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๐Ÿ” haim avron ๐Ÿ“‚ Physics
Showing 2080 results for "haim avron" in Physics
Physics Preprint PDF DOI

A No-Cloning Trade-off Between Black Hole No-Hair and Horizon Smoothness

Sudhanva Joshi, Sunil Kumar Mishra ยท 2026

The black hole no-hair theorem is traditionally derived from the uniqueness theorems of general relativity. We show that a quantitative form follows from unitarity together with the standard semiclassโ€ฆ

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Spin-Induced Nonlinear Scalarization of Kerr Black Holes in Einstein-scalar-Gauss-Bonnet Gravity

Meng-Yun Lai, Hyat Huang, Jutta Kunz, Yun Soo Myung, De-Cheng Zou ยท 2026

We investigate spin-induced scalarization of Kerr black holes in an Einstein-scalar-Gauss-Bonnet (EsGB) model that does not admit a linear tachyonic instability of the scalar-free solution. The scalarโ€ฆ

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Thermodynamic Phase Transitions in Einstein-Maxwell-Scalar-Gauss-Bonnet Gravity

Cristian Erices, Stella Kiorpelidi ยท 2026

Although asymptotically flat black holes generically lack thermodynamic phase transitions, we show that curvature-induced scalarization of electrically charged black holes in Einstein-Maxwell- Scalar-โ€ฆ

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Physics Preprint PDF DOI

Spontaneous spherical symmetry breaking of black holes with resonant hair

Jose Ferreira, Carlos A. R. Herdeiro, Eugen Radu, Miguel Zilhao ยท 2026

Black holes with resonant hair are static, spherical, electrically charged solutions of the Einstein-Maxwell-(gauged-)scalar system. Scalar self-interactions are mandatory for their existence. Initialโ€ฆ

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Physics Preprint PDF DOI

Shadow dependent phenomenology framework for rotating black hole metric

Nikko John Leo S. Lobos, Emmanuel T. Rodulfo ยท 2026

We establish a thermodynamic-optical duality that directly bridges the semiclassical quantum evaporation of black holes with their classical macroscopic geometry. By employing a diffeomorphic inversioโ€ฆ

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Time Like Geodesics of Regular Black Holes with Scalar Hair

P. A. Gonzalez, Marco Olivares, Eleftherios Papantonopoulos, Yerko Vasquez ยท 2026

We investigate timelike geodesics in asymptotically flat regular black holes supported by a phantom scalar field characterized by a scalar charge $A$. This parameter removes the central singularity anโ€ฆ

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Gyrokinetic simulations on zonal flow-turbulence spreading coupling

Min Ki Jung, Sumin Yi, Taik Soo Hahm, Yong-Su Na ยท 2026

Zonal flows and turbulence spreading play important roles in magnetic fusion plasma confinement, yet their coupling mechanisms remain elusive. Using global nonlinear gyrokinetic simulations, we show tโ€ฆ

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Geometrically Regular Black Holes with Hedgehog Scalar Hair

Sebastian Bahamonde ยท 2026

We study a simple theory based on general relativity, minimally coupled to a constrained scalar triplet and to an auxiliary non-propagating three-form sector. Within a spherically symmetric hedgehog aโ€ฆ

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Physics Preprint PDF DOI

A First-Order Eikonal Framework for Quasinormal Modes, Shadows, Strong Lensing, and Grey-Body Factors in a Scalarized Black-Hole Metric

Bekir Can Lutfuoglu, Javlon Rayimbaev, Sardor Murodov, Jakhongir Kurbanov, Muhammad Matyoqubov ยท 2026

We construct an analytic geodesic-optics description of quasinormal ringing, black-hole shadows, strong lensing, and grey-body factors for the static spherical metric introduced in Eq.~(9) of Ref.~\ciโ€ฆ

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Thermodynamics of Chern-Simons AdS$_5$ black holes coupled to $\mathrm{SU}(2)$ solitons

Laura Andrianopoli, Dusan {DJ}or{dj}evic, Olivera Miskovic ยท 2026

We investigate properties of the five-dimensional Chern--Simons AdS black hole coupled to $\mathrm{SU}(2)$ solitons by means of a minisuperspace approximation adapted to static, spherically symmetric โ€ฆ

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Rotating Thin Shells in Einstein-Gauss-Bonnet Gravity

Joao D. Alvares, Tiago V. Fernandes ยท 2026

A rotating metric solution in Einstein-Gauss-Bonnet gravity with a negative cosmological constant was recently found in the Chern-Simons point. We construct a rotating thin shell gluing two spacetimesโ€ฆ

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Phase Transitions in Primary Hair Planar Black Holes and Solitons

Som Abhisek Mohanty, Subhash Mahapatra ยท 2026

We present a new family of Ricci-flat black hole and soliton solutions with primary scalar hair in asymptotically anti-de Sitter (AdS) space in $D$ dimensions. By solving the coupled Einstein-scalar fโ€ฆ

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Nonlinear response of soft hair beds to Poiseuille flows

Mani Sai Suryateja Jammalamadaka, Jonas Smucker, Jose R Alvarado ยท 2026

Biological surfaces with micrometer-scale protrusions, such as microvilli, crustacean hairs, and cilia, often interact with pressure-driven fluid flow, resulting in a two-way elastoviscous problem. Chโ€ฆ

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Axial gravitational perturbations and echo-like signals of a hairy black hole from gravitational decoupling

Yi Yang, Ali Ovgun, Gaetano Lambiase, Dong Liu, Zheng-Wen Long ยท 2026

We study axial gravitational perturbations of a hairy black hole constructed in the framework of gravitational decoupling and investigate the geometric origin of echo-like late-time signals in this spโ€ฆ

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Effects of Schwarzschild's Black Hole Singularities on Complex Scalar Field

Z.E. Musielak, J.L. Fry, G.W. Kanan ยท 2026

Complex scalar fields described by a novel Klein-Gordon equation derived from gauge and group theories are considered at the Schwarzschild's black hole singularities. It is shown that the field is welโ€ฆ

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Microscopic Origin of Page Curve

Artem Averin ยท 2026

Applications of the Ryu-Takayanagi formula to evaporating black holes are known to reproduce the Page curve, although leaving open the microscopic origin of the necessary black hole degrees of freedomโ€ฆ

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Extracting Energy from Magnetized Rotating Black Holes in Horndeski Gravity via the Magnetic Penrose Process

Ke Wang, Xiao-Xiong Zeng ยท 2026

In Horndeski gravity, we investigate how to extract energy from a rotating black hole immersed in a uniform magnetic field $B$ based on the Magnetic Penrose Process. We map the ergosphere and negativeโ€ฆ

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No hair but plenty of feathers: are birds black holes?

Andrew Laeuger, Taylor Knapp ยท 2026

The imitative verb "chirp" is thought to originate from 16th-century Middle English. Meanwhile, this same word has been used to describe the gravitational waves (GWs) emitted from the merger of compacโ€ฆ

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Geometry of the Ising persistence problem and the universal Bonnet-Manin Painlev\'e VI distribution

Ivan Dornic, Robert Conte ยท 2026

We determine the full persistence probability distribution for a non-Markovian stochastic process, motivated by first-passage questions arising in interacting spin systems and allied systems. We show โ€ฆ

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Open-System Adiabatic Quantum Search under Dephasing

Afaf El Kalai, Peter J. Eder, Christian B. Mendl ยท 2026

Adiabatic quantum algorithms must evolve slowly enough to suppress non-adiabatic transitions while remaining fast enough to be practical. In open systems, this trade-off is reshaped by decoherence. Foโ€ฆ

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