The Astrophysical Journal · 1991 · 1.8K citations · 0 references
Natural SciencesAstronomyPhysicsAstrophysicsCosmologyGravitationAstrophysical SimulationsComputational AstrophysicsDark MatterGalaxy ClustersGaussian ProcessesMonte Carlo MethodsDark Matter ClusteringDark Matter HalosExcursion Set TheoryInitial Density PerturbationsMass DistributionMass Distribution EstimationProbability Mass FunctionsStar-forming Clumps
It is pointed out that most schemes for determining the mass function of virialized objects from the statistics of the initial density perturbation field suffer from the cloud-in-cloud problem of miscounting the number of low-mass clumps, many of which would have been subsumed into larger objects. The paper proposes a solution based on the theory of the excursion sets of F(r, R<SUB>f),</SUB> the four-dimensional initial density perturbation field smoothed with a continuous hierarchy of filters of radii R sub f.