Renormalization group approaches to Quantum Gravity and Tensions in Modern Cosmology
arXiv:2410.11970 · doi:10.22323/1.463.0186
Abstract
Asymptotic Safety is a promising framework towards the understanding, in a non-perturbative way, of Quantum Gravity. It treats the Newton's constant G_N and the cosmological constant Λas running coupling of an effective action. At the phenomenological point of view the values of G_N and Λdepend on the energy density of the system under consideration. This fact has interesting astrophysical and cosmological consequences. The present work discusses the effects on the distance measurements from SNIa light curves and on the strong and weak gravitational lensing measurements.
References in corpus (13)
- Exact evolution equation for the effective potential
- Singularity-free gravitational collapse and asymptotic safety
- A review on analytical studies in Gravitational Lensing
- A Safe Beginning for the Universe?
- Asymptotic Safety, Singularities, and Gravitational Collapse
- Inflation from Asymptotically Safe Theories
- Black Holes in Asymptotically Safe Gravity
- Using Host Galaxy Photometric Redshifts to Improve Cosmological Constraints with Type Ia Supernova in the LSST Era
- Effective field equations and scale-dependent couplings in gravity
- Swiss-cheese cosmologies with variable and from the renormalization group
- Safe essential scalar-tensor theories
- Constraining the swiss-cheese IR-fixed point cosmology with cosmic expansion
- Phenomenological footprints of Lambda varying gravity theories inspired from quantum gravity models in the multi-messenger era