On the Stability of the CMB Autocorrelation Function on Cosmological Parameters

Simple item page
dc.creatorMelkonian, A. A.
dc.date1999-02-20
dc.date.accessioned2026-07-07T02:30:32Z
dc.date.available2026-07-07T02:30:32Z
dc.descriptionThe 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.
dc.descriptionLatex, 4 pages, 3 EPS figures. e-mail: anahit@lx2.yerphi.am
dc.identifierhttps://arxiv.org/abs/astro-ph/9902301
dc.identifierhttp://arxiv.org/abs/astro-ph/9902301
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13849
dc.subjectAstrophysics
dc.titleOn the Stability of the CMB Autocorrelation Function on Cosmological Parameters
dc.typetext

Files

Collections

arXiv