Radial oscillations of charged strange stars

8th International Workshop on Hadron Physics

Arbañil, J.D.V.^1 ; Malheiro, M.^1

Departamento de Física, Instituto Tecnológico de Aeronáutica, Centro Técnico Aeroespacial, São José dos Campos, SP

12228-900, Brazil^1

关键词: Charge fractions;    Energy density;    Fluid pressures;    Fundamental modes;    Model equations;    Modified equation;    Radial oscillation;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/706/5/052022/pdf
DOI  :  10.1088/1742-6596/706/5/052022

来源: IOP

【 摘 要 】

The radial oscillations of charged strange quark stars is investigated. It is considered that the fluid pressure follows the MIT bag model equation of state and the charge density to be proportional to the energy density, ρe= αρ (where α is proportionality constant). The modified equations of radial oscillations to the introduction of the electric charge are integrated to determine the fundamental mode. It is found that the stability of the charged object decreases with the increment of the central energy density and with the growth of the charge fraction.