On the Stability of the CMB Autocorrelation Function on Cosmological Parameters

Details On the Stability of the CMB Autocorrelation Function on Cosmological Parameters On the Stability of the CMB Autocorrelation Function on Cosmological Parameters

1999-02-20

arxiv.org/abs/astro-ph/9902301v1

Astronomy and Astrophysics

Astrophysics

Latex, 4 pages, 3 EPS figures. e-mail: anahit@lx2.yerphi.am

Scientific paper

The properties of the Cosmic Microwave Background Radiation angular
autocorrelation function in Friedman Universe with negative curvature (k=-1)
are studied. The dependence of the spectral index of autocorrelation function
on the density parameter of the Universe is studied numerically, taking into
account the effect of geodesic mixing, occuring in k=-1 curvature Universes.

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