Wormholes in 4D Einstein-Gauss-Bonnet gravity

被引:93
|
作者
Jusufi, Kimet [1 ,2 ]
Banerjee, Ayan [3 ]
Ghosh, Sushant G. [3 ,4 ]
机构
[1] State Univ Tetovo, Phys Dept, Ilinden St Nn, Tetovo 1200, North Macedonia
[2] Ss Cyril & Methodius Univ, Fac Nat Sci & Math, Inst Phys, Arhimedova 3, Skopje 1000, North Macedonia
[3] Univ KwaZulu Natal, Astrophys & Cosmol Res Unit, Private Bag X54001, ZA-4000 Durban, South Africa
[4] Jamia Millia Islamia, Ctr Theoret Phys, New Delhi 110025, India
来源
EUROPEAN PHYSICAL JOURNAL C | 2020年 / 80卷 / 08期
关键词
TENSOR; SPACE;
D O I
10.1140/epjc/s10052-020-8287-x
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
Recent times witnessed a significant interest in regularizing, a D -> 4 limit, of EGB gravity initiated by Glavan and Lin [Phys. Rev. Lett. 124, 081301 (2020)] by re-scaling GB coupling constant as alpha/( D - 4) and taking limit D -> 4, and in turn these regularized 4D gravities have non-trivial gravitational dynamics. Interestingly, the maximally or spherically symmetric solution to all the regularized gravities coincides in the 4D case. In view of this, we obtain an exact spherically symmetric wormhole solution in the 4D EGB gravity for an isotropic and anisotropic matter sources. In this regard, we consider also a wormhole with a specific radial-dependent shape function, a power-law density profile as well as by imposing a particular equation of state. To this end, we analyze the flare-out conditions, embedding diagrams, energy conditions and the volume integral quantifier. In particular our -ve branch results, in the limit alpha -> 0, reduced exactly to vis-a-vis 4D Morris-Thorne of GR.
引用
收藏
页数:13
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