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181
Periodic orbits and gravitational wave radiation in short hair black hole spacetimes for an extreme mass ratio system
Published 2025-01-01“…Abstract For a short hair black hole(BH) that bypasses the “no-short-hair” theorem, its hair parameters have a significant impact near the event horizon and may thus carry the internal information of the BH. …”
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182
Hubble Space Telescope Observations within the Sphere of Influence of the Powerful Supermassive Black Hole in PKS 0745-191
Published 2025-01-01Subjects: “…Supermassive black holes…”
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183
Black Holes Have More States than Those Defined by the Bekenstein–Hawking Entropy: A Simple Argument
Published 2024-12-01Subjects: “…black hole entropy…”
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184
The Relation between the Quasi-Localized Energy-Momentum Complexes and the Thermodynamic Potential for the Schwarzschild-de Sitter Black Hole
Published 2017-01-01“…Here M is the patch between cosmological event horizon and black hole event horizon of the SdS black hole solution. …”
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185
Heun-Type Solutions of the Klein-Gordon and Dirac Equations in the Garfinkle-Horowitz-Strominger Dilaton Black Hole Background
Published 2019-01-01“…We study the Klein-Gordon and the Dirac equations in the background of the Garfinkle-Horowitz-Strominger black hole in the Einstein frame. Using a SO(3,1)×U(1)-gauge covariant approach, as an alternative to the Newman-Penrose formalism for the Dirac equation, it turns out that these solutions can be expressed in terms of Heun confluent functions and we discuss some of their properties.…”
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186
Distinguishing black holes with and without spontaneous scalarization in Einstein-scalar-Gauss–Bonnet theories via optical features
Published 2024-12-01“…Our findings reveal that the scalarized black holes consistently exhibit smaller shadow sizes and reduced brightness compared to Schwarzschild black holes. …”
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187
P-v Criticality of a Specific Black Hole in f(R) Gravity Coupled with Yang-Mills Field
Published 2018-01-01“…We study the P-v criticality of a specific charged AdS type black hole (SBH) in f(R) gravity coupled with Yang-Mills field. …”
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188
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189
Classical eikonal from Magnus expansion
Published 2025-01-01Subjects: “…Black Holes…”
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190
Pseudospectra of complex momentum modes
Published 2025-01-01Subjects: “…Black Holes…”
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191
Bulge Oscillation Driven by Outflows of Active Galactic Nuclei. I. Fast Outflow Case
Published 2025-01-01Subjects: Get full text
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192
The holographic landscape of symmetric product orbifolds
Published 2020-01-01Subjects: Get full text
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193
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Weak gravity conjecture validation with photon spheres of quantum corrected Reissner–Nordstrom–AdS black holes in Kiselev spacetime
Published 2025-02-01“…Abstract In this study, we investigate the Weak Gravity Conjecture (WGC) in the context of quantum-corrected Reissner–Nordstrom–AdS (RN-AdS) black holes within Kiselev spacetime. Our focus is on photon spheres, which serve as markers for stable and unstable photon spheres. …”
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195
A 22 Billion M⊙ Black Hole in Holmberg 15A with Keck KCWI Spectroscopy and Triaxial Orbit Modeling
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196
Central AdS Generalized Ay{\'o}n-Beato-Garc{\'\i}a Black Holes and Joule-Thomson Expansion
Published 2022-10-01Subjects: “…nonsingular black holes…”
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197
Optical features and thermal properties of charged AdS Euler–Heisenberg black hole surrounded by perfect fluid dark matter
Published 2025-02-01“…Finally, we extend our study to the optical features of the charged Euler–Heisenberg black hole surrounded by perfect fluid dark matter, such as the black hole shadow and energy emission rate and observe the impact of the coupling parameter.…”
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198
Unveiling the Emission Mechanisms of Blazar PKS 1510−089. II. Jet−BLR Connection and Black Hole Mass Estimation
Published 2025-01-01Subjects: Get full text
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199
Semianalytical Fokker–Planck Models for Nuclear Star Clusters
Published 2025-01-01Subjects: Get full text
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200
Perfect Fluid Dark Matter Influence on Thermodynamics and Phase Transition for a Reissner-Nordstrom-Anti-de Sitter Black Hole
Published 2019-01-01“…Based on Reissner-Nordstrom-anti-de Sitter(RN-AdS) black hole surrounded by perfect fluid dark matter, we study the thermodynamics and phase transition by extending the phase space defined by the charge square Q2 and the conjugate quantity ψ, where ψ is a function of horizon radius. …”
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