Published August 21, 2013
| Version v1
Journal article
Symmetries and consistency relations in the large scale structure of the universe
Creators
- 1. Physics Division, National Technical University of Athens, 15780 Zografou Campus, Athens (Greece)
- 2. Department of Theoretical Physics and Center for Astroparticle Physics (CAP), 24 quai E. Ansermet, CH-1211 Geneva 4 (Switzerland)
Description
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
Availability note (English)
Available from http://dx.doi.org/10.1016/j.nuclphysb.2013.05.009Additional details
Identifiers
- DOI
- 10.1016/j.nuclphysb.2013.05.009;
- arXiv
- arXiv:1302.0130v2;
- PII
- S0550-3213(13)00271-X;
Publishing Information
- Journal Title
- Nuclear Physics. B
- Journal Volume
- 873
- Journal Issue
- 3
- Journal Page Range
- p. 514-529
- ISSN
- 0550-3213
- CODEN
- NUPBBO
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 45062284
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- EQUATIONS OF MOTION; GALAXIES; GRAVITATION; GRAVITATIONAL INSTABILITY; NONLUMINOUS MATTER; RELATIVISTIC RANGE; SYMMETRY; UNIVERSE
- Descriptors DEC
- DIFFERENTIAL EQUATIONS; ENERGY RANGE; EQUATIONS; INSTABILITY; MATTER; PARTIAL DIFFERENTIAL EQUATIONS; PLASMA INSTABILITY
Optional Information
- Copyright
- Copyright (c) 2013 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.