Second-order Lagrangian perturbation theory initial conditions for resimulations
- 21 April 2010
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 403 (4) , 1859-1872
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This publication has 33 references indexed in Scilit:
- Transients from initial conditions in cosmological simulationsMonthly Notices of the Royal Astronomical Society, 2006
- Early structure in CDMMonthly Notices of the Royal Astronomical Society, 2005
- Galaxy Clusters in Hubble Volume Simulations: Cosmological Constraints from Sky Survey PopulationsThe Astrophysical Journal, 2002
- Multiscale Gaussian Random Fields and Their Application to Cosmological SimulationsThe Astrophysical Journal Supplement Series, 2001
- Dark matter haloes within clustersMonthly Notices of the Royal Astronomical Society, 1998
- Lagrangian theory of gravitational instability of Friedman-Lematre cosmologies - a generic third-order model for non-linear clusteringMonthly Notices of the Royal Astronomical Society, 1994
- The statistics of peaks of Gaussian random fieldsThe Astrophysical Journal, 1986
- The evolution of large-scale structure in a universe dominated by cold dark matterThe Astrophysical Journal, 1985
- Numerical techniques for large cosmological N-body simulationsThe Astrophysical Journal Supplement Series, 1985
- N-body simulations of galaxy clustering. I - Initial conditions and galaxy collapse timesThe Astrophysical Journal, 1979