A new asymptotical flat and spherically symmetric solution in the generalized Einstein-Cartan-Kibble-Sciama gravity and gravitational lensing

被引:9
|
作者
Chen, Songbai [1 ,2 ,3 ,4 ,5 ]
Zhang, Lu [1 ,2 ,3 ]
Jing, Jiliang [1 ,2 ,3 ,4 ,5 ]
机构
[1] Hunan Normal Univ, Inst Phys, Changsha 410081, Hunan, Peoples R China
[2] Hunan Normal Univ, Dept Phys, Changsha 410081, Hunan, Peoples R China
[3] Hunan Normal Univ, Minist Educ, Key Lab Low Dimens Quantum Struct & Quantum Contr, Changsha 410081, Hunan, Peoples R China
[4] Hunan Normal Univ, Synerget Innovat Ctr Quantum Effects & Applicat, Changsha 410081, Hunan, Peoples R China
[5] Yangzhou Univ, Coll Phys Sci & Technol, Ctr Gravitat & Cosmol, Yangzhou 225009, Jiangsu, Peoples R China
来源
EUROPEAN PHYSICAL JOURNAL C | 2018年 / 78卷 / 11期
基金
中国国家自然科学基金;
关键词
POINCARE GAUGE-THEORY; BLACK-HOLES; SPIN; RELATIVITY; UNIVERSE; SUPERNOVAE; TORSION; FIELD; CONSTRAINTS; 2ND-ORDER;
D O I
10.1140/epjc/s10052-018-6466-9
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We firstly present a new asymptotical flat and spherically symmetric solution in the generalized Einstein-Cartan-Kibble-Sciama theory of gravity and then investigate the propagation of photon in this background. This solution possesses three independent parameters which affect sharply photon sphere, deflection angle of light ray and gravitational lensing. Since the condition of existence of horizons is not inconsistent with that of photon sphere, there exists a special case where there is horizon but no photon sphere in this spacetime. Especially, we find that in this special case, the deflection angle of a light ray near the event horizon tends to a finite value rather than diverges, which is not explored in other spacetimes. We also study the strong gravitational lensing in this spacetime with the photon sphere and then probe how the spacetime parameters affect the coefficients in the strong field limit.
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页数:14
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