A field theory approach to cosmological density perturbations
classification
🌀 gr-qc
keywords
perturbationsadiabaticapproachcosmologicaldensityeffectiveexpandingfield
read the original abstract
Adiabatic perturbations propagate in the expanding universe like scalar massless fields in some effective Robertson-Walker space-time.
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.