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Physics

arXiv preprints from January 1, 2026 through September 8, 2026 — 00:15:25 EST

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Posted in physics.flu-dyn · 2026-01-15 · Mohan Padmanabha, Jörg Kuhnert, Nicolas R. Gauger, Pratik Suchde

Boundary treatment algorithms for meshfree RANS turbulence modeling

In this paper, we propose improved wall-treatment strategies for meshfree methods applied to turbulent flows. The goal is to enhance wall-function handling in simulations of high-Reynolds-number turbulent flows and to understand the performance of turbulence models within these frameworks. While wall-function techniques are well...

💬 0 commentsarXiv:2601.10661v2PDF
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Posted in quant-ph · 2026-01-15 · Georgios Theologou, Mikkel F. Andersen, Sandro Wimberger

Counterdiabatic driving for random-gap Landau-Zener transitions

The Landau--Zener (LZ) model describes a two-level quantum system that undergoes an avoided crossing. In the adiabatic limit, the transition probability vanishes. An auxiliary control field $H_\text{CD}$ can be reverse-engineered so that the full Hamiltonian $H_0 + H_\text{CD}$ reproduces adiabaticity for all parameter values. Our aim...

💬 0 commentsarXiv:2601.10659v1PDF
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Posted in physics.soc-ph · 2026-01-15 · Joseph Uguet, Nicola Tollin, Jordi Morato

Transforming Crises into Opportunities: From Chaos to Urban Antifragility

Urban crises - floods, pandemics, economic shocks, and conflicts - function as accelerators of urban change, exposing structural vulnerabilities while creating windows for reinvention. Building on a prior theoretical contribution that identified fifteen principles of urban antifragility, this paper tests and operationalizes the...

💬 0 commentsarXiv:2601.10658v1PDF
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Posted in quant-ph · 2026-01-15 · Carlo Cafaro, James Schneeloch

Symmetry-Based Perspectives on Hamiltonian Quantum Search Algorithms and Schrodinger's Dynamics between Orthogonal States

It is known that the continuous-time variant of Grover's search algorithm is characterized by quantum search frameworks that are governed by stationary Hamiltonians, which result in search trajectories confined to the two-dimensional subspace of the complete Hilbert space formed by the source and target states. Specifically, the...

💬 0 commentsarXiv:2601.10655v2PDF
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Posted in quant-ph · 2026-01-15 · M. P. Tonne, Kh. P. Gnatenko

Quantifying the properties of evolutionary quantum states of the XXZ spin model using quantum computing

The entanglement distance of evolutionary quantum states of a two-spin system with the XXZ model has been studied. The analysis has been conducted both analytically and using quantum computing. An analytical dependence of the entanglement distance on the values of the model coupling constants and the parameters of the initial states...

💬 0 commentsarXiv:2601.10650v2PDF
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Posted in cond-mat.stat-mech · 2026-01-15 · Rupak Majumder, Shamik Gupta

Synchronization with Annealed Disorder and Higher-Harmonic Interactions in Arbitrary Dimensions: When Two Dimensions Are Special

The impact of disorder on collective phenomena depends crucially on whether it is quenched or annealed. In synchronization problems, quenched disorder in higher dimensional Kuramoto models is known to produce unconventional dimensional effects, including a striking odd even dichotomy: synchronization transitions are continuous in even...

💬 0 commentsarXiv:2601.10646v1PDF
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Posted in astro-ph.GA · 2026-01-15 · Ksenia I. Smirnova, Dmitri S. Wiebe

HII regions in NGC 628: the view of two catalogs

The study is devoted to comparing the parameters of the interstellar medium of HII regions in the Kongiu and Groves catalogs for the galaxy NGC 628. The article analyzes the characteristics of star-forming regions, including a comparison of radiation fluxes in the ranges of 7.7 $μ$m and 21 $μ$m and in the H$α$, H$β$, OIII and CO...

