pith. sign in

arxiv: hep-ph/0102183 · v1 · pith:HCA3DS3Pnew · submitted 2001-02-15 · ✦ hep-ph · astro-ph· cond-mat.str-el· gr-qc· hep-th

Frontiers of Inflationary Cosmology

classification ✦ hep-ph astro-phcond-mat.str-elgr-qchep-th
keywords cosmologicalcosmologyinflationaryproblemsreviewsomeamplificationanderson
0
0 comments X
read the original abstract

After a brief review of the theory of cosmological perturbations, I highlight some recent progress in the area of reheating in inflationary cosmology, focusing in particular on parametric amplification of super-Hubble cosmological fluctuations, and on the role of noise in the resonance dynamics (yielding a new proof of Anderson localization). I then discuss several important conceptual problems for the current realizations of inflation based on fundamental scalar matter fields, and review some new approaches at solving these problems.

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.