Emergence of phantom cold dark matter from spacetime diffusion

22 Oct 2024
Seminars and colloquia
Time
-
Venue
Beecroft Seminar Room
Denys Wilkinson Building, Department of Physics, University of Oxford, Keble Road, Oxford OX1 3RH
Speaker(s)

Emanuele Panella, University College London

Seminar series
Cosmology
For more information contact

Abstract

A way to reconcile general relativity and quantum field theory without quantizing the geometry is requiring that the metric evolves stochastically. In this talk, I will first review the main ideas and motivations around hybrid theories that handle the interaction between classical and quantum degrees of freedom in a consistent manner. In the second half of the talk, I will describe how spacetime diffusion can produce experimentally falsifiable predictions. In particular, I will describe how the stochastic evolution results in the spatial metric diffusing away from its deterministic value, generating phantom dark matter that has the potential to reproduce CDM phenomenology.