Effective cosmological constant induced by stochastic fluctuations of Newton's constant
arXiv:1603.04170 · doi:10.1016/j.physletb.2016.07.015
Abstract
We consider implications of the microscopic dynamics of spacetime for the evolution of cosmological models. We argue that quantum geometry effects may lead to stochastic fluctuations of the gravitational constant, which is thus considered as a macroscopic effective dynamical quantity. Consistency with Riemannian geometry entails the presence of a time-dependent dark energy term in the modified field equations, which can be expressed in terms of the dynamical gravitational constant. We suggest that the late-time accelerated expansion of the Universe may be ascribed to quantum fluctuations in the geometry of spacetime rather than the vacuum energy from the matter sector.
10 pages, 1 figure, v2: added legend in Fig.1 and a reference
References in corpus (3)
Cited by in corpus (7)
- Fundamental Physics with the Square Kilometre Array
- Dimensional flow and fuzziness in quantum gravity: emergence of stochastic spacetime
- Quantum Gravity and Cosmology: an intimate interplay
- The role of noise in the early universe
- Constraining a stochastic variation of the gravitational coupling with binary systems
- Emergence of phantom cold dark matter from spacetime diffusion
- Critical Analysis of Replacing Dark Matter and Dark Energy with a Model of Stochastic Spacetime