Features of galactic halo in a brane world model and observational constraints

被引:37
作者
Nandi, K. K. [1 ,2 ,3 ]
Filippov, A. I. [3 ]
Rahaman, F. [4 ]
Ray, Saibal [5 ]
Usmani, A. A. [6 ]
Kalam, M. [7 ]
DeBenedictis, A. [8 ,9 ]
机构
[1] Univ N Bengal, Dept Math, Siliguri 734013, W Bengal, India
[2] Bashkir State Pedag Univ, Joint Res Lab, Ufa 450000, Russia
[3] Sterlitamak State Pedag Acad, Dept Theoret Phys, Sterlitamak 453103, Russia
[4] Jadavpur Univ, Dept Math, Kolkata 700032, W Bengal, India
[5] Govt Coll Engn & Ceram Technol, Dept Phys, Kolkata 700010, W Bengal, India
[6] Aligarh Muslim Univ, Dept Phys, Aligarh 202002, Uttar Pradesh, India
[7] Netaji Nagar Coll Women, Dept Phys, Kolkata 700092, W Bengal, India
[8] Simon Fraser Univ, Pacific Inst Math Sci, Burnaby, BC V5A 1S6, Canada
[9] Simon Fraser Univ, Dept Phys, Burnaby, BC V5A 1S6, Canada
关键词
gravitation; galaxies: general; galaxies: structure; dark matter; LUMINOSITY SPIRAL GALAXIES; OPTICAL-MECHANICAL ANALOGY; EXTENDED ROTATION CURVES; DARK-MATTER; SCALAR FIELDS; WORMHOLES; ANTIGRAVITY; CLUSTERS; TENSOR; INDEX;
D O I
10.1111/j.1365-2966.2009.15399.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Several aspects of the 4d imprint of the 5d bulk Weyl radiation are investigated within a recently proposed model solution. It is shown that the solution has a number of physically interesting properties. The constraints on the model imposed by combined measurements of rotation curve and lensing are discussed. A brief comparison with a well-known scalar field model is also given.
引用
收藏
页码:2079 / 2087
页数:9
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