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The three-point function in an ensemble of numerical simulationsThe three-point function in Fourier space is evaluated for an ensemble of 2D numerical simulations with nine initial power spectra distinguished by spectral index and cutoff. To remove the main dependences on scale and time, results are presented as the reduced amplitude Q in the hierarchical model. To lowest nonvanishing order in perturbation theory, Q is a constant, independent of length scale, of time, and of initial spectrum. The results show that in the nonlinear regime of evolution, normalizing to Q does remove the main variations, but systematic dependences on spectral index and cutoff remain at late times that depend on properties of the initial spectrum. Models with initial power cut off on a scale that has been evolved far into the nonlinear regime are indistinguishable from models with no cutoff.
Document ID
19920063028
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Fry, J. N.
(Florida, University Gainesville, United States)
Melott, Adrian L.
(NASA Headquarters Washington, DC United States)
Shandarin, Sergei F.
(Kansas, University Lawrence, United States)
Date Acquired
August 15, 2013
Publication Date
July 10, 1992
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 393
Issue: 2 Ju
ISSN: 0004-637X
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-637X
Accession Number
92A45652
Funding Number(s)
CONTRACT_GRANT: NSF AST-89-11327
CONTRACT_GRANT: NAGW-1793
CONTRACT_GRANT: NAGW-1288
Distribution Limits
Public
Copyright
Other

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