宇宙学中的闵可夫函数
天体物理学
2008-02-03 v2
摘要
闵可夫函数提供了一种新颖的工具来表征宇宙中星系大尺度分布。本文对这些形态测度的基本特征进行简要教程，并指出其对于模拟数据和星系红移目录的实际应用。
引用
@article{arxiv.astro-ph/9508154,
title = {Minkowski Functionals in Cosmology},
author = {J. Schmalzing and M. Kerscher and T. Buchert},
journal= {arXiv preprint arXiv:astro-ph/9508154},
year = {2008}
}
备注
9 pages, uuencoded gzipped ps-file, 300 kByte Proc. ``International School of Physics Enrico Fermi'', Course CXXXII: Dark Matter in the Universe, Varenna 1995, eds.: S. Bonometto, J. Primack, A. Provenzale, IOP, to appear; Corrected typing error in the last formula. Now it reads: \frac{M_{\mu-\nu}(D)}{M_0(D)} ^^^^ on the right side of the equation under the sum