4–6 May 2015
University of Pittsburgh
US/Eastern timezone

Holographic models with a small cosmological constant at Finite Temperature

4 May 2015, 17:45
15m
G26 (University of Pittsburgh)

G26

University of Pittsburgh

Pittsburgh, PA 15260
parallel talk Cosmology II

Speaker

Bithika Jain (Syracuse University)

Description

The cosmological constant problem can be reformulated in the brane world models. In this talk I will discuss a “soft-wall” realization of the Randall Sundrum geometry where the infrared brane plays a lesser role as a cutoff for large curvature effects and low energy observables such as spectrum of states are largely insensitive to its position. I will explore the finite temperature behavior of such models by studying geometries which include a horizon or a “black brane” along the extra dimension in the presence of non-trivial scalar field vacuum expectation value. A first order geometric phase transition proceeds via bubble nucleation between the two different gravity solutions. I shall then compare these results to the Randall Sundrum phase transition with Goldberger-Wise stabilization.

Author

Jay Hubisz (Syracuse University)

Co-authors

Bithika Jain (Syracuse University) Don Bunk (Hamilton College)

Presentation materials