💬 0 commentsarXiv:2601.10642v1PDF
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Posted in astro-ph.CO · 2026-01-15 · R. M. Sullivan, E. Gjerløw, M. Galloway, D. J. Watts, R. Aurvik, A. Basyrov, L. A. Bianchi, A. Bonato, M. Brilenkov, H. K. Eriksen, U. Fuskeland, K. A. Glasscock, L. T. Hergt, D. Herman, J. G. S. Lunde, A. I. Silva Martins, M. San, D. Sponseller, N. -O. Stutzer, H. Thommesen, V. Vikenes, I. K. Wehus, L. Zapelli

Cosmoglobe DR2. VI. Disentangling hot and cold thermal dust emission with Planck HFI

We present a four-component high-resolution model of thermal dust emission for microwave and sub-mm frequencies derived from Planck HFI, WHAM and Gaia. The resulting high-resolution model derived here forms the basis for the thermal dust model employed in the Cosmoglobe DR2 reanalysis of COBE-DIRBE. The four dust components are called...

💬 0 commentsarXiv:2601.10640v1PDF
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Posted in cond-mat.mes-hall · 2026-01-15 · Rinsuke Yamada, Daichi Kurebayashi, Yukako Fujishiro, Shun Okumura, Daisuke Nakamura, Fehmi S. Yasin, Taro Nakajima, Tomoyuki Yokouchi, Akiko Kikkawa, Yasujiro Taguchi, Yoshinori Tokura, Oleg A. Tretiakov, Max Hirschberger

Emergent electric field induced by dissipative sliding dynamics of domain walls in a Weyl magnet

The dynamic motion of topological defects in magnets induces an emergent electric field, as exemplified by the continuous flow of skyrmion vortices. However, the electrodynamics underlying this emergent field remains poorly understood. In this context, magnetic domain walls - one dimensional topological defects with two collective...

💬 0 commentsarXiv:2601.10638v1PDF
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Posted in astro-ph.SR · 2026-01-15 · Zihao Yang, Sarah Gibson, Matthias Rempel, Giuliana de Toma

Measuring the Coronal Magnetic Field with 2D Coronal Seismology: A Forward-Modeling Validation

In recent years, a two-dimensional (2D) coronal seismology technique applied to spectral-imaging data from the Coronal Multi-channel Polarimeter (CoMP) and UCoMP has enabled routine measurement of the global coronal magnetic field. The technique combines coronal transverse wave phase speed from Doppler measurements with electron...

💬 0 commentsarXiv:2601.10637v1PDF
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Posted in cond-mat.stat-mech · 2026-01-15 · Damián H. Zanette, Eric A. Rozán

Exact and Approximate Constants of Motion in Stochastic Contact Processes

We study a variety of stochastic contact processes -- directly related to models of rumor and disease spreading -- from the viewpoint of their constants of motion, either exact or approximated. Much as in deterministic systems, constants of motion in stochastic dynamics make it possible to reduce the number of relevant variables,...

💬 0 commentsarXiv:2601.10776v1PDF
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Posted in astro-ph.SR · 2026-01-15 · R. Wesson, J. E. Drew, M. J. Barlow, J. García-Rojas, R. Greimel, D. Jones, A. Manchado, R. A. H. Morris, A. Zijlstra, P. J. Storey, J. A. L. Aguerri, S. R. Berlanas, E. Carrasco, G. B. Dalton, E. Gafton, R. García-Benito, A. L. González-Morán, B. Gänsicke, S. Hughes, S. Jin, R. Raddi, R. Sanchez-Janssen, E. Schallig, D. J. B. Smith, S. C. Trager, N. A. Walton

WEAVE imaging spectroscopy of NGC 6720: an iron bar in the Ring

We present spatially resolved spectroscopic observations of the planetary nebula NGC 6720, the Ring Nebula, taken during the science verification phase of WEAVE, a new instrument mounted on the William Herschel Telescope on La Palma. We use the instrument's Large Integral Field Unit (LIFU) to obtain spectra of the Ring Nebula,...

💬 0 commentsarXiv:2601.10635v1PDF
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Posted in hep-ph · 2026-01-15 · Indrani Nilima, Mujeeb Hasan, Mohammad Yousuf Jamal, Salman Ahamad Khan, B. K. Singh

Medium-Induced Quarkonium Dissociation at Finite Chemical Potential and Weak Magnetic Field

We investigate the in-medium modification and dissociation of heavy quarkonium in a hot QCD medium at finite quark chemical potential and in the weak magnetic-field regime. Starting from the one-loop resummed gluon propagator in the imaginary-time formalism, and incorporating non-perturbative effects through a phenomenological...

