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 protovoid or supercluster 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 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.
CITATION STYLE
Bertschinger, E. (1987). Path integral methods for primordial density perturbations - Sampling of constrained Gaussian random fields. The Astrophysical Journal, 323, L103. https://doi.org/10.1086/185066
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