pith. sign in

arxiv: hep-th/0412097 · v1 · pith:HNYPFKQInew · submitted 2004-12-09 · ✦ hep-th · astro-ph· gr-qc· hep-ph

The Holographic Approach to Cosmology

T. Banks , W. Fischler This is my paper
classification ✦ hep-th astro-phgr-qchep-ph
keywords holographicapproachcosmologyaccountaustinauthorschallengescompatible
0
0 comments X
read the original abstract

We review the successes and challenges of the holographic approach to cosmology. The model predicts an exactly scale invariant fluctuation spectrum with long and short distance cut-offs. It can account for the observed fluctuations in the CMB and might explain the low power at large scales. We outline various cosmological histories compatible with holographic initial conditions. This paper is based on talks given by the authors at Cosmo 04 in Toronto, and the 2004 Tamura Symposium in Austin

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Can Primordial Black Holes Be Seeds for Early Galaxies in Models Satisfying the Covariant Entropy Bound?

    hep-ph 2026-07 unverdicted novelty 3.0

    In CEB-obeying models, postulated distributions of primordial black holes decaying to radiation can fit CMB data, account for all dark matter, and seed the early galaxies detected by JWST, with some Planck-scale remna...