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.
Is the universe matter dominated or energy dominated? The very early universe was "energy dominated" in the sense that only a small fraction of the energy of the universe at that time was in the form of the rest energy of matter and antimatter. Much of the energy of the universe was in the form of electromagnetic radiation. It is not known whether the universe originally had an excess of matter over antimatter or whether the excess of matter developed as time went on. Most cosmologists favor the idea that reactions in the early universe led to the excess of matter, but the mechanism is not known. As the universe expanded it cooled, until, about 300,000 years after the Big Bang, the quanta of radiation (photons) no longer had enough energy to create electrons and positrons. As the universe continued to expand, the radiation cooled still further, until today all that is left of it is the microwave background radiation at a temperature of 2.7 K. The amount of energy in the background radiation plus all the light energy from stars is only a tiny fraction of the rest energy of matter. Therefore, today, the visible universe appears to be matter dominated. However, it is an open question whether other, as yet unseen, forms of energy exist that would make the universe energy dominated.