Spinning boson stars and Kerr black holes with scalar hair: The effect of self-interactions

被引：35

作者：

Herdeiro, Carlos A. R. ^{[1
]}

Radu, Eugen

Runarsson, Helgi F.

机构：

[1] Univ Aveiro, Dept Fs, Campus Santiago, P-3810183 Aveiro, Portugal

来源：

INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 2016年 / 25卷 / 09期

基金：

欧盟地平线“2020”;

关键词：

Black holes; scalar field; boson stars; self-interactions;

D O I：

10.1142/S0218271816410145

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Self-interacting boson stars (BSs) have been shown to alleviate the astrophysically low maximal mass of their nonself-interacting counterparts. We report some physical features of spinning self-interacting BSs, namely their compactness, the occurrence of ergo-regions and the scalar field profiles, for a sample of values of the coupling parameter. The results agree with the general picture that these BSs are comparatively less compact than the nonself-interacting ones. We also briefly discuss the effect of scalar self-interactions on the properties of Kerr black holes with scalar hair.

引用

页数：11

共 18 条

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