S
Seyed Hossein Hendi
Researcher at Shiraz University
Publications - 272
Citations - 8849
Seyed Hossein Hendi is an academic researcher from Shiraz University. The author has contributed to research in topics: Black hole & Black hole thermodynamics. The author has an hindex of 55, co-authored 263 publications receiving 7620 citations. Previous affiliations of Seyed Hossein Hendi include Center for Excellence in Education & Yasouj University.
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Extended phase space thermodynamics and P-V criticality of black holes with a nonlinear source
TL;DR: In this article, the authors considered the solutions of Einstein gravity in the presence of a generalized Maxwell theory, namely power Maxwell invariant, and investigated the analogy of nonlinear charged black hole solutions with the Van der Waals liquid-gas system in the extended phase space where the cosmological constant appeared as pressure.
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Van der Waals like behavior of topological AdS black holes in massive gravity
TL;DR: In this article, van der Waals phase transitions of charged black holes in massive gravity were investigated, and it was shown that the mass of the graviton can generate a range of new phase transitions for topological black holes.
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Asymptotic charged BTZ black hole solutions
TL;DR: In this article, the authors generalized the (2 + 1)-dimensional Reissner-Nordstrom (BTZ) black hole to a three dimensional EH-based nonlinear electromagnetic field, motivated from obtaining a finite value for the self-energy of a pointlike charge.
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Einstein-Born-Infeld-Massive Gravity: adS-Black Hole Solutions and their Thermodynamical properties
TL;DR: In this article, the authors study massive gravity in the presence of Born-Infeld nonlinear electrodynamics and calculate the conserved and thermodynamic quantities and check the validation of the first law of thermodynamics.
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Phase transition and thermodynamic geometry of Einstein-Maxwell-dilaton black holes
TL;DR: In this article, the authors consider linearly charged dilatonic black holes and study their thermodynamic behavior in the context of phase transitions and thermodynamic geometry, and they show that, depending on the values of the parameters, these black holes can undergo two types of phase transition.