String theory in polar coordinates and the vanishing of the one-loop Rindler entropy

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作者
Thomas G. Mertens
Henri Verschelde
Valentin I. Zakharov
机构
[1] Princeton University,Joseph Henry Laboratories
[2] Ghent University,School of Biomedicine
[3] Department of Physics and Astronomy,undefined
[4] ITEP,undefined
[5] Moscow Inst Phys & Technol,undefined
[6] Far Eastern Federal University,undefined
关键词
Black Holes in String Theory; Conformal Field Models in String Theory; Tachyon Condensation;
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摘要
We analyze the string spectrum of flat space in polar coordinates, following the small curvature limit of the SL2ℝ/U1\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$ \mathrm{S}\mathrm{L}\left(2,\mathbb{R}\right)/\mathrm{U}(1) $$\end{document} cigar CFT. We first analyze the partition function of the cigar itself, making some clarifications of the structure of the spectrum that have escaped attention up to this point. The superstring spectrum (type 0 and type II) is shown to exhibit an involution symmetry, that survives the small curvature limit. We classify all marginal states in polar coordinates for type II superstrings, with emphasis on their links and their superconformal structure. This classification is confirmed by an explicit large τ2 analysis of the partition function. Next we compare three approaches towards the type II genus one entropy in Rindler space: using a sum-over-fields strategy, using a Melvin model approach as in [1] and finally using a saddle point method on the cigar partition function. In each case we highlight possible obstructions and motivate that the correct procedures yield a vanishing result: S = 0. We finally discuss how the QFT UV divergences of the fields in the spectrum disappear when computing the free energy and entropy using Euclidean techniques.
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