Video URL
https://pirsa.org/19110051Planckian discreteness and dark energy phenomenology
APA
Perez, A. (2019). Planckian discreteness and dark energy phenomenology. Perimeter Institute for Theoretical Physics. https://pirsa.org/19110051
MLA
Perez, Alejandro. Planckian discreteness and dark energy phenomenology. Perimeter Institute for Theoretical Physics, Nov. 13, 2019, https://pirsa.org/19110051
BibTex
@misc{ scivideos_PIRSA:19110051, doi = {10.48660/19110051}, url = {https://pirsa.org/19110051}, author = {Perez, Alejandro}, keywords = {Quantum Gravity}, language = {en}, title = {Planckian discreteness and dark energy phenomenology}, publisher = {Perimeter Institute for Theoretical Physics}, year = {2019}, month = {nov}, note = {PIRSA:19110051 see, \url{https://scivideos.org/pirsa/19110051}} }
Alejandro Perez Aix-Marseille University
Abstract
I will explain how dark energy in cosmology could arise from the
noisy diffusion of energy from the low energy degrees of freedom of matter (described in terms of QFT)
to the fundamental Planckian granularity (expected from quantum gravity). This
perspective leads to a natural model resolving the fine tuning problem associated to the small
value of the cosmological constant. However, recent observations suggest that the dark energy
component in our universe might not be constant and should instead have grown from the recombination time to the present.
I will present new ideas suggesting a possible explanation within the same framework.