Dark matter supporting traversable wormholes in the Galactic halo

被引:2
|
作者
Sarkar, Susmita [1 ]
Sarkar, Nayan [2 ]
Aktar, Somi [3 ]
Sarkar, Moumita [3 ]
Rahaman, Farook [3 ]
Yadav, Anil Kumar [4 ]
机构
[1] Haldia Inst Technol, Dept Appl Sci & Humanities, Haldia 721606, West Bengal, India
[2] Karimpur Pannadevi Coll, Dept Math, Nadia 741152, West Bengal, India
[3] Jadavpur Univ, Dept Math, Kolkata 700 032, India
[4] United Coll Engn & Res, Dept Phys, Greater Noida 201306, India
关键词
Milky Way galactic halo; Dark matter; Wormhole; POSSIBLE EXISTENCE; EMPIRICAL-MODELS; DENSITY PROFILE; ENERGY; CONSTRUCTION; STABILITY; CAUSALITY; FORM;
D O I
10.1016/j.newast.2023.102183
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the Morris-Thorne traversable asymptotically flat and non-flat wormholes in the galactic halo of the Milky Way Galaxy(MWG) based on the Einasto dark matter(DM) density profile. Our reported shape function is positive and increasing in nature, moreover, satisfies all the essential wormhole representing conditions i.e. the reported shape function forms wormhole like structures in the galactic halo region of the MWG. Furthermore, the wormhole containing the DM candidate of the halo shelters wormholes by violating the null energy condition (NEC) with respect to three different redshift functions. The wormholes, namely, WH1 and WH2 corresponding to the first two choices of redshift functions are asymptotically flat while the WH3 corresponding to the third choice of redshift function is asymptotically non-flat. We, here, also analyze the ANEC violating matter content, embedding surface, and proper radial distance for our solutions.
引用
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页数:8
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