Tidal forces in Kiselev black hole
M. Umair ShahzadCAMS, UCP Business School, University of Central Punjab, Lahore, PakistanAbdul JawadDepartment of Mathematics, COMSATS Institute of Information Technology, Lahore, 54000, Pakistan
2017en
ABI
Abstract
The aim of this paper is to examine the tidal forces occurring in a Kiselev black hole surrounded by radiation and dust fluids. It is noted that the radial and angular components of the tidal force change the sign between event and Cauchy horizons. We solve the geodesic deviation equation for radially free-falling bodies toward Kiselev black holes. We explain the geodesic deviation vector graphically and point out the location of the event and Cauchy horizons for specific values of the radiation and dust parameters.
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