NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Cosmic background radiation anisotropy in an open inflation, cold dark matter cosmogonyWe compute the cosmic background radiation anisotropy, produced by energy-density fluctuations generated during an early epoch of inflation, in an open cosmological model based on the cold dark matter scenario. At Omega(sub 0) is approximately 0.3-0.4, the Cosmic Background Explorer (COBE) normalized open model appears to be consistent with most observations.
Document ID
19950043329
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Kamionkowski, Marc (School of Natural Science, Inst. for Advanced Study, Princeton, NJ United States)
Ratra, Bharat (Princeton Univ. Princeton, NJ, United States)
Spergel, David N. (Princeton Univ. Observatory, Princeton, NJ, United States)
Sugiyama, Naoshi (Univ. of California, Berkeley, CA United States)
Date Acquired
August 16, 2013
Publication Date
October 10, 1994
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters
Volume: 434
Issue: 1
ISSN: 0004-637X
Subject Category
ASTROPHYSICS
Funding Number(s)
CONTRACT_GRANT: NSF ASC-93-18135
CONTRACT_GRANT: NSF PHY-89-21378
CONTRACT_GRANT: NAGW-2448
CONTRACT_GRANT: DE-FG02-90ER-40542
CONTRACT_GRANT: NSF AST-88-58145
Distribution Limits
Public
Copyright
Other