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Path Integral Methods for Primordial Density Perturbations

Published online by Cambridge University Press:  03 August 2017

Edmund Bertschinger
Affiliation:
Department of Physics, M.I.T., Cambridge, MA 02139, U.S.A.
James M. Gelb
Affiliation:
Department of Physics, M.I.T., Cambridge, MA 02139, U.S.A.

Abstract

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Path integrals may be used to describe the statistical properties of a random field such as the primordial density perturbation field. In this framework the probability distribution is given for a Gaussian random field subjected to constraints such as the presence of a peak of given curvature at a specific location in the initial conditions. An algorithm has been constructed for generating samples of a constrained Gaussian random field on a lattice using Monte Carlo techniques. The algorithm is equivalent to, but much faster than, generating unconstrained random samples repeatedly until a sample is found satisfying the desired constraints to arbitrary precision. The method makes possible a systematic study of the density field around peaks or other constrained regions in the biased galaxy formation scenario and it is effective for generating initial conditions for N-body simulations with rare objects in the computational volume.

Type
Appendix 1: Poster Papers
Copyright
Copyright © Reidel 1988