Impact of charged and quantum-correction on the dynamics of scalar shell surrounded by Kiselev black hole

• Published in: Annals of physics 2024-05, Vol.464, p.169658, Article 169658
• Main Authors: Javed, Faisal, Alshehri, Mansoor H.
• Format: Article
• Language: English
• Subjects: Black hole; Scalar field; Stability analysis; Thin-shell formalism
• ISSN: 0003-4916; 1096-035X
• DOI: 10.1016/j.aop.2024.169658

The objective of this study is to investigate the geometric configurations of a thin-shell in the framework of quantum-corrected charged Kiselev black holes. In order to do this, a cut and paste technique is employed to align the inner Minkowski spacetime with the black hole solutions under consideration. Our research explores the effects of quantum-correction on the stability of thin-shell using linearized radial perturbation method incorporating the phantomlike equation of state such as quintessence. This approach allows for the identification of stable configurations of the thin-shell situated beyond the expected location of the event horizon in the exterior manifold. Moreover, it is evident that the stability of the thin-shell is significantly dependent on the parameters associated with the black hole solutions. In this study, we investigate the dynamics of the thin-shell configuration using Klein–Gordon’s equation of motion, including both massive and massless scalar fields. The results of our study suggest that the presence of the scalar field has a significant impact on the behavior of the thin-shell, resulting in notable phenomena such as expansion and collapse. The aforementioned results provide valuable insights into the behavior of black hole solutions by examining the dynamics of thin-shells in relation to quantum-correction parameters involving scalar fields. In summary, it is observed that the presence of a quantum-correction parameter has the effect of reducing the stable configuration of a Kiselev black holes. •Construction of thin-shell in the framework of quantum-corrected charged Kiselev black holes.•Stability of thin-shell with linearized radial perturbation.•Effects of phantomlike equation of state on the stability of thin-shell.•Dynamics of scalar shell composed with massless and massive scalar fields.