Black Holes with Intrinsic Spin

Abstract

We analyze the general black hole solutions to the four dimensional STU model recently constructed by Chow and Compere. We define a dilute gas limit where the black holes can be interpreted as excited states of an extremal ground state. In this limit we express the black hole entropy and the excitation energy in terms of physical quantities with no need for parametric charges. We discuss a dual microscopic CFT description that incorporates all electric and magnetic charges. This description is recovered geometrically by identification of a near horizon BTZ region. We construct the subtracted geometry with no restrictions on charges by analyzing the scalar wave equation in the full geometry. We determine the matter sources that support the subtracted geometry by studying a scaling limit and show that the general geometry permits a dilute gas description with parameters that we specify.

36 pg, harvmac

References in corpus (4)

• Lectures on Quantum Black Holes
• Subtracted Geometry From Harrison Transformations
• On The Stability of Non-Supersymmetric Attractors in String Theory
• Attraction, with Boundaries

Cited by in corpus (6)

• AdS${}_2$ Holographic Dictionary
• Vacuum Polarization of STU Black Holes and their Subtracted Geometry Limit
• An Analysis of the Wave Equation for the $U(1{)}^2$ Gauged Supergravity Black Hole
• Thermodynamics of Asymptotically Conical Geometries
• Wave Equation for the Wu Black Hole
• Entanglement entropy of subtracted geometry black holes