Early Evolution of the Universe and its Present Structure (Paperback, Softcover reprint of the original 1st ed. 1983)

Since the last International Astronomical Union Symposium that dealt with matters cosmological, there have been dramatic advances, both on the observational and theoretical fronts. Modern high-efficiency detectors have made possible extensive magnitude-limited redshift surveys, which have permitted observational cosmologists to construct three-dimensional maps of large regions of space. What seems to emerge is a distribution of matter in extensive, flat, but probably filamentary, and possibly interconnected, superclusters, serving as interstices between vast voids in space. Meanwhile, theoretical ideas that were highly speculative a few years ago have begun to be taken seriously as possibly describing conditions in the very early universe. And brand new ideas, such as that of the inflationary universe, hold promise of solving outstanding observational, theoretical, and philosophical problems in cosmology. A new look at grand unified theories and concepts of supersymmetry have brought observational and theoretical cosmologists to a common meeting ground with modern particle physicists.

General

Imprint:	Kluwer Academic Publishers
Country of origin:	Netherlands
Series:	International Astronomical Union Symposia, 104
Release date:	September 1983
First published:	1983
Editors:	G.O. Abell • G. Chincarini
Dimensions:	244 x 170 x 29mm (L x W x T)
Format:	Paperback
Pages:	564
Edition:	Softcover reprint of the original 1st ed. 1983
ISBN-13:	978-90-277-1662-0
Categories:	Books > Science & Mathematics > Astronomy, space & time > Cosmology & the universe Promotions
LSN:	90-277-1662-5
Barcode:	9789027716620

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