Speaker
Bharath Sambasivam
Description
We consider dynamical fully 5-Dimensional cosmological solutions of the holographic dilaton to study an out-of-equilibrium alternative to the thermal Randall-Sundrum conformal phase transition. It is well known that this transition is typically strongly first order, with the requirement of a perturbative 5D gravity theory obstructing completion of the transition. We comment on a class of initial conditions that generically leads to completion of the phase transition with increased perturbative control of the 5D theory associated with higher likelihood of success.
Authors
Bharath Sambasivam
Cem Eröncel
(Syracuse University)
Gabriele Rigo
(IPhT, Saclay)
Jay Hubisz
(Syracuse University)
Seung J. Lee
(Korea University)
