Obtenção da densidade eletrônica do modelo YMW16 para distâncias de estrelas de pulsares via Teoria de Campos.

Abstract

The Model YMW16 describes a calculation method to obtain electron density for estimating the distance of pulsar and FRB’s stars. Through the parameters addressed for galaxies of thick disks we arrived in the same formulation for electron density, via quantum eld theory. Using the Dirac equation coupled to a background eld with a prole of a hyperbolic tangent, we simulate the galactic disc and obtain the electronic density of the YMW model16.