Numerical boson stars with a single Killing vector. I. The D ≥ 5 case

被引:13
作者
Stotyn, Sean [1 ]
Leonard, C. Danielle [2 ]
Oltean, Marius [3 ]
Henderson, Laura J. [4 ]
Mann, Robert B. [4 ]
机构
[1] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada
[2] Univ Oxford, Dept Phys, Oxford OX1 3RH, England
[3] McGill Univ, Dept Phys, Montreal, PQ H3A 2T8, Canada
[4] Univ Waterloo, Dept Phys & Astron, Waterloo, ON N2L 3G1, Canada
来源
PHYSICAL REVIEW D | 2014年 / 89卷 / 04期
基金
加拿大自然科学与工程研究理事会;
关键词
BLACK-HOLES;
D O I
10.1103/PhysRevD.89.044017
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We numerically construct asymptotically anti-de Sitter boson star solutions using a minimally coupled D-1/2tuplet complex scalar field in D = 5, 7, 9, 11 dimensions. The metric admits multiple Killing vector fields in general, however the scalar fields are only invariant under a particular combination, leading to such boson star solutions possessing just a single helical Killing symmetry. These boson stars form a one parameter family of solutions, which can be parametrized by the energy density at their center. As the central energy density tends to infinity, the angular velocity, mass, and angular momentum of the boson star exhibit damped harmonic oscillations about finite central values, while the Kretschmann invariant diverges, signaling the formation of a black hole in this limit.
引用
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页数:11
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