Table of Contents
Fetching ...

Entropy of Non-Extreme Charged Rotating Black Holes in String Theory

Mirjam Cvetic, Donam Youm

TL;DR

The paper provides explicit classical solutions for non-extreme rotating black holes in N=4 (or N=8) string vacua, detailing four-charge four-dimensional and three-charge five-dimensional configurations. It furnishes the Bekenstein-Hawking entropy in a form that naturally splits into left-moving and right-moving contributions, highlighting the role of angular momentum in the four-dimensional case and drawing parallels to D-brane microstate counting. By employing solution-generating techniques via boosts and leveraging duality symmetries, the authors connect these macroscopic entropies to potential microscopic interpretations on the D-brane world-volume. The work strengthens the link between rotating black holes in string theory and their D-brane descriptions, suggesting symmetric charge-decomposition structures and offering a framework for future microscopic entropy calculations. Overall, it advances understanding of how classical black hole thermodynamics in string theory aligns with D-brane microphysics and duality mappings.

Abstract

We give the explicit expression for four-dimensional rotating charged black hole solutions of N=4 (or N=8) superstring vacua, parameterized by the ADM mass, four charges (two electric and two magnetic charges, each arising from a different U(1) gauge factors), and the angular momentum (as well as the asymptotic values of four toroidal moduli of two-torus and the dilaton-axion field). The explicit form of the thermodynamic entropy is parameterized in a suggestive way as a sum of the product of the `left-moving' and the `right-moving' terms, which may have an interpretation in terms of the microscopic degrees of freedom of the corresponding D-brane configuration. We also give an analogous parameterization of the thermodynamic entropy for the recently obtained five-dimensional rotating charged black holes parameterized by the ADM mass, three U(1) charges and two rotational parameters (as well as the asymptotic values of one toroidal modulus and the dilaton).

Entropy of Non-Extreme Charged Rotating Black Holes in String Theory

TL;DR

The paper provides explicit classical solutions for non-extreme rotating black holes in N=4 (or N=8) string vacua, detailing four-charge four-dimensional and three-charge five-dimensional configurations. It furnishes the Bekenstein-Hawking entropy in a form that naturally splits into left-moving and right-moving contributions, highlighting the role of angular momentum in the four-dimensional case and drawing parallels to D-brane microstate counting. By employing solution-generating techniques via boosts and leveraging duality symmetries, the authors connect these macroscopic entropies to potential microscopic interpretations on the D-brane world-volume. The work strengthens the link between rotating black holes in string theory and their D-brane descriptions, suggesting symmetric charge-decomposition structures and offering a framework for future microscopic entropy calculations. Overall, it advances understanding of how classical black hole thermodynamics in string theory aligns with D-brane microphysics and duality mappings.

Abstract

We give the explicit expression for four-dimensional rotating charged black hole solutions of N=4 (or N=8) superstring vacua, parameterized by the ADM mass, four charges (two electric and two magnetic charges, each arising from a different U(1) gauge factors), and the angular momentum (as well as the asymptotic values of four toroidal moduli of two-torus and the dilaton-axion field). The explicit form of the thermodynamic entropy is parameterized in a suggestive way as a sum of the product of the `left-moving' and the `right-moving' terms, which may have an interpretation in terms of the microscopic degrees of freedom of the corresponding D-brane configuration. We also give an analogous parameterization of the thermodynamic entropy for the recently obtained five-dimensional rotating charged black holes parameterized by the ADM mass, three U(1) charges and two rotational parameters (as well as the asymptotic values of one toroidal modulus and the dilaton).

Paper Structure

This paper contains 7 sections, 23 equations.