Thin accretion disks and charged rotating dilaton black holes
M Heydari-Fard, M Heydari-Fard… - The European Physical …, 2020 - Springer
Einstein-Maxwell-dilaton theory is an interesting theory of gravity for studying scalar fields in
the context of no-hair theorem. In this work, we consider static charged dilaton and charged …
the context of no-hair theorem. In this work, we consider static charged dilaton and charged …
Static spherically symmetric Einstein-Yang-Mills-dilaton black hole and its thermodynamics
MM Stetsko - Physical Review D, 2020 - APS
A static black hole with spherical symmetry is obtained and examined in the framework of
Einstein-Yang-Mills-dilaton theory. The obtained black hole solution allowed us to derive …
Einstein-Yang-Mills-dilaton theory. The obtained black hole solution allowed us to derive …
Static dilatonic black hole with nonlinear Maxwell and Yang–Mills fields of power-law type
MM Stetsko - General Relativity and Gravitation, 2021 - Springer
Static spherically symmetric black hole solution is obtained in the framework of Einstein-
dilaton theory with nonlinear Maxwell and Yang–Mills fields of power-law type. It is observed …
dilaton theory with nonlinear Maxwell and Yang–Mills fields of power-law type. It is observed …
Higher dimensional slowly rotating dilaton black holes in AdS spacetime
A Sheykhi, M Allahverdizadeh - … Review D—Particles, Fields, Gravitation, and …, 2008 - APS
In this paper, with an appropriate combination of three Liouville-type dilaton potentials, we
obtain the higher dimensional charged slowly rotating dilaton black hole solution for …
obtain the higher dimensional charged slowly rotating dilaton black hole solution for …
[HTML][HTML] Thermodynamics of charged Brans–Dicke AdS black holes
A Sheykhi, MM Yazdanpanah - Physics Letters B, 2009 - Elsevier
It is well known that in four dimensions, black hole solution of the Brans–Dicke–Maxwell
equations is just the Reissner–Nordstrom solution with a constant scalar field. However, in …
equations is just the Reissner–Nordstrom solution with a constant scalar field. However, in …
Properties of rotating Einstein-Maxwell-dilaton black holes in odd dimensions
JL Blázquez-Salcedo, J Kunz, F Navarro-Lérida - Physical Review D, 2014 - APS
We investigate rotating Einstein-Maxwell-dilaton (EMd) black holes in odd dimensions.
Focusing on black holes with equal-magnitude angular momenta, we determine the domain …
Focusing on black holes with equal-magnitude angular momenta, we determine the domain …
Static spherically symmetric black hole's solution in Einstein–Maxwell–Yang–Mills-dilaton theory
MM Stetsko - International Journal of Modern Physics A, 2021 - World Scientific
In this work a static spherically symmetric black hole's solution within the Einstein–Maxwell–
Yang–Mills-dilaton theory is derived. The obtained solution is examined, in particular, we …
Yang–Mills-dilaton theory is derived. The obtained solution is examined, in particular, we …
Slowly rotating Einstein–Maxwell-dilaton black hole and some aspects of its thermodynamics
MM Stetsko - The European Physical Journal C, 2019 - Springer
A slowly rotating black hole solution in Einstein–Maxwell-dilaton gravity is considered. Using
the obtained solution we investigate thermodynamic functions such as the black hole's …
the obtained solution we investigate thermodynamic functions such as the black hole's …
Extremal charged rotating dilaton black holes in odd dimensions
M Allahverdizadeh, J Kunz, F Navarro-Lérida - Physical Review D—Particles …, 2010 - APS
Employing higher-order perturbation theory, we find a new class of charged rotating black
hole solutions of Einstein-Maxwell-dilaton theory with general dilaton coupling constant …
hole solutions of Einstein-Maxwell-dilaton theory with general dilaton coupling constant …
Higher dimensional charged rotating dilaton black holes
A Sheykhi, M Allahverdizadeh - General Relativity and Gravitation, 2010 - Springer
In this paper, we present the metric for the n-dimensional charged slowly rotating dilaton
black hole with N=[(n− 1)/2] independent rotation parameters, associated with N orthogonal …
black hole with N=[(n− 1)/2] independent rotation parameters, associated with N orthogonal …