Abstract

We compute semi-classical corrections to the energy of rotating open Nambu-Goto strings with and without masses at the ends, using methods from quantum field theory on curved space-times.

Highlights

  • For several reasons, the Nambu-Goto string is an interesting model: It exhibits diffeomorphism invariance, making it a toy model for gravity

  • The other approach to effective string theory in noncritical dimensions, related to Liouville theory, is defined by the Polchinski-Strominger (PS) action [10]. It is derived by fixing the parametrization to conformal gauge and introducing singular supplementary terms in order to preserve the conformal symmetry at the quantum level

  • (17), we find that the spectrum of Lq should be the integers, as expected for an angular momentum operator

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Summary

INTRODUCTION

The Nambu-Goto string is an interesting model: It exhibits diffeomorphism invariance, making it a toy model for (quantum) gravity. The other approach to effective string theory in noncritical dimensions, related to Liouville theory, is defined by the Polchinski-Strominger (PS) action [10] It is derived by fixing the parametrization to conformal gauge and introducing singular supplementary terms in order to preserve the conformal symmetry at the quantum level. This is quite different from our approach to effective string theory [9]: There, gauge conditions are only imposed on the fluctuations φ, the parametrization of the classical solution Xbeing arbitrary This corresponds to the standard treatment of Yang-Mills theories in background fields or of perturbative quantum gravity.. H 1⁄4 H0 þ OðR−1γ−12Þ; with H0 independent of R and γ.3 In our parametrization, the relation between the world-sheet Hamiltonian H, the quantum correction Eq to the target space energy E, and the quantum correction Lq1;2 to the angular momentum L1;2 is

R ðH þ
A MOTIVATING EXAMPLE
THE CLASSICAL ROTATING STRING
FLUCTUATIONS OF THE ROTATING STRING
THE WORLD-SHEET HAMILTONIAN AND THE TARGET SPACE ENERGY
RENORMALIZING THE WORLD-SHEET HAMILTONIAN
VIII. DEGENERACIES OF EXCITED STATES
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