Speaker
José Carlos de Oliveira
(Federal University of Roraima)
Description
In the present work we have obtained the equation of state and the population of baryons and leptons to the highly asymmetric dense stellar matter, with the purpose of studying the effects of hyperons on the structure of neutron stars. To this end, we adopted the Zimanyi-Moszkowski model in the mean field approximation. From the equation of state obtained with the model, we solve numerically the Tolman-Oppenheimer-Volkoff (TOV) equation to the internal structure of neutron stars.
Author
José Carlos de Oliveira
(Federal University of Roraima)
Co-authors
Prof.
Hilário Rodrigues
(Centro Federal de Educação Tecnológica Celso Suckow da Fonseca (CEFET-RJ))
Prof.
Sérgio B. Duarte
(Centro Brasileiro de Pesquisas Físicas (CBPF/RJ))
Prof.
Marcelo Chiapparini
(Universidade do Estado do Rio de Janeiro - UERJ)