A Generalized Double Chaplygin Model for Anisotropic Matter: The Newtonian Case

被引:6
作者
Abellan, Gabriel [1 ]
Rincon, Angel [2 ,3 ]
Sanchez, Eduard [1 ]
机构
[1] Univ Cent Venezuela, Escuela Fis, Fac Ciencias, Caracas 1050, Venezuela
[2] Univ Alicante, Dept Fis Aplicada, Campus San Vicente Raspeig, E-03690 Alicante, Spain
[3] Univ Tarapaca, Sede Esmeralda, Avda Luis Emilio Recabarren 2477, Iquique 1113749, Chile
关键词
relativistic stars; generalized Chaplygin model; anisotropy; STARS; EQUATIONS;
D O I
10.3390/universe9080352
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this work, we investigate astrophysical systems in a Newtonian regime using anisotropic matter. For this purpose, we considered that both radial and tangential pressures satisfy a generalized Chaplygin-type equation of state. Using this model, we found the Lane-Emden equation for this system and solved it numerically for several sets of parameters. Finally, we explored the mass supported by this physical system and compared it with the Chandrasekhar mass.
引用
收藏
页数:13
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