💬 0 commentsarXiv:2601.10634v1PDF
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Posted in cond-mat.mes-hall · 2026-01-15 · Hagen Gress, Cody L. Ritt, Inal Shomakhov, Kaan Altmisdort, Michelle Quien, Zitang Wei, John R. Lawall, Narasimha Boddeti, Michael S. Strano, J. Scott Bunch, Kamil L. Ekinci

Molecularly Thin Polyaramid Nanomechanical Resonators

Two-dimensional polyaramids exhibit strong hydrogen bonding to create molecularly thin nanosheets analogous to graphene. Here, we report the first nanomechanical resonators made out of a two-dimensional polyaramid, 2DPA-1, with thicknesses as small as 8 nm. To fabricate these molecular-scale resonators, we transferred nanofilms of...

💬 0 commentsarXiv:2601.10633v2PDF
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Posted in astro-ph.EP · 2026-01-15 · Andres F. Izquierdo, Jaehan Bae, Maria Galloway-Sprietsma, Ewine F. van Dishoeck, Stefano Facchini, Giovanni Rosotti, Jochen Stadler, Myriam Benisty, Leonardo Testi

Circumplanetary Disk Candidate in the Disk of HD 163296 Traced by Localized Emission from Simple Organics

Atacama Large Millimeter/submillimeter Array observations suggest that the disc of HD 163296 is being actively shaped by embedded, yet unseen protoplanets, as indicated by numerous gas and dust substructures consistent with planet-disc interaction models. We report the first detection of simple organic molecules, HCN and C2H, tracing...

💬 0 commentsarXiv:2601.10631v1PDF
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Posted in gr-qc · 2026-01-15 · Rajdeep Mazumdar, Kalyan Malakar, Kalyan Bhuyan

Dynamics of Late time cosmology in $f(Q,L_{m})$ Gravity with Constraints from DESI DR2 BAO Data

We investigate late-time cosmology in the context of modified $f(Q,L_m)$ gravity, considering a non-linear model$ f(Q,L_m) = αQ + βL_m^n + λ$ where, $α$, $β$, $λ$, and $n$ are some free parameters. The modified Friedmann equations are derived for a barotropic cosmic fluid, and an analytical solution for the Hubble parameter $H(z)$ is...

💬 0 commentsarXiv:2601.10627v1PDF
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Posted in math-ph · 2026-01-15 · Pavel Drozdov, Giorgio Gubbiotti, Danilo Latini

Discrete-time maximally superintegrable systems and deformed symmetry algebras: the Calogero-Moser case

We determine the complete structure of the symmetry algebras associated with the N-body Calogero-Moser system and its maximally superintegrable discretization. We prove that the discretization naturally leads to a nontrivial deformation of the continuous symmetry algebra, with the discretization parameter playing the rôle of a...

💬 0 commentsarXiv:2601.10625v2PDF
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Posted in hep-ph · 2026-01-15 · Yu-Han Ni, Chao Wu, Jiang-Hao Yu

Massless-Massive Amplitude Correspondence II: Constructive Massive Amplitudes in Standard Model

In the minimal helicity-chirality formalism, we systematically construct higher-point massive amplitudes from the fundamental building blocks: the contact three-point and four-point massive amplitudes. The inclusion of four-point contact amplitudes is essential to maintain gauge invariance in the spontaneously broken Standard Model....

💬 0 commentsarXiv:2601.10622v1PDF
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Posted in hep-ph · 2026-01-15 · Yu-Han Ni, Chao Wu, Jiang-Hao Yu

Massless-Massive Amplitude Correspondence I: Helicity-chirality Matching and On-shell Higgsing

In this work, the massless-massive correspondence for the on-shell scattering amplitudes is constructed so the massive amplitudes could inherit advantageous techniques developed in the massless calculation. This correspondence is established by matching massless amplitudes to Minimal Helicity-Chirality (MHC) amplitudes, which arise...

💬 0 commentsarXiv:2601.10620v1PDF
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Posted in cond-mat.str-el · 2026-01-15 · Karol I. Wysokiński, Marcin M. Wysokiński

Beyond Hubbard: the role of correlated hopping interaction in superconductors and quantum dot devices

We investigate the role of strong Coulomb interactions beyond the standard Hubbard model in two distinct physical contexts. First, we analyze the superconducting phase transition occurring near the Mott metal-insulator transition. Second, we study transport properties of artificial nano-scale structures containing quantum dots coupled...

