Approximate angular diameter distance in a locally inhomogeneous universe with nonzero cosmological constant

被引：24
作者：
Demianski, M
de Ritis, R
Marino, AA
Piedipalumbo, E
机构：
[1] Compl Univ Monte S Angelo, Ist Nazl Fis Nucl, Sez Napoli, I-80126 Naples, Italy
[2] Osserv Astron Capodimonte, I-80131 Naples, Italy
来源：
ASTRONOMY & ASTROPHYSICS | 2003年 / 411卷 / 02期
关键词：
cosmology : gravitational lensing; cosmology : theory;
D O I：
10.1051/0004-6361:20031234
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We discuss the general and approximate angular diameter distance in the Friedman-Robertson-Walker cosmological models with nonzero cosmological constant. We modify the equation for the angular diameter distance by taking into account the fact that locally the distribution of matter is non homogeneous. We present exact solutions of this equation in a few special cases. We propose an approximate analytic solution of this equation which is simple enough and sufficiently accurate to be useful in practical applications.
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收藏
页码：33 / 40
页数：8
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