Method for distinguishing very compact stellar objects from black holes

被引:6
作者
Akhmedov, Emil T. [1 ,2 ]
Kalinov, Daniil A. [1 ]
Popov, Fedor K. [1 ,2 ,3 ]
机构
[1] Natl Res Univ Higher Sch Econ, Int Lab Representat Theory & Math Phys, Vavilova 7, Moscow 117312, Russia
[2] Inst Theoret & Expt Phys, B Cheremushkinskaya 25, Moscow 117218, Russia
[3] Moscow Inst Phys & Technol, Inst Skii Per 9, Dolgoprudnyi 141700, Russia
关键词
BOSON-FERMION STARS; GEOMETRY; EQUATION; COLLAPSE; GRAVITY;
D O I
10.1103/PhysRevD.93.064006
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We propose a way to distinguish a compact stellar object, whose size is very close to its Schwarzschild radius, from the collapsing stars. Namely, we show that massive fields in the vicinity of a very compact stellar object have discrete energy levels. (These levels are different from the standard nonrelativistic ones present in Coulomb-type potentials and from the quasinormal modes.) At the same time, we show that there are no such discrete levels for massive fields in the vicinity of a collapsing star.
引用
收藏
页数:6
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