💬 0 commentsarXiv:2601.10619v1PDF
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Posted in astro-ph.HE · 2026-01-15 · Kratika Mazde, Angelo Ricarte, George N. Wong

On the Physical Origins of the Millimeter Fundamental Plane in Active Galactic Nuclei

Observations of active galactic nuclei have revealed a correlation between millimeter luminosity, X-ray luminosity, and mass, suggesting the emission in each of these bands is powered by a common source. Starting with a set of five general relativistic magnetohydrodynamic simulations with dynamically important magnetic fields, we...

💬 0 commentsarXiv:2601.10612v1PDF
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Posted in physics.ao-ph · 2026-01-15 · Axel Seifert, Christoph Siewert, Fabian Jakub, Leonie von Terzi, Stefan Kneifel

On the geometry of aggregate snowflakes

Snowflakes play a crucial role in weather and climate. A significant portion of precipitation that reaches the surface originates as ice, even when it ultimately falls as rain. Contrary to the popular image of symmetric, dendritic crystals, most large snowflakes are irregular aggregates formed through the collision of primary ice...

💬 0 commentsarXiv:2601.10608v1PDF
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Posted in hep-th · 2026-01-15 · Reiko Liu, Wen-Jie Ma

Unifying soft and hard dynamics: The hard current algebra in celestial holography

Soft current algebras capture the infrared structure of scattering in asymptotically flat spacetimes, but an analogous algebraic description of finite-energy dynamics has been missing. We uncover an infinite-dimensional hard current algebra that encodes finite-energy contributions to scattering and implies novel Ward identities. The...

💬 0 commentsarXiv:2601.10601v1PDF
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Posted in astro-ph.EP · 2026-01-15 · John H. Livingston, Erik A. Petigura, Trevor J. David, Kento Masuda, James Owen, David Nesvorný, Konstantin Batygin, Jerome de Leon, Mayuko Mori, Kai Ikuta, Akihiko Fukui, Noriharu Watanabe, Jaume Orell Miquel, Felipe Murgas, Hannu Parviainen, Judith Korth, Florence Libotte, Néstor Abreu García, Pedro Pablo Meni Gallardo, Norio Narita, Enric Pallé, Motohide Tamura, Atsunori Yonehara, Andrew Ridden-Harper, Allyson Bieryla, Alessandro A. Trani, Eric E. Mamajek, David R. Ciardi, Varoujan Gorjian, Lynne A. Hillenbrand, Luisa M. Rebull, Elisabeth R. Newton, Andrew W. Mann, Andrew Vanderburg, Guðmundur Stefánsson, Suvrath Mahadevan, Caleb Cañas, Joe Ninan, Jesus Higuera, Kamen Todorov, Jean-Michel Désert, Lorenzo Pino

A young progenitor for the most common planetary systems in the Galaxy

The Galaxy's most common known planetary systems have several Earth-to-Neptune-size planets in compact orbits. At small orbital separations, larger planets are less common than their smaller counterparts by an order of magnitude. The young star V1298 Tau hosts one such compact planetary system, albeit with four planets that are...

