Planckian discreteness and dark energy phenomenology
PIRSA ID:
19110051
Series:
Quantum Gravity
Event Type:
Seminar
Scientific Area(s):
Quantum Gravity
End date:
Speaker(s):
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.