Dark Information in Black Hole with $\lambda\varphi$ Fluid

TL;DR

This paper explores how a $bb ext{-}b1\

Contribution

It introduces a new black hole solution in a $bb ext{-}b1\

Findings

The $bb ext{-}b1\

The radiation spectrum is nonthermal and differs significantly at the last stage due to the $bb ext{-}b1\

Dark information increases despite reduced black hole lifetime

Abstract

It has been shown that the nonthermal spectrum of Hawking radiation will lead to information-carrying correlations between emitted particles in the radiation. The mutual information carried by such correlations can not be locally observed and hence is dark. With dark information, the black hole information is conserved. In this paper, we look for the spherically symmetric black hole solution in a $\lambda\varphi$ fluid model and investigate the radiation spectrum and dark information of the black hole. The spacetime structure of this black hole is similar to that of the Schwarzschild one, while its horizon radius is decreased by the $\lambda\varphi$ fluid. By using the statistical mechanical method, the nonthermal radiation spectrum is calculated. This radiation spectrum is very different from the Schwarzschild case at its last stage because of the effect of the $\lambda\varphi$ fluid. The $\lambda\varphi$ fluid reduces the lifetime of the black hole, but increases the dark information of the Hawking radiation.