Implication of Classical Black Hole Evaporation Conjecture to Floating Black Holes

TL;DR

This paper explores the implications of the classical black hole evaporation conjecture within Randall-Sundrum models, proposing a phase diagram that suggests diverse black object families consistent with the conjecture.

Contribution

It introduces a new phase diagram scenario for black objects in extended Randall-Sundrum models, aligning with the classical black hole evaporation conjecture.

Findings

Proposes a phase diagram consistent with the evaporation conjecture.

Suggests a rich variety of black object families.

Supports the conjecture's implications in extended models.

Abstract

In Randall-Sundrum single-brane (RS-II) model, it was conjectured that there is no static large black hole localized on the brane based on adS/CFT correspondence. Here we consider the phase diagram of black objects in the models extended from the RS-II model. We propose a scenario for the phase diagram consistent with the classical black hole evaporation conjecture. The proposed scenario indicates the existence of a rich variety of the families of black objects.