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Effects of shear and rotation on the spherical collapse model for clustering dark energy (2014)

First Author: Pace F

Attributed to: Theoretical Cosmology funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stu1782

Publication URI: http://dx.doi.org/10.1093/mnras/stu1782

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 1