Evolution of boson-fermion stars

被引：1

作者：

Valdez-Alvarado, Susana ^{[1
]}

Palenzuela, Carlos ^{[2
]}

Alic, Daniela ^{[3
]}

Arturo Urena-Lopez, L. ^{[1
]}

Becerril, Ricardo ^{[4
]}

机构：

[1] Univ Guanajuato, DCI, Dept Fis, Campus Leon, Leon 37150, Guanajuato, Mexico

[2] Univ Toronto, Canadian Inst Theoret Astrophys, Toronto, ON, Canada

[3] Albert Einstein Inst, Max Planck Inst Gravitat Phys, Potsdam, Germany

[4] Univ Michoacana, Inst Fis & Matemat, Morelia 58040, Michoacan, Mexico

来源：

IX WORKSHOP OF THE GRAVITATION AND MATHEMATICAL PHYSICS DIVISION OF THE MEXICAN PHYSICAL SOCIETY | 2012年 / 1473卷

关键词：

Scalar fields; boson; fermion; self-gravitating systems; STABILITY; CONFIGURATIONS;

D O I：

10.1063/1.4748532

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The boson-fermion stars can be modeled with a complex scalar field coupled minimally to a perfect fluid (i.e., without viscosity and non-dissipative). We present a study of these solutions and their dynamical evolution by solving numerically the Einstein-Klein-Gordon-Hydrodynamic (EKGHD) system. It is shown that stable configurations exist, but stability of general configurations depends finely upon the number of bosons and fermions.

引用

页码：43 / 48

页数：6

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