Mabuchi spectrum from the minisuperspace
arXiv:1511.06150 · doi:10.1016/j.physletb.2016.05.013
Abstract
It was recently shown that other functionals contribute to the effective action for the Liouville field when considering massive matter coupled to two-dimensional gravity in the conformal gauge. The most important of these new contributions corresponds to the Mabuchi functional. We propose a minisuperspace action that reproduces the main features of the Mabuchi action in order to describe the dynamics of the zero-mode. We show that the associated Hamiltonian coincides with the (quantum mechanical) Liouville Hamiltonian. As a consequence the Liouville theory and our model of the Mabuchi theory both share the same spectrum, eigenfunctions and - in this approximation - correlation functions.
arXiv comment4 pages; v2: change presentation but conclusion unchanged, match published version
References in corpus (12)
- Liouville theory revisited
- Liouville Field Theory -- A decade after the revolution
- Rolling Tachyons from Liouville theory
- Fractional Quantum Hall Effect in a Curved Space: Gravitational Anomaly and Electromagnetic Response
- Geometry of Quantum Hall States: Gravitational Anomaly and Kinetic Coefficients
- FQHE on curved backgrounds, free fields and large N
- Conformal field theory on the plane
- Notes on Liouville Theory at c<=1
- Gravitational Actions in Two Dimensions and the Mabuchi Functional
- Scaling Lee-Yang Model on a Sphere. I. Partition Function
- Random Geometry, Quantum Gravity and the Kähler Potential
- 2D Quantum Gravity at One Loop with Liouville and Mabuchi Actions
Cited by in corpus (6)
- 2D gravitational Mabuchi action on Riemann surfaces with boundaries
- BRST cohomology of timelike Liouville theory
- Minisuperspace computation of the Mabuchi spectrum
- Integrable higher-dimensional cosmology with separable variables in an Einstein-dilaton-antisymmetric field theory
- Gravitational action for a massive Majorana fermion in 2d quantum gravity
- A short note on dynamics and degrees of freedom in classical gravity