Towards an analytic construction of the wavefunction of boson stars

被引:21
|
作者
Kling, Felix [1 ]
Rajaraman, Arvind [1 ]
机构
[1] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA
基金
美国国家科学基金会;
关键词
STRONG CP PROBLEM; SCHRODINGER-NEWTON EQUATIONS; PRIMORDIAL BLACK-HOLES; INVISIBLE-AXION; DWARF GALAXIES; SCALAR FIELDS; MATTER; PSEUDOPARTICLES; CONSERVATION; VACUUM;
D O I
10.1103/PhysRevD.96.044039
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Light scalar fields can form gravitationally bound compact objects called boson stars. The profile of boson stars in the Newtonian limit is described by the Gross-Pitaevskii-Poisson equations. We present a semianalytic solution to these equations and construct the profile of boson stars formed by a noninteracting scalar field. Our solution is stable with respect to numerical errors and has accuracy better than 10-6 over the entire range.
引用
收藏
页数:9
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