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๐Ÿ” omar khadir ๐Ÿ“‚ Physics
Showing 1127 results for "omar khadir" in Physics
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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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Benchmarking Universal Machine-Learned Interatomic Potentials for High-Temperature Metal-Organic Framework Chemistry

Connor W. Edwards, Jack D. Evans ยท 2026

Universal machine-learned interatomic potentials (uMLIPs) offer a promising approach to performing atomistic simulations at near-DFT accuracy with greatly reduced computational cost. Here, we present โ€ฆ

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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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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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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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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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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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A Covariant Phase Space Approach to Einstein-AEther Gravity

Walter Arata, Stefano Liberati, Giulio Neri ยท 2026

Black hole thermodynamics in Lorentz-violating gravity is subtle because different excitations propagate at different speeds and hence identify different causal horizons. We revisit Einstein--AEther gโ€ฆ

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Mercury Craters Named after Tajik-Persian Poets: Planetary Nomenclature as a Form of Preserving Cultural Heritage

Rizoi Bakhromzod ยท 2026

Nine impact craters on Mercury bear the names of Persian-Tajik poets: Rudaki, Saadi, Nizami, Rumi, Navoi, Firdousi, Hafiz, Sanai, and Mahsati. We compile IAU-approved coordinates, diameters, quadrant โ€ฆ

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Extracting $B_s\to D_s^*\ell\nu_\ell$ form factors

Anastasia Boushmelev, Matthew Black, Oliver Witzel ยท 2026

Semileptonic $B_{(s)}$ decays are of great phenomenological interest because they allow to determine e.g. CKM matrix elements or test lepton flavor universality. Taking advantage of already existing lโ€ฆ

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An effective cosmological constant as black hole primary hair

Christos Charmousis, Pedro G. S. Fernandes, Mokhtar Hassaine ยท 2026

We study Generalized Proca theories inspired by the recent regularised Proca theory of four-dimensional Gauss-Bonnet gravity. By abandoning the rigid constraints typically imposed by specific regulariโ€ฆ

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Stable black hole solutions with cosmological hair

Laurens Smulders, Johannes Noller ยท 2026

Dynamical dark energy theories generically introduce a time-dependent field that causes the accelerated expansion of the Universe on large scales. When embedding black hole solutions in such a cosmoloโ€ฆ

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The Steep Price of No Hair in a Modified Loop Quantum Cosmology

Meysam Motaharfar, Parampreet Singh ยท 2026

A specific loop quantum cosmology model, mLQC-I, motivated by Thiemann's regularization of the Hamiltonian constraint, leads to the resolution of the big bang singularity and bounce in the isotropic sโ€ฆ

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More on near-horizon charges black holes with gravitational hair in three dimensions

Seyed Naseh Sajadi, Supakchai Ponglertsakul, Julio Oliva ยท 2026

With the aim of continuing the exploration of near-horizon charges in higher-curvature gravity, searching for sectors leading to universal behaviors, we first provide a thorough revision and formulae โ€ฆ

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Cosmic anisotropic hair of nonlocal RT gravity

Jiajun Zhou, Shuxun Tian, Zong-Hong Zhu ยท 2026

Nonlocal RT gravity has proven effective in explaining the late-time cosmic acceleration while remaining consistent with local gravity tests. However, most previous cosmological studies of this theoryโ€ฆ

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Local kinetic sensors for adaptive mesh and algorithm refinement

R. M. Strassle, S. A. Hosseini, I. V. Karlin ยท 2026

This paper presents novel refinement sensors for the application to adaptive mesh and algorithm refinement (AMAR) with kinetic models, such as discrete velocity and lattice Boltzmann methods. While reโ€ฆ

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Periodic Orbits and Gravitational Radiation from Extreme Mass-Ratio Inspirals as Probes of Black Hole Quantum Hair

Yiru Zhang, Meirong Tang, Zhaoyi Xu ยท 2026

The classical no-hair theorem states that stationary black holes in general relativity can be completely described by only a small set of global parameters. Within this framework, no additional geometโ€ฆ

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One-Dimensional Metallic Polymeric Nitrogen

Kewei Ding, Junyi Miao, Ying Liu, Anxin Yu, Cheng Lu, Wenrui Zhang, Yanchun Li, Haipeng Su, Zhongxue Ge, Xianlong Wang ยท 2026

The pressure-induced metallic states of light elements attract significant attention, because of potential applications as high-temperature superconductor and high-energy-density material, especially โ€ฆ

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$\sigma$ bands driven high-temperature superconductivity in hydrogenated hexagonal BC$_3$ monolayer

Guo Chen, Ru Zheng, Jin-Hua Sun, Fengjie Ma, Xun-Wang Yan, Miao Gao, Tian Cui, Zhong-Yi Lu ยท 2026

Material with metallic $\sigma$-bonding bands is expected to be a high-temperature superconductor, due to the sensitivity of $\sigma$ electrons to lattice vibration. Based on the first-principles calcโ€ฆ

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