The Cosmology of Nothing
Abstract
For more seventy years physicists have appreciated that Nature's vacuum is far from empty. The discovery of the Lamb shift in Hydrogen provided dramatic verification of the reality of the quantum vacuum. The advent of gauge theories has led us to believe that the physics of the vacuum is even richer, with the possibility of instantons, vacuum phase transitions, vacuum defects (monopoles, domain walls, cosmic strings and nontopological solitons), vacuum energy, and degenerate vacua states (with different local realizations of the laws of physics). Cosmology offers a unique laboratory for exploring the ``physics of nothing.'' In this lecture I focus on the implications of vacuum energy for cosmology -- in particular, inflation -- and discuss the flood of observations that are testing the inflationary paradigm and in process probing the physics of nothing. I also discuss the possibility that today vacuum energy plays a dynamically important role (as a cosmological constant).
Cite
@article{arxiv.astro-ph/9703195,
title = {The Cosmology of Nothing},
author = {Michael S. Turner},
journal= {arXiv preprint arXiv:astro-ph/9703195},
year = {2007}
}
Comments
32 pages LaTeX (sprocl.sty) with 8 eps figures. Published in Vacuum and Vacua: The Physics of Nothing, edited A. Zichichi (World Scientific, 1996), p. 50