Dirac-Proca stars

被引:0
|
作者
Ma, Tian-Xiang [1 ,2 ,3 ,4 ]
Liang, Chen [1 ,2 ,3 ,4 ]
Ren, Ji-Rong [1 ,2 ,3 ,4 ]
Wang, Yong-Qiang [1 ,2 ,3 ,4 ]
机构
[1] Lanzhou Univ, Lanzhou Ctr Theoret Phys, Key Lab Quantum Theory & Applicat, MoE, Lanzhou 730000, Peoples R China
[2] Lanzhou Univ, Inst Theoret Phys, Key Lab Theoret Phys Gansu Prov, Lanzhou 730000, Peoples R China
[3] Lanzhou Univ, Res Ctr Gravitat, Lanzhou 730000, Peoples R China
[4] Lanzhou Univ, Sch Phys Sci & Technol, Lanzhou 730000, Peoples R China
基金
中国国家自然科学基金;
关键词
BOSON STARS; DARK-MATTER; SCALAR;
D O I
10.1103/PhysRevD.109.084012
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider a Dirac-Proca star (DPS) model that consists of the Einstein gravity in four-dimensional spacetime, a Proca field, and two Dirac fields through minimal coupling. By numerically solving this model, we obtain two types of solutions: synchronized frequency solutions and nonsynchronized frequency solutions. We find that in the case of two kinds of matter fields, different families of solutions can be obtained in both synchronized and nonsynchronized frequency cases, and the two families can shift to each other when certain parameters are changed. Moreover, we calculate the binding energy of multifield solutions and give the relationship between binding energy E and synchronized frequency (omega) over tilde (nonsynchronized frequency (omega) over tilde (P)).
引用
收藏
页数:13
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