Geodesics of Hayward black hole surrounded by quintessence

Scattering and absorption cross sections of Schwarzschild–anti-de Sitter black hole with quintessence

“…if we consider d 2 u dφ 2 = 0 the positive root corresponds to the radius of the critical orbit for null geodesic u c substituting in (10), we obtain the critical impact parameter bc .…”

“…Where Some cases of ω allow a relatively simple treatment of the properties of the geodesic equation of motion (10), then in order to analyze the geodesic equation we consider ω = −2/3, that can be written as;…”

“…Applying the ideas of Kiselev (2003) [6] that present a new static spherically symmetric exact solutions of the Einstein equations for quintessential matter surrounding a BH, different investigations have emerged. For example; the null geodesics for Schwarzschild surrounded by quintessence in [7] is addressed as well as Reissner-Nordström surrounded by quintessence in [8] also the thermodynamics of the black holes with quintessence are studied in [9] and Hayward black hole surrounded by quintessence in [10].…”

Quasinormal modes of the Hayward black hole surrounded by quintessence: scalar, electromagnetic and gravitational perturbations

“…Kiselev [19] proposed static and spherically symmetric solutions that describe BHs surrounded by quintessence. We focus our attention to the static, spherically symmetric Hayward BH [26] surrounded by quintessence, described by the line element [31]…”

“…Also, [29,30] studied the QNM of Hayward BH. The Geodesics structure for Hayward BH surrounded by quintessence in [31].…”