Journal
NUCLEAR PHYSICS B
Volume 873, Issue 3, Pages 514-529Publisher
ELSEVIER
DOI: 10.1016/j.nuclphysb.2013.05.009
Keywords
-
Categories
Funding
- Swiss National Science Foundation (SNSF) [200021140236]
Ask authors/readers for more resources
We study the symmetries enjoyed by the Newtonian equations of motion of the non-relativistic dark matter fluid coupled to gravity which give rise to the phenomenon of gravitational instability. We also discuss some consistency relations involving the soft limit of the (n + 1)-correlator functions of matter and galaxy overdensities. (C) 2013 Published by Elsevier B.V.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available