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Quasi-periodic oscillations and particle motion around charged black hole surrounded by a cloud of strings and quintessence field in Rastall gravity

Asifa AshrafZhejiang Normal University, Zhejiang Normal University, Jinhua, Zhejiang, 321004, CHINAAllah DittaMathematics , Shanghai University, Shanghai University Shanghai, China, Shanghai, 200444, CHINADeğer SofuoğluPhysics, Istanbul University, Istanbul University Science Faculty, Physics Department Mathematical Physics Division, Vezneciler Fatih, Istanbul, 341324, TURKEYWen‐Xiu MaMathematics and Statistics, University of Southern California, Mathematics and Statistics, Tampa, 33620, UNITED STATESFaisal JavedDepartment of Physics, Zhejiang Normal University, Department of Physics, Jinhua, 321004, CHINAFarruh AtamurotovInha University in Tashkent, Inha University in Tashkent, Tashkent, Tashkent, 100170, CHINAAsif MahmoodKing Saud University, Kind Saud University, RIYADH, 11421, SAUDI ARABIA
Physica Scriptajournal2024en
ABI

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Abstract This work mainly focuses on unveiling the particle dynamics features of black holes. For this objective, we utilize the charged black hole geometry consisting of the cloud strings and quintessence under the ansatz of Rastall gravity. We have calculated and analyzed the effective potential, angular momentum, particle energy, horizon radius, inner stable circular orbit, photon sphere radius, quasi-periodic oscillations, and effective force to reveal the dynamical features. We in detail discussed the effects of charge in black hole, Rastall parameter, strings of cloud parameter, and quintessential parameter on the calculated results. To ensure the scenario of accelerated expansion, ω q lies in the range −1 < ω q < −1/3. From this specific range, we choose ω q = −2/3.

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