Starting from a non standard approach to the Unruh effect, we present a description of the emission of radiation from a black hole that avoids quantization of scalar fields and Bogoliubov transformations, but assumes the existence of a maximal acceleration. In this framework the description appears closer to the original heuristic Hawking's point of view, with respect to the standard scenario.
From the particle pair production to the Hawking - Unruh radiation in the maximal acceleration hypothesis
Antonio Feoli
2019-01-01
Abstract
Starting from a non standard approach to the Unruh effect, we present a description of the emission of radiation from a black hole that avoids quantization of scalar fields and Bogoliubov transformations, but assumes the existence of a maximal acceleration. In this framework the description appears closer to the original heuristic Hawking's point of view, with respect to the standard scenario.File in questo prodotto:
Non ci sono file associati a questo prodotto.
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
