The expansive nondecelerative universe - Gravitational effects and their manifestation in black holes evaporation and far-infrared spectra

TL;DR

This paper explores the Expansive Nondecelerative Universe model's implications for gravity, black hole evaporation, and infrared spectra, providing a unified framework for understanding gravitational energy distribution and its observable effects.

Contribution

It applies Vaidya metrics within the model to localize gravitational energy, linking macroscopic black hole evaporation with microscopic infrared spectral phenomena.

Findings

Gravitational energy can be localized using Vaidya metrics.

The model explains black hole evaporation through gravitational effects.

Infrared spectral properties are influenced by gravitational energy distribution.

Abstract

The paper summarizes the background of Expensive Nondecelerative Universe model and its main consequences for gravitation. Applying the Vaidya metrics, the model allows for the localization and determination of the density and quantity of gravitational energy created by a body with the mass m in the distance r. The consequences are manifested both in a macrosystem (Hawking's phenomenon of black holes evaporation) and microworld phenomenon (far-infrared spectral properties)