THE DEFLECTION OF LIGHT RAYS IN THE GALAXIES’ HALOS OF DARK MATTER

Authors

  • G.M. Avkhunbayeva Fesenkov Astrophysical Institute, Almaty, Kazakhstan
  • Y.K. Aimuratov Abay Kazakh National Pedagogical University, Almaty, Kazakhstan
  • A.Zh. Umiralieva Fesenkov Astrophysical Institute, Almaty, Kazakhstan

Abstract

The deflection of light rays in the halos of dark matter described by Navarro-Frenk-White, Burket, Einasto and Kravtsov-Klypin profiles were searched. Numerical estimations for deflecting angles gives magnitude ~0.”00001, that are two orders smaller than achievement accuracy at the gravitational microlensing.

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Published

2017-10-10

Issue

Vol. 2011 No. 3 (2011): KazNU Bulletin. Physics series

Section

Theoretical Physics. Nuclear and Elementary Particle Physics. Astrophysics

How to Cite

[1]
G. Avkhunbayeva, Y. Aimuratov, and A. Umiralieva, “THE DEFLECTION OF LIGHT RAYS IN THE GALAXIES’ HALOS OF DARK MATTER”, Rec.Contr.Phys., vol. 2011, no. 3, pp. 59–67, Oct. 2017, Accessed: Jul. 09, 2026. [Online]. Available: https://bph.kaznu.kz/index.php/zhuzhu/article/view/978

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