Quantum String Dynamics in the conformal invariant SL(2,R) WZWN Background: Anti-de Sitter Space with Torsion

TL;DR

This paper investigates classical and quantum string dynamics in a conformally invariant SL(2,R) WZWN background with torsion, revealing how conformal invariance influences string interactions, mass spectrum, and thermodynamics compared to non-conformal AdS spacetime.

Contribution

It provides a detailed analysis of string behavior in a conformally invariant background, highlighting the effects on the mass spectrum, entropy, and absence of Hagedorn temperature, with comparisons to non-conformal AdS.

Findings

High-mass string states follow m ~ HN for large N.

Level spacing grows proportionally with N, d(m^2 alpha')/dN ~ N.

No Hagedorn temperature; partition function is well-defined at all positive temperatures.

Abstract

We consider classical and quantum strings in the conformally invariant background corresponding to the SL(2,R) WZWN model. This background is locally anti-de Sitter spacetime with non-vanishing torsion. Conformal invariance is expressed as the torsion being parallelized. The precise effect of the conformal invariance on the dynamics of both circular and generic classical strings is extracted. In particular, the conformal invariance gives rise to a repulsive interaction of the string with the background which precisely cancels the dominant attractive term arising from gravity. We perform both semi-classical and canonical string-quantization, in order to see the effect of the conformal invariance of the background on the string mass spectrum. Both approaches yield that the high-mass states are governed by m sim HN (N,`large integer'), where m is the string mass and H is the Hubble constant. It follows that the level spacing grows proportionally to N: d(m^2 alpha')/dN sim N, while the entropy goes like: S sim sqrt{m}. Moreover, it follows that there is no Hagedorn temperature,so that the partition function is well defined at any positive temperature. All results are compared with the analogue results in Anti- de Sitter spacetime, which is a non conformal invariant background. Conformal invariance simplifies the mathematics of the problem but the physics remains mainly unchanged. Differences between conformal and non-conformal backgrounds only appear in the intermediate region of the string spectrum, but these differences are minor. For low and high masses, the string mass spectra in conformal and non-conformal backgrounds are identical. Interestingly enough, conformal invariance fixes the value of the spacetime curvature to be -69/(26 alpha').