String Quantization in Curved Spacetimes: Null String Approach
arXiv:hep-th/9412081 · doi:10.1142/S0217732395002611
Abstract
We study quantum strings in strong gravitational fields. The relevant small parameter is , where is the curvature of the spacetime and is the string tension. Within our systematic expansion we obtain to zeroth order the null string (string with zero tension), while the first order correction incorporates the string dynamics. We apply our formalism to quantum null strings in de Sitter spacetime. After a reparametrization of the world-sheet coordinates, the equations of motion are simplified. The quantum algebra generated by the constraints is considered, ordering the momentum operators to the right of the coordinate operators. No critical dimension appears. It is anticipated however that the conformal anomaly will appear when the first order corrections proportional to , are introduced.
6 pages, plain Tex, no figures
Cited by in corpus (17)
- M Theory Model of a Big Crunch/Big Bang Transition
- An action variable of the sine-Gordon model
- On the tensionless limit of gauged WZW models
- String dynamics in cosmological and black hole backgrounds: The null string expansion
- Null Strings in Schwarzschild Spacetime
- Quantum gravity as a Fermi liquid
- Exact String Solutions in Nontrivial Backgrounds
- Anomalous dimension and local charges
- Strings in Homogeneous Background Spacetimes
- Tensionless String in the Notoph Background
- Null Strings in Kerr Spacetime
- Worldsheet Instantons and a Null String Limit of Born-Infeld Theory
- String Propagation in Bianchi Type I models: Dynamical anisotropy Damping and Consequences
- String Tension and the Generation of the Conformal Anomaly
- Analytical results for string propagation near a Kaluza-Klein black hole
- Null Strings Gauged and Reloaded, I: Null Strings Have Carroll-Weyl Gauge Symmetry
- String dynamics near a Kaluza-Klein black hole