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Light domain walls, massive neutrinos and the large scale structure of the UniverseDomain walls generated through a cosmological phase transition are considered, which interact nongravitationally with light neutrinos. At a redshift z greater than or equal to 10(exp 4), the network grows rapidly and is virtually decoupled from the matter. As the friction with the matter becomes dominant, a comoving network scale close to that of the comoving horizon scale at z of approximately 10(exp 4) gets frozen. During the later phases, the walls produce matter wakes of a thickness d of approximately 10h(exp -1)Mpc, that may become seeds for the formation of the large scale structure observed in the Universe.
Document ID
19910015553
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Massarotti, Alessandro
(Chicago Univ. IL., United States)
Date Acquired
September 6, 2013
Publication Date
April 1, 1991
Subject Category
Atomic And Molecular Physics
Report/Patent Number
NASA-CR-188446
FERMILAB-PUB-91/104-A
NAS 1.26:188446
Report Number: NASA-CR-188446
Report Number: FERMILAB-PUB-91/104-A
Report Number: NAS 1.26:188446
Accession Number
91N24867
Funding Number(s)
CONTRACT_GRANT: NAGW-1340
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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