Shadow of a Kaluza-Klein rotating dilaton black hole

被引:196
作者
Amarilla, Leonardo [1 ]
Eiroa, Ernesto F. [1 ,2 ]
机构
[1] Univ Buenos Aires, Fac Ciencias Exactas & Nat, Dept Fis, RA-1428 Buenos Aires, DF, Argentina
[2] Inst Astron & Fis Espacio, RA-1428 Buenos Aires, DF, Argentina
来源
PHYSICAL REVIEW D | 2013年 / 87卷 / 04期
关键词
GALACTIC-CENTER; FIELD; PARAMETERS;
D O I
10.1103/PhysRevD.87.044057
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the shadow produced by a spinning Kaluza-Klein black hole in Einstein gravity coupled to a Maxwell field and a dilaton. The size and the shape of the shadow depend on the mass, the charge, and the angular momentum. We find that, for fixed values of these parameters, the shadow is slightly larger and less deformed than for its Kerr-Newman counterpart. DOI: 10.1103/PhysRevD.87.044057
引用
收藏
页数:7
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