Angular Diameter Distances in Clumpy Friedmann Universes
天体物理学
2009-10-30 v1
摘要
Solving null-geodesic equations, behavior of angular diameter distances is studied in inhomogeneous cosmological models, which are given by performing N-body simulations with the CDM spectrum. The distances depend on the separation angle of ray pairs, the mass and the radius of particles cosisting of galaxies and dark matter balls, and cosmological model parameters. The calculated distances are compared with the Dyer- Roeder distance, and after many ray-shooting, the average, dispersion and distribution of the clumpiness parameter are derived.
引用
@article{arxiv.astro-ph/9806047,
title = {Angular Diameter Distances in Clumpy Friedmann Universes},
author = {Kenji Tomita},
journal= {arXiv preprint arXiv:astro-ph/9806047},
year = {2009}
}
备注
12 pages, 18 Postscript figures