Lectures on the Microscopic Modeling of the 5-dim. Black Hole of IIB String Theory and the $D_1-D_5$ System
Spenta R. Wadia

TL;DR
This paper reviews the microscopic modeling of the five-dimensional black hole in type IIB string theory using the D1-D5 brane system, focusing on brane dynamics and their thermodynamic properties.
Contribution
It provides a detailed discussion of low energy brane dynamics and their role in black hole thermodynamics, emphasizing non-renormalization in the supergravity regime.
Findings
Derivation of black hole entropy from brane microstates
Calculation of Hawking radiation rates from brane dynamics
Validation of supergravity regime applicability
Abstract
In these notes we review the theory of the microscopic modeling of the 5-dim. black hole of type IIB string theory in terms of the brane system. The emphasis here is more on the brane dynamics rather than on supergravity solutions. We present a discussion of the low energy brane dynamics and account for black hole thermodynamics and Hawking radiation rates. These considerations are valid in the regime of supergravity due to the non-renormalization of the low energy dynamics in this model.
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