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141
Exploring the Enigma of Particle Dynamics and Plasma Lensing Using Einstein–Euler–Heisenberg Black Hole Geometry
Published 2025-01-01Subjects: “…Einstein–Euler–Heisenberg black hole…”
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142
Particle motion and QPOs around Euler-Heisenberg black hole immersed in cold dark matter halo
Published 2025-03-01“…We explore the motion of particles in the vicinity of an Euler-Heisenberg black hole immersed in a cold dark matter halo, focusing on how the black hole parameters influence particle dynamics. …”
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143
Magnetic reconnection and energy extraction from a Konoplya–Zhidenko rotating non-Kerr black hole
Published 2025-01-01“…This means that in the Konoplya–Zhidenko rotating non-Kerr black hole spacetime one can extract more energy via magnetic reconnection than in the Kerr black hole case. …”
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144
Evolution of interior entropy of a loop quantum-corrected black hole pierced by a cosmic string
Published 2025-02-01“…The concept of interior entropy of black hole provides a possible way to deal with information problem. …”
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145
Star−Disk Collisions: Implications for Quasi-periodic Eruptions and Other Transients near Supermassive Black Holes
Published 2024-01-01Subjects: Get full text
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146
Quasinormal modes and GUP-corrected Hawking radiation of BTZ black holes within modified gravity frameworks
Published 2025-02-01“…The findings indicate that increasing mass and parameter values results in a raised potential barrier, implying stronger confinement of perturbations and impacting black hole stability. Incorporating the generalized uncertainty principle, we also study its effect on the thermodynamics of rotating BTZ black holes, demonstrating how GUP modifies black hole radiation, potentially observable in QNM decay rates. …”
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147
A Dual Active Black Hole Candidate with Mass Ratio ~7:1 in a Disk Galaxy
Published 2025-01-01“…Considering almost every massive galaxy is associated with multiple dwarf satellites around it, minor mergers involving galaxies with disproportional stellar masses should be much more common than major mergers, which would naturally lead to black hole (BH) pairs with significantly different masses. …”
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148
Gravitational odd-parity perturbation of a Horndeski hairy black hole: quasinormal mode and parameter constraint
Published 2025-01-01“…Abstract During the binary black hole coalescence, gravitational waves emitted at the ringdown stage can be well described by black hole perturbation theory, where the quasinormal modes (QNMs) become the important ingredient in modeling the pattern waveform. …”
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149
Hawking Radiation-Quasi-Normal Modes Correspondence and Effective States for Nonextremal Reissner-Nordström Black Holes
Published 2014-01-01“…It is known that the nonstrictly thermal character of the Hawking radiation spectrum harmonizes Hawking radiation with black hole (BH) quasi-normal modes (QNM). This paramount issue has been recently analyzed in the framework of both Schwarzschild BHs (SBH) and Kerr BHs (KBH). …”
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150
Multi-messenger probes of asteroid mass primordial black holes: Superradiance spectroscopy, Hawking radiation, and microlensing
Published 2025-02-01“…Superradiance provides a unique opportunity for investigating dark sectors as well as primordial black holes, which themselves are candidates for dark matter over a wide mass range. …”
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151
Understanding the Broad-line Region of Active Galactic Nuclei with Photoionization. I. The Moderate-accretion Regime
Published 2025-01-01Subjects: “…Black hole physics…”
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152
The Kramers escape rate of phase transitions for the 6-dimensional Gauss-Bonnet AdS black hole with triple phases
Published 2025-02-01“…One is a dynamic equilibrium of the transition from the medium black hole state to the large black hole state and the transition from the small black hole state to the medium black hole state. …”
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153
Uncovering Deterministic Behavior of Black Hole IGR J17091–3624: A Twin of GRS 1915+105
Published 2025-01-01Subjects: Get full text
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154
Maximally Localized States and Quantum Corrections of Black Hole Thermodynamics in the Framework of a New Generalized Uncertainty Principle
Published 2015-01-01“…On the other hand, in the framework of this new GUP we calculate quantum corrections to the thermodynamic quantities of the Schwardzschild black hole, such as the Hawking temperature, the entropy, and the heat capacity, and give a remnant mass of the black hole at the end of the evaporation process. …”
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155
Star shearing season: transient signals in wave-like dark matter experiments from black hole formation
Published 2025-02-01“…When these objects are turned into black holes due to a supernova or a binary merger this “hair” could be “shorn” off. …”
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156
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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157
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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158
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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159
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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160
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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