The following sections of this BookRags Literature Study Guide is offprint from Gale's For Students Series: Presenting Analysis, Context, and Criticism on Commonly Studied Works: Introduction, Author Biography, Plot Summary, Characters, Themes, Style, Historical Context, Critical Overview, Criticism and Critical Essays, Media Adaptations, Topics for Further Study, Compare & Contrast, What Do I Read Next?, For Further Study, and Sources.
(c)1998-2002; (c)2002 by Gale. Gale is an imprint of The Gale Group, Inc., a division of Thomson Learning, Inc. Gale and Design and Thomson Learning are trademarks used herein under license.
The following sections, if they exist, are offprint from Beacham's Encyclopedia of Popular Fiction: "Social Concerns", "Thematic Overview", "Techniques", "Literary Precedents", "Key Questions", "Related Titles", "Adaptations", "Related Web Sites". (c)1994-2005, by Walton Beacham.
The following sections, if they exist, are offprint from Beacham's Guide to Literature for Young Adults: "About the Author", "Overview", "Setting", "Literary Qualities", "Social Sensitivity", "Topics for Discussion", "Ideas for Reports and Papers". (c)1994-2005, by Walton Beacham.
All other sections in this Literature Study Guide are owned and copyrighted by BookRags, Inc.
Flat universe is the term used to describe a universe that is expanding and will continue to expand forever, albeit at a rate that will eventually approach zero. The solution of Einstein's general relativistic equations for the entire universe predicts one of three possibilities: the universe can start out expanding, but eventually stop expanding and begin to contract; it can be flat; or it can expand forever at an ever-increasing rate. The case of a flat universe is special, because unless the universe is very close to being flat, its lifetime is calculated to be much shorter than the observed age of the universe.
There is a critical energy density required for the universe to be flat; the ratio of the actual energy density to the critical density is a parameter called Omega (). For a flat universe, is exactly one. Until recently, it was believed that the universe was flat, but recent evidence shows that the universal expansion may actually be accelerating, leading us to believe that the universe is not completely flat.