The three-point function in large-scale structure – I. The weakly non-linear regime in N-body simulations
Open Access
- 21 June 2002
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 333 (2) , 443-453
- https://doi.org/10.1046/j.1365-8711.2002.05431.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 30 references indexed in Scilit:
- Cosmic microwave background bispectrum and slow-roll inflationMonthly Notices of the Royal Astronomical Society, 2000
- The Angular Three‐Point Correlation Function in the Quasi‐linear RegimeThe Astrophysical Journal, 2000
- The Projected Three-Point Correlation Function: Theory and ObservationsThe Astrophysical Journal, 1999
- The Power Spectrum, Bias Evolution, and the Spatial Three‐Point Correlation FunctionThe Astrophysical Journal, 1999
- Non-Gaussian effects in the cosmic microwave background from inflationPhysical Review D, 1994
- The three-point correlation function of the cosmic microwave background in inflationary modelsThe Astrophysical Journal, 1994
- Perturbations from cosmic strings in cold dark matterPhysical Review Letters, 1992
- Non-gaussian density perturbations in inflationary cosmologiesPhysics Letters B, 1987
- Numerical techniques for large cosmological N-body simulationsThe Astrophysical Journal Supplement Series, 1985
- The Galaxy correlation hierarchy in perturbation theoryThe Astrophysical Journal, 1984