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Massive neutrinos and the pancake theory of galaxy formationThree problems encountered by the pancake theory of galaxy formation in a massive neutrino-dominated universe are discussed. A nonlinear model for pancakes is shown to reconcile the data with the predicted coherence length and velocity field, and minimal predictions are given of the contribution from the large-scale matter distribution.
Document ID
19840053569
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/184274
Authors
Schaeffer, R. (Commissariat al'Energie Atomique, Service de Physique Theoretique, Gif-sur-Yvette Essonne, France)
Silk, J. (California, University Berkeley, CA, United States)
Date Acquired
August 12, 2013
Publication Date
June 1, 1984
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters to the Editor
Volume: 281
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
84A36356
Funding Number(s)
CONTRACT_GRANT: NGR-05-003-578
CONTRACT_GRANT: DE-AT03-82ER-60069
Distribution Limits
Public
Copyright
Other

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