Lemaitre-Tolman Universes and CMB Anisotropies

Details Lemaitre-Tolman Universes and CMB Anisotropies Lemaitre-Tolman Universes and CMB Anisotropies

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002nmgm.meet.1984s&link_type=abstract

"THE NINTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and R

Physics

Scientific paper

Many papers have been devoted to estimate the Cosmic Microwave Background (CMB) anisotropy produced by isolated spherical cosmological structures. These estimations were performed using the Swiss-Cheese model and the Lemaitre-Tolman solution (LTS) of Einstein's equations. We focus our attention on a series of papers based on the LTS, in which the anisotropies produced by isolated Great Attractor-Like (GAL) objects and voids were studied in detail. The most interesting results were obtained in the case of very open universes (Ω < 0.5). Some of these results and the perspectives for future LTS estimates of CMB anisotropies are discussed.

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