One-loop quantum cosmological correction to the gravitational constant in the closed Friedmann-Robertson-Walker universe
arXiv:1010.0823 · doi:10.1142/S0217751X10050275
Abstract
In this paper, we calculate the one-loop quantum cosmological corrections to the kink energy in the closed Friedmann-Robertson-Walker universe in which the fluctuation potential has a shape invariance property. We use the generalized zeta function regularization method to implement our setup for describing quantum kink-like states. It is conjectured that the corrections lead to the renormalized gravitational constant.
References in corpus (13)
- Supersymmetry and Quantum Mechanics
- Topological boundary conditions, the BPS bound, and elimination of ambiguities in the quantum mass of solitons
- Energy, Central Charge, and the BPS Bound for 1+1 Dimensional Supersymmetric Solitons
- Heat kernels and zeta-function regularization for the mass of the supersymmetric kink
- Cosmological properties of a class of decaying cosmologies
- Unambiguous one-loop quantum energies of 1+1 dimensional bosonic field configurations
- One-loop surface tensions of (supersymmetric) kink domain walls from dimensional regularization
- Generalized Zeta Functions and One-loop Corrections to Quantum Kink Masses
- Fermionic One-Loop Corrections to Soliton Energies in 1+1 Dimensions
- Mode regularization of the susy sphaleron and kink: zero modes and discrete gauge symmetry
- Derivative Expansion and Soliton Masses
- Tunneling in Decaying Cosmologies and the Cosmological Constant Problem
- On Duru-Kleinert Path Integral In Quantum Cosmology