S-Brane Thermodynamics
Alexander Maloney, Andrew Strominger, Xi Yin

TL;DR
This paper analyzes the thermodynamic properties of s-branes in string theory, revealing their thermal states, boundary conditions, and interactions with D-branes, with implications for understanding time-dependent backgrounds and black hole analogies.
Contribution
It provides an exact worldsheet CFT description of s-branes, constructs their boundary states, and computes their interactions and RR fields, highlighting novel thermal and boundary phenomena.
Findings
Open string pair production is thermal at temperature 1/4 pi.
At lambda=1/2, s-branes become arrays of sD-branes with half-unit s-charge.
The force between sD-branes and D-branes is 11/12 of the D-D force.
Abstract
The description of string-theoretic s-branes at g_s=0 as exact worldsheet CFTs with a (lambda cosh X^0) or (lambda e^(X^0)) boundary interaction is considered. Due to the imaginary-time periodicity of the interaction under X^0 -> X^0 + 2 pi i, these configurations have intriguing similarities to black hole or de Sitter geometries. For example, the open string pair production as seen by an Unruh detector is thermal at temperature T = 1/4 pi. It is shown that, despite the rapid time dependence of the s-brane, there exists an exactly thermal mixed state of open strings. The corresponding boundary state is constructed for both the bosonic and superstring cases. This state defines a long-distance Euclidean effective field theory whose light modes are confined to the s-brane. At the critical value of the coupling lambda=1/2, the boundary interaction simply generates an SU(2) rotation by pi…
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