On quasinormal modes in 4D black hole solutions in the model with anisotropic fluid
S. V. Bolokhov, V. D. Ivashchuk

TL;DR
This paper investigates quasinormal modes of a family of 4D black hole solutions influenced by anisotropic fluid, revealing their properties, global structure, and how they conform to the Hod conjecture across different parameters.
Contribution
It introduces a new family of black hole solutions with anisotropic fluid and analyzes their quasinormal modes, global structure, and thermodynamic properties, extending known results to a broader class.
Findings
Quasinormal modes match Schwarzschild results as q approaches infinity.
Hod conjecture holds for all q ≥ 2 and allowed parameters.
Global structure varies with q, resembling Reissner-Nordström or Schwarzschild types.
Abstract
We consider a family of 4-dimensional black hole solutions from Dehnen et al. ( Grav. Cosmol. 9:153, arXiv: gr-qc/0211049, 2003) governed by natural number , which appear in the model with anisotropic fluid and the equations of state: , , where and are pressures in radial and transverse directions, respectively, and is the density. These equations of state obey weak, strong and dominant energy conditions. For the metric of the solution coincides with that of the Reissner-Nordstr\"om one. The global structure of solutions is outlined, giving rise to Carter-Penrose diagram of Reissner-Nordstr\"om or Schwarzschild types for odd or even , respectively. Certain physical parameters corresponding to BH solutions (gravitational mass, PPN parameters, Hawking temperature and entropy) are…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Advanced Mathematical Physics Problems