💬 0 commentsarXiv:2601.10598v1PDF
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Posted in hep-ex · 2026-01-15 · BESIII Collaboration, M. Ablikim, M. N. Achasov, P. Adlarson, X. C. Ai, R. Aliberti, A. Amoroso, Q. An, Y. Bai, O. Bakina, Y. Ban, H. -R. Bao, V. Batozskaya, K. Begzsuren, N. Berger, M. Berlowski, M. B. Bertani, D. Bettoni, F. Bianchi, E. Bianco, A. Bortone, I. Boyko, R. A. Briere, A. Brueggemann, H. Cai, M. H. Cai, X. Cai, A. Calcaterra, G. F. Cao, N. Cao, S. A. Cetin, X. Y. Chai, J. F. Chang, T. T. Chang, G. R. Che, Y. Z. Che, C. H. Chen, Chao Chen, G. Chen, H. S. Chen, H. Y. Chen, M. L. Chen, S. J. Chen, S. M. Chen, T. Chen, X. R. Chen, X. T. Chen, X. Y. Chen, Y. B. Chen, Y. Q. Chen, Z. K. Chen, J. C. Cheng, L. N. Cheng, S. K. Choi, X. Chu, G. Cibinetto, F. Cossio, J. Cottee-Meldrum, H. L. Dai, J. P. Dai, X. C. Dai, A. Dbeyssi, R. E. de Boer, D. Dedovich, C. Q. Deng, Z. Y. Deng, A. Denig, I. Denisenko, M. Destefanis, F. De Mori, X. X. Ding, Y. Ding, Y. X. Ding, J. Dong, L. Y. Dong, M. Y. Dong, X. Dong, M. C. Du, S. X. Du, S. X. Du, X. L. Du, Y. Y. Duan, Z. H. Duan, P. Egorov, G. F. Fan, J. J. Fan, Y. H. Fan, J. Fang, J. Fang, S. S. Fang, W. X. Fang, Y. Q. Fang, L. Fava, F. Feldbauer, G. Felici, C. Q. Feng, J. H. Feng, L. Feng, Q. X. Feng, Y. T. Feng, M. Fritsch, C. D. Fu, J. L. Fu, Y. W. Fu, H. Gao, Y. Gao, Y. N. Gao, Y. N. Gao, Y. Y. Gao, Z. Gao, S. Garbolino, I. Garzia, L. Ge, P. T. Ge, Z. W. Ge, C. Geng, E. M. Gersabeck, A. Gilman, K. Goetzen, J. D. Gong, L. Gong, W. X. Gong, W. Gradl, S. Gramigna, M. Greco, M. D. Gu, M. H. Gu, C. Y. Guan, A. Q. Guo, J. N. Guo, L. B. Guo, M. J. Guo, R. P. Guo, X. Guo, Y. P. Guo, A. Guskov, J. Gutierrez, T. T. Han, F. Hanisch, K. D. Hao, X. Q. Hao, F. A. Harris, C. Z. He, K. L. He, F. H. Heinsius, C. H. Heinz, Y. K. Heng, C. Herold, P. C. Hong, G. Y. Hou, X. T. Hou, Y. R. Hou, Z. L. Hou, H. M. Hu, J. F. Hu, Q. P. Hu, S. L. Hu, T. Hu, Y. Hu, Z. M. Hu, G. S. Huang, K. X. Huang, L. Q. Huang, P. Huang, X. T. Huang, Y. P. Huang, Y. S. Huang, T. Hussain, N. Hüsken, N. in der Wiesche, J. Jackson, Q. Ji, Q. P. Ji, W. Ji, X. B. Ji, X. L. Ji, X. Q. Jia, Z. K. Jia, D. Jiang, H. B. Jiang, P. C. Jiang, S. J. Jiang, X. S. Jiang, Y. Jiang, J. B. Jiao, J. K. Jiao, Z. Jiao, S. Jin, Y. Jin, M. Q. Jing, X. M. Jing, T. Johansson, S. Kabana, N. Kalantar-Nayestanaki, X. L. Kang, X. S. Kang, M. Kavatsyuk, B. C. Ke, V. Khachatryan, A. Khoukaz, O. B. Kolcu, B. Kopf, L. Kröger, M. Kuessner, X. Kui, N. Kumar, A. Kupsc, W. Kühn, Q. Lan, W. N. Lan, T. T. Lei, M. Lellmann, T. Lenz, C. Li, C. Li, C. H. Li, C. K. Li, D. M. Li, F. Li, G. Li, H. B. Li, H. J. Li, H. L. Li, H. N. Li, Hui Li, J. R. Li, J. S. Li, J. W. Li, K. Li, K. L. Li, L. J. Li, Lei Li, M. H. Li, M. R. Li, P. L. Li, P. R. Li, Q. M. Li, Q. X. Li, R. Li, S. X. Li, Shanshan