Gravitational lensing study of cold dark matter-led galactic halo. (English) Zbl 1490.83047
Summary: In this work, the spacetime geometry of the halo region in spiral galaxies is obtained considering the observed flat galactic rotation curve feature, invoking the Tully-Fisher relation and assuming the presence of cold dark matter in the galaxy. The gravitational lensing analysis is performed treating the so-obtained spacetime as a gravitational lens. It is found that the aforementioned spacetime as the gravitational lens can consistently explain the galaxy-galaxy weak gravitational lensing observations and the lensing observations of the well-known Abell 370 and Abell 2390 galaxy clusters.
MSC:
| 83C56 | Dark matter and dark energy |
| 83C50 | Electromagnetic fields in general relativity and gravitational theory |
| 78A45 | Diffraction, scattering |
| 83C55 | Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) |
| 76E07 | Rotation in hydrodynamic stability |
| 14H50 | Plane and space curves |
| 85A05 | Galactic and stellar dynamics |
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