Semiclassical geometrodynamics of homogeneous cosmology
Abstract
We study the classical-quantum (CQ) hybrid dynamics of homogeneous cosmology from a Hamiltonian perspective where the classical gravitational phase space variables and matter state evolve self-consistently with full backreaction. We compare numerically the classical and CQ dynamics for isotropic and anisotropic models, including quantum scalar-field induced corrections to the Kasner exponents. Our results indicate that full backreaction effects leave traces at late times in cosmological evolution; in particular, the scalar energy density at late times provides a potential contribution to dark energy. We also show that the CQ equations admit exact static solutions for the isotropic, and the anisotropic Bianchi IX universes with the scalar field in a stationary state.
Keywords
Cite
@article{arxiv.2210.07458,
title = {Semiclassical geometrodynamics of homogeneous cosmology},
author = {Viqar Husain and Muhammad Muzammil},
journal= {arXiv preprint arXiv:2210.07458},
year = {2024}
}
Comments
13 pages, 5 figures; substantially extended, title changed, version to appear in Phys Rev D