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Characteristic microwave-background distortions from collapsing spherical domain wallsThe redshift distortion induced by collapsing spherical domain walls is calculated. The most frequent microwave background distortions are found to occur at large angles in the form of blue disks. This is the angular region currently measured by the COBE satellite. COBE could therefore detect signals predicted here for domain walls with surface energy density of the order of MeV. Such values for sigma are proposed in the late-time phase-transition scenario of Hill et al. (1989).
Document ID
19910027720
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Goetz, Guenter
(Chicago Univ. Chicago, IL, United States)
Notzold, Dirk
(Chicago, University; NASA/Fermilab Astrophysics Center Batavia, IL, United States)
Date Acquired
August 14, 2013
Publication Date
October 29, 1990
Publication Information
Publication: Physical Review Letters
Volume: 65
ISSN: 0031-9007
Subject Category
Astrophysics
Accession Number
91A12343
Funding Number(s)
CONTRACT_GRANT: NAGW-1340
CONTRACT_GRANT: NAGW-1321
CONTRACT_GRANT: NSF AST-88-22595
Distribution Limits
Public
Copyright
Other

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