Li, T. Li, T. Y. Li, W. D. Li, W. G. Li, X. Li, X. H. Li, X. K. Li, X. L. Li, X. Y. Li, X. Z. Li, Y. Li, Y. G. Li, Y. P. Li, Z. H. Li, Z. J. Li, Z. X. Li, Z. Y. Li, C. Liang, H. Liang, Y. F. Liang, Y. T. Liang, G. R. Liao, L. B. Liao, M. H. Liao, Y. P. Liao, J. Libby, A. Limphirat, D. X. Lin, L. Q. Lin, T. Lin, B. J. Liu, B. X. Liu, C. X. Liu, F. Liu, F. H. Liu, Feng Liu, G. M. Liu, H. Liu, H. B. Liu, H. H. Liu, H. M. Liu, Huihui Liu, J. B. Liu, J. J. Liu, K. Liu, K. Liu, K. Y. Liu, Ke Liu, L. Liu, L. C. Liu, Lu Liu, M. H. Liu, P. L. Liu, Q. Liu, S. B. Liu, W. M. Liu, W. T. Liu, X. Liu, X. K. Liu, X. L. Liu, X. Y. Liu, Y. Liu, Y. Liu, Y. B. Liu, Z. A. Liu, Z. D. Liu, Z. Q. Liu, Z. Y. Liu, X. C. Lou, H. J. Lu, J. G. Lu, X. L. Lu, Y. Lu, Y. H. Lu, Y. P. Lu, Z. H. Lu, C. L. Luo, J. R. Luo, J. S. Luo, M. X. Luo, T. Luo, X. L. Luo, Z. Y. Lv, X. R. Lyu, Y. F. Lyu, Y. H. Lyu, F. C. Ma, H. L. Ma, Heng Ma, J. L. Ma, L. L. Ma, L. R. Ma, Q. M. Ma, R. Q. Ma, R. Y. Ma, T. Ma, X. T. Ma, X. Y. Ma, Y. M. Ma, F. E. Maas, I. MacKay, M. Maggiora, S. Malde, Q. A. Malik, H. X. Mao, Y. J. Mao, Z. P. Mao, S. Marcello, A. Marshall, F. M. Melendi, Y. H. Meng, Z. X. Meng, G. Mezzadri, H. Miao, T. J. Min, R. E. Mitchell, X. H. Mo, B. Moses, N. Yu. Muchnoi, J. Muskalla, Y. Nefedov, F. Nerling, H. Neuwirth, Z. Ning, S. Nisar, Q. L. Niu, W. D. Niu, Y. Niu, C. Normand, S. L. Olsen, Q. Ouyang, S. Pacetti, X. Pan, Y. Pan, A. Pathak, Y. P. Pei, M. Pelizaeus, H. P. Peng, X. J. Peng, Y. Y. Peng, K. Peters, K. Petridis, J. L. Ping, R. G. Ping, S. Plura, V. Prasad, F. Z. Qi, H. R. Qi, M. Qi, S. Qian, W. B. Qian, C. F. Qiao, J. H. Qiao, J. J. Qin, J. L. Qin, L. Q. Qin, L. Y. Qin, P. B. Qin, X. P. Qin, X. S. Qin, Z. H. Qin, J. F. Qiu, Z. H. Qu, J. Rademacker, C. F. Redmer, A. Rivetti, M. Rolo, G. Rong, S. S. Rong, F. Rosini, Ch. Rosner, M. Q. Ruan, N. Salone, A. Sarantsev, Y. Schelhaas, K. Schoenning, M. Scodeggio, W. Shan, X. Y. Shan, Z. J. Shang, J. F. Shangguan, L. G. Shao, M. Shao, C. P. Shen, H. F. Shen, W. H. Shen, X. Y. Shen, B. A. Shi, H. Shi, J. L. Shi, J. Y. Shi, S. Y. Shi, X. Shi, H. L. Song, J. J. Song, M. H. Song, T. Z. Song, W. M. Song, Y. X. Song, Zirong Song, S. Sosio, S. Spataro, S. Stansilaus, F. Stieler, S. S Su, G. B. Sun, G. X. Sun, H. Sun, H. 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Search for sub-GeV dark particles in $η\toπ^0+\rm{invisible}$ decay

Using (10087$\pm$44)$\times$10$^{6}$ $J/ψ$ events collected with the BESIII detector at the BEPCII collider at the center-of-mass energy of $\sqrt{s}=3.097~\rm{GeV}$, we report the first search for $η\toπ^0S\toπ^0χ\barχ$ with $S$ denotes an on-shell dark scalar boson and $χ$ an invisible dark matter particle. No significant signals...

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