Loop quantum modified gravity and its cosmological application
arXiv:1211.5024 · doi:10.1007/s11467-013-0277-0
Abstract
A general nonperturvative loop quantization procedure for metric modified gravity is reviewed. As an example, this procedure is applied to scalar-tensor theories of gravity. The quantum kinematical framework of these theories is rigorously constructed. Both the Hamiltonian and master constraint operators are well defined and proposed to represent quantum dynamics of scalar-tensor theories. As an application to models, we set up the basic structure of loop quantum Brans-Dicke cosmology. The effective dynamical equations of loop quantum Brans-Dicke cosmology are also obtained, which lay a foundation for the phenomenological investigation to possible quantum gravity effects in cosmology.
18pages. arXiv admin note: substantial text overlap with arXiv:1107.5157
References in corpus (15)
- Quantum Gravity at a Lifshitz Point
- Dark Energy and the Accelerating Universe
- Quantum Nature of the Big Bang: Improved dynamics
- Corrections to the Friedmann Equations from LQG for a Universe with a Free Scalar Field
- Critical Gravity in Four Dimensions
- Loop Quantum Cosmology: An Overview
- Hamiltonian Formulation of Palatini f(R) theories a la Brans-Dicke
- Extension of loop quantum gravity to theories
- Path Integrals and the WKB approximation in Loop Quantum Cosmology
- New length operator for loop quantum gravity
- Effective Scenario of Loop Quantum Cosmology
- Loop quantum Brans-Dicke cosmology
- Exact cosmological solution of a Scalar-Tensor Gravity theory compatible with the model
- Brans-Dicke Scalar Field as a Unique k-essence
- Coherent State Functional Integral in Loop Quantum Cosmology: Alternative Dynamics