Gravitational lensing and anisotropies of the cosmic background radiation on small angular scales
Author(s) -
J. M. Liu,
Jian Gong Gao
Publication year - 1995
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-8711
pISSN - 0035-8711
DOI - 10.1093/mnras/277.1.152
Subject(s) - physics , gravitational lens , astrophysics , anisotropy , omega , background radiation , cosmic cancer database , cosmic background radiation , cosmic microwave background , weak gravitational lensing , gravitation , gravitational wave , radiation , strong gravitational lensing , astronomy , galaxy , optics , redshift , quantum mechanics
We investigate the effect of gravitational lensing, produced by linear density perturbations, for anisotropies of the Cosmic Background Radiation (CBR) on scales of arcminutes. In calculations, a flat universe (\Omega=1) and the Harrison-Zel'dovich spectrum (n=1) are assumed. The numerical results show that on scales of a few arcminutes, gravitational lensing produces only negligible anisotropies in the temperature of the CBR. Our conclusion disagrees with that of Cay\'{o}n {\it et al.} who argue that the amplification of \Delta T/T on scales \le 3' may even be larger than 100\%
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