Teoria Grossa para o Decaimento Beta: Eficiência, Vantagens e Desvantagens em Aplicações Astrofísicas

Roberto Claudino Ferreira; Alejandro Javier Dimarco; Arturo Rodolfo Samana

doi:10.22481/exon.v3i2.19449

Authors

Roberto Claudino Ferreira Southwest Bahia State University
Alejandro Javier Dimarco Universidade Estadual de Santa Cruz
Arturo Rodolfo Samana Universidade Estadual de Santa Cruz

DOI:

https://doi.org/10.22481/exon.v3i2.19449

Keywords:

Taxas, Decaimento Beta, Teoria Grossa

Abstract

This work consists of a survey about the model Gross Theory for the Beta Decay, encompassing and linking the ideas and approaches presented by the authors of the original Gross Theory parameters most current experimental mass defects and removing some approximations to the function Fermi. We performed a comparison of results calculated for a sample of 94 nuclei of interest in the Pre-supernova with the experimental data and with other models when available, to analyze the efficiency, advantages and disadvantages of the Gross Theory for astrophysical applications.

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