The origin of scaling in the galaxy distribution
Open Access
- 1 August 1999
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 307 (2) , 376-386
- https://doi.org/10.1046/j.1365-8711.1999.02592.x
Abstract
No abstract availableKeywords
This publication has 36 references indexed in Scilit:
- Self-Similarity and Scaling Behavior of Scale-free Gravitational ClusteringThe Astrophysical Journal, 1996
- Properties of the cosmological density distribution functionThe Astrophysical Journal, 1995
- Non-linear evolution of density perturbations using the approximate constancy of the gravitational potentialMonthly Notices of the Royal Astronomical Society, 1994
- Linear Evolution of the Gravitational Potential: A New Approximation for the Nonlinear Evolution of Large-Scale StructureThe Astrophysical Journal, 1993
- Aspects of Zel'dovich ApproximationThe Astrophysical Journal, 1993
- Lagrangian theory of gravitational instability of Friedman–Lemaître cosmologies – second-order approach: an improved model for non-linear clusteringMonthly Notices of the Royal Astronomical Society, 1993
- Testing approximations for non-linear gravitational clusteringMonthly Notices of the Royal Astronomical Society, 1993
- The gravity-induced quasi-Gaussian correlation hierarchyThe Astrophysical Journal, 1992
- Lagrangian theory of gravitational instability of Friedman-Lematre cosmologies and the 'Zel'dovich approximation'Monthly Notices of the Royal Astronomical Society, 1992
- A lognormal model for the cosmological mass distributionMonthly Notices of the Royal Astronomical Society, 1991