Low-redshift formula for the luminosity distance in a LTB model with cosmological constant

The European Physical Journal C

Pisin Chen¹  Antonio Enea Romano² 

[1] Leung Center for Cosmology and Particle Astrophysics, National Taiwan University, Taipei, Taiwan;Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 94025, Menlo Park, CA, USA;Leung Center for Cosmology and Particle Astrophysics, National Taiwan University, Taipei, Taiwan;Yukawa Institute for Theoretical Physics, Kyoto University, 606-8502, Kyoto, Japan;Instituto de Fisica, Universidad de Antioquia, A.A.1226 , Medellin, Colombia;

关键词: Cosmological Constant;    Elliptic Function;    Geodesic Equation;    Local Inhomogeneity;    Luminosity Distance;   

DOI  :  10.1140/epjc/s10052-014-2780-z

来源: Springer

【 摘 要 】

We calculate the low-redshift Taylor expansion for the luminosity distance for an observer at the center of a spherically symmetric matter inhomogeneity with a non-vanishing cosmological constant. We then test the accuracy of the formulas comparing them to the numerical calculation for different cases for both the luminosity distance and the radial coordinate. The formulas can be used as a starting point to understand the general non-linear effects of a local inhomogeneity in the presence of a cosmological constant, without making any special assumption as regards the inhomogeneity profile.

【 授权许可】

CC BY