Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992rmxaa..24..113c&link_type=abstract
Revista Mexicana de Astronomia y Astrofisica, 24, 113
Astronomy and Astrophysics
Astronomy
Scientific paper
RESUMEN Utilizando metodos de integraci6n numerica se resuelven las ecuaciones de movimiento dinamicas que caracterizan un modelo de Universo constituido de dos fluidos la era de la recombinaci6n. Asumiendo perturbaciones iniciales en la densidad de materia del orden cle 10-6 y en Ia densidad de radiaci6n de 10-12 se obtienen solamente es decrecientes. ABSTRACT Via numerical methods, the dynamic equations of motion for characterizing a fluid modd of the Universe during the recombination era are solved. The only time decreasing behavior for initial conditions in matter, and radiation, density perturbatioiis of the order of 10-6 and 1012 respectively. Kcy : COSMOLOGY
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