Published April 28, 1986
| Published + Erratum
Journal Article
Open
Two-Point Correlation for Rich Clusters of Galaxies
- Creators
- Otto, S.
-
Politzer, H. David
-
Wise, Mark B.
Abstract
The rich-cluster two-point correlation function is examined in a model where rich clusters of galaxies form at high peaks of primordial Gaussian mass-density fluctuations (averaged over a suitable volume). Particular attention is paid to the case when the primordial fluctuations have a Zel'dovich spectrum.
Additional Information
© 1986 American Physical Society. Received 27 February 1986. This work was supported in part by the U. S. Department of Energy under Contracts No. DE-AC-03-81-ER40050 and No. DE-AT03-83-ER31118. One of us (S.O.) is a Bantrell Fellow. Another of us (M.B.W.) is an Alfred P. Sloan Fellow and a U. S. Department of Energy Outstanding Junior Investigator (under Contract No. DE-F603-84ER40172).Errata
Two-Point Correlation for Rich Clusters of Galaxies S. Otto, H. David Politzer, and Mark B. Wise Phys. Rev. Lett. 56, 2772Attached Files
Published - PhysRevLett.56.1878.pdf
Erratum - PhysRevLett.56.2772.pdf
Files
PhysRevLett.56.2772.pdf
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Additional details
- Eprint ID
- 70893
- Resolver ID
- CaltechAUTHORS:20161005-152736636
- DE-AC-03-81-ER40050
- Department of Energy (DOE)
- DE-AT03-83-ER31118
- Department of Energy (DOE)
- Bantrell Fellowship
- Alfred P. Sloan Foundation
- DE-F603-84ER40172
- Department of Energy (DOE)
- Created
-
2016-10-05Created from EPrint's datestamp field
- Updated
-
2023-06-01Created from EPrint's last_modified field