Inflationary Cosmology
Abstract
Inflation is a bold and expansive extension of the Standard Cosmology. It holds the promise to extend our understanding of the Universe to within 10^{-32}sec of the big bang and answer most of the pressing questions in cosmology. Its boldest assertion is that all the structure observed in the Universe today arose from quantum-mechanical fluctuations on subatomic scales. A flood of cosmological observations and laboratory experiments are testing inflation and within five years we should know whether inflation is to become part of a new standard cosmology.
Cite
@article{arxiv.astro-ph/9704040,
title = {Inflationary Cosmology},
author = {Michael S. Turner},
journal= {arXiv preprint arXiv:astro-ph/9704040},
year = {2007}
}
Comments
25 pages LaTeX (cupconf.sty) with eps figures. To be published in Relativistic Astrophysics: A Conference in Honour of Igor Novikov's 60th Birthday (Cambridge University Press, Cambridge, 1997)