Rankings
Publications
Search Publications
Cited-by Search
Sources
Publishers
Scholars
Scholars
Top Cited Scholars
Organizations
About
Scilit
About Us
Advisory Board
Data Sources
Career
Support / Contact
User Guide
Publisher User
Search Function
Rankings Function
API Resource
Scilit Knowledge
Metrics
Scilit Recognitions
Publications Classification
Media
News
Blog
Login
Register
Home
Publications
The failure of cosmological perturbation theory in the new ekpyrotic scenario
Home
Publications
The failure of cosmological perturbation theory in the new ekpyrotic scenario
The failure of cosmological perturbation theory in the new ekpyrotic scenario
Author:
DL
D H Lyth
D H Lyth
Article Alert
Citation Alert
Add to Library
Cite
Download
Share
Download
Download PDF
Download
Preprint
Publisher website
Google Scholar
29 September 2001
preprint
Published by
arXiv
in
arXiv
DOI:
https://doi.org/10.48550/arXiv.hep-ph/0110007
Abstract
Cosmological perturbation theory fails in the new ekpyrotic scenario before the scale factor of the Universe reaches zero. As a result, the scenario does not provide a mechanism for generating the observed curvature perturbation at the bounce.
Keywords
COSMOLOGICAL PERTURBATION THEORY
PERTURBATION THEORY
EKPYROTIC SCENARIO
NEW EKPYROTIC
SCENARIO
THEORY
All Related Versions
Version 1, 2001-09-29, ArXiv
Version 2, 2001-12-11, ArXiv
Version 3, 2001-12-19, ArXiv
Version 4, 2002-01-08, ArXiv
Published version:
Physics Letters B, 526 (3-4), 173.
Related articles
Scroll to top