Bottom-up holographic models for cosmology
Abstract
In this note, we investigate some simple generalizations of a bottom-up holographic approach to cosmology introduced in arXiv:1810.10601. Our models utilize the Karch/Randall/Takayanagi ansatz for the gravitational dual of a boundary conformal field theory, involving pure AdS gravity and an end-of-the-world brane. Following a suggestion made in arXiv:2102.05057, we consider models with an additional interface brane in the bulk. We find that solutions with a viable cosmological interpretation exist only if our model is further generalized, for example by including an Einstein-Hilbert term in the ETW brane action. The physical validity of such models is discussed from the perspective of the effective theory.
Cite
@article{arxiv.2203.03096,
title = {Bottom-up holographic models for cosmology},
author = {Chris Waddell},
journal= {arXiv preprint arXiv:2203.03096},
year = {2022}
}
Comments
Minor typos corrected in Section 3, and Appendices A and C