Static configurations and evolution of higher dimensional brane-dilaton black hole system

TL;DR

This paper investigates static and dynamic behaviors of higher-dimensional dilaton black holes interacting with branes, revealing how dimensionality and extremality influence brane configurations and black hole expulsion.

Contribution

It provides new insights into the static configurations and evolution of higher-dimensional dilaton black hole-brane systems across different coupling constants and extremality conditions.

Findings

Nonextremal black holes have two static brane configurations.

Brane expulsion from black holes occurs faster in higher dimensions.

Extremal black holes always expel the brane regardless of parameters.

Abstract

Static configurations and a dynamical evolution of the system composed of a higher-dimensional spherically symmetric dilaton black hole and the Dirac-Goto-Nambu brane were investigated. The studies were conducted for three values of the dilaton coupling constant, describing the uncoupled case, the low-energy limit of the string theory and dimensionally reduced Klein-Kaluza theories. When the black hole is nonextremal, two types of static configurations are observed, a brane which intersects the black hole horizon and a brane not having any common points with the accompanying black hole. As the number of spacetime dimensions increases, the brane bend in the vicinity of the black hole disappears closer to its horizon. Dynamical evolution of the system results in an expulsion of the black hole from the brane. It proceeds faster for bigger values of the bulk spacetime dimension and thicker branes. The value of the dilatonic coupling constant does not influence neither the static configurations nor the dynamical behavior of the examined nonextremal system. In the extremal dilaton black hole case one obtains expulsion of the brane which is independent on the spacetime dimensionality and the value of the coupling constant. Dynamical studies of the configurations in the extremal case reveal that the course of evolution of the system is similar to the nonextremal one, except for a slightly earlier expulsion of the black hole from the brane.