation creation and black hole evaporation can be reached keeping the surface of its horizon constant. This conclusion is in accordance with the second law of thermodynamics.