On Random Walks with a General Moving Barrier
arXiv:astro-ph/0508384 · doi:10.1086/499802
Abstract
Random walks with a general, nonlinear barrier have found recent applications ranging from reionization topology to refinements in the excursion set theory of halos. Here, we derive the first-crossing distribution of random walks with a moving barrier of an arbitrary shape. Such a distribution is shown to satisfy an integral equation that can be solved by a simple matrix inversion, without the need for Monte Carlo simulations, making this useful for exploring a large parameter space. We discuss examples in which common analytic approximations fail, a failure which can be remedied using the method described here.
6 pages, 7 figures, submitted to ApJ
References in corpus (17)
- Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes
- An excursion set model of hierarchical clustering: Ellipsoidal collapse and the moving barrier
- The Growth of HII Regions During Reionization
- A hierarchy of voids: Much ado about nothing
- Cosmological Reionization by Stellar Sources
- The Reionization History at High Redshifts I: Physical Models and New Constraints from CMB Polarization
- Taxing the Rich: Recombinations and Bubble Growth During Reionization
- Cosmic Reionisation by Stellar Sources: Population III Stars
- Cosmic Reionisation by Stellar Sources: Population II Stars
- Simulating IGM Reionization
- An Analytical Model for the Triaxial Collapse of Cosmological Perturbations
- An excursion set model for the distribution of dark matter and dark matter haloes
- The Evidence of Absence: Galaxy Voids in the Excursion Set Formalism
- Did the Universe Reionize at Redshift Six?
- Cosmic Mass Functions from Gaussian Stochastic Diffusion Processes
- Was the Universe Reionized at Redshift 10?
- Non-Markov Excursion Set Model of Dark Matter Halo Abundances
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