Abstract

Classical rotating closed string are folded strings. At the folding points the scalar curvature associated with the induced metric diverges. As a consequence one cannot properly quantize the fluctuations around the classical solution since there is no complete set of normalizable eigenmodes. Furthermore in the non-critical effective string action of Polchinski and Strominger, there is a divergence associated with the folds. We overcome this obstacle by putting a massive particle at each folding point which can be used as a regulator. Using this method we compute the spectrum of quantum fluctuations around the rotating string and the intercept of the leading Regge trajectory. The results we find are that the intercepts are a = 1 and a = 2 for the open and closed string respectively, independent of the target space dimension. We argue that in generic theories with an effective string description, one can expect corrections from finite masses associated with either the endpoints of an open string or the folding points on a closed string. We compute explicitly the corrections in the presence of these masses.

Highlights

  • The quantization of strings in non-critical dimensions and in particular in four spacetime dimensions is an utmost important question for the description of nature in terms of a string theory

  • We argue that in generic theories with an effective string description, one can expect corrections from finite masses associated with either the endpoints of an open string or the folding points on a closed string

  • If we use the massive particle at every folding point as a regulator and take it to zero, we show that the intercept, including the contribution from the PS term, for rotating open strings takes the form

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Summary

Introduction

The quantization of strings in non-critical dimensions and in particular in four spacetime dimensions is an utmost important question for the description of nature in terms of a string theory. If we use the massive particle at every folding point as a regulator and take it to zero, we show that the intercept, including the contribution from the PS term, for rotating open strings takes the form. For both open and closed strings, the result in the massless limit is that the intercept is independent of the dimension, a result which generalizes what was found in [1] to the closed string.

Folded strings: generalities
Classical folded solutions of the string equations of motion
Rotating folded string solutions in flat spacetime
Rotating closed strings in flat spacetime
Rotating closed strings in two planes of rotation
Rotating open string solutions
Rotating open strings in magnetic fields
Rotating open string with massive endpoints
T L2 arcsin β 4
Rotating strings in magnetic field with massive endpoints
Rotating folded closed strings in holography
Rotating folded strings in AdS
Rotating folded strings in confining backgrounds
Folded non-rotating string solutions
Quantum fluctuations on strings with folds
Expanding around classical solutions Starting from the Nambu-Goto action
Expanding around rotating strings
The intercept
Expanding around rotating closed string
Closed string with massive folds
Classical rotating solution with massive folding points
Transverse fluctuations
Quantizing the folded open string
Classical solution with folding point mass
T L2 γf 4 arcsin βf γf βf2
Transverse modes
Planar mode
The intercept of non-critical rotating strings
Closed folded string
Closed string in two planes of rotation
Open string
Summary and open questions
Full Text
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