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Interpretation of large-scale deviations from the Hubble flow

Grinstein, B. and Politzer, H. David and Rey, S.-J. and Wise, Mark B. (1987) Interpretation of large-scale deviations from the Hubble flow. Astrophysical Journal, 314 (2). pp. 431-438. ISSN 0004-637X. doi:10.1086/165076. https://resolver.caltech.edu/CaltechAUTHORS:20161005-153314099

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Abstract

The theoretical expectation for large-scale streaming velocities relative to the Hubble flow is expressed in terms of statistical correlation functions. Only for objects that trace the mass would these velocities have a simple cosmological interpretation. If some biasing effects the objects' formation, then nonlinear gravitational evolution is essential to predicting the expected large-scale velocities, which also depend on the nature of the biasing.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/165076DOIArticle
http://adsabs.harvard.edu/abs/1987ApJ...314..431GADSArticle
ORCID:
AuthorORCID
Politzer, H. David0000-0002-4983-6621
Additional Information:© 1987 American Astronomical Society. Provided by the NASA Astrophysics Data System. Received 1986 June 20; accepted 1986 September 9. Work supported in part by the US Department of Energy under contract DEAC03-81-ER40050. Supported in part by US Department of Energy Outstanding Junior Investigator Program under contract DE-FG03-84-ER40172.
Funders:
Funding AgencyGrant Number
Department of Energy (DOE)DE-FG03-84-ER40172
Department of Energy (DOE)DE-AC03-81-ER40050
Issue or Number:2
DOI:10.1086/165076
Record Number:CaltechAUTHORS:20161005-153314099
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20161005-153314099
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:70895
Collection:CaltechAUTHORS
Deposited By: Joy Painter
Deposited On:05 Oct 2016 22:42
Last Modified:11 Nov 2021 04:36

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