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Physics

arXiv preprints from January 1, 2026 through July 20, 2026 — 02:52:11 EST

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Posted in quant-ph · 2026-01-16 · Elias Pescoller, Santiago Beltrán-Romero, Sebastian Egginger, Nicolas Jungwirth, Martino Zanetti, Dominik Hornof, Michael S. Seifner, Iva Březinová, Philipp Haslinger, Thomas Juffmann, Johannes Kofler, Philipp Schindler, Dennis Rätzel

Coupling free electrons to a trapped-ion quantum computer

Freely propagating electrons may serve as quantum probes that can become coherently correlated with other quantum systems, offering access to advanced metrological resources. We propose a setup that coherently couples free electrons in an electron microscope to a trapped-ion quantum processor, enabling non-destructive,...

💬 0 commentsarXiv:2601.11446v1PDF
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Posted in physics.soc-ph · 2026-01-16 · Bilge Taskin, Teddy Lazebnik

An Epidemiological Modeling Take on Religion Dynamics

Religions are among the most consequential social institutions, shaping collective identities, moral norms, and political organization across societies and historical periods. Nevertheless, despite extensive scholarship describing conversion, competition, and secularization, there is still no widely adopted formal model that captures...

💬 0 commentsarXiv:2601.11436v1PDF
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Posted in astro-ph.GA · 2026-01-16 · Drew Lapeer, Daniela Calzetti, Kathryn Grasha, Angela Adamo, Bruce G. Elmegreen, Arjan Bik, Giacomo Bortolini, Anne Buckner, Michele Cignoni, Matteo Correntim, Debra Meloy Elmegreen, H. Faustino Vieira, Max Hamilton, Kelsey Johnson, Thomas S. -Y Lai, Sean T. Linden, Subhransu Maji, Matteo Messa, Göran Östlin, Alex Pedrini, E. Sabbi, Linda J. Smith

FEAST: Probing Hierarchical Star Formation with the Spatial Distributions of Young Star Clusters

We apply the angular two-point correlation function (TPCF) to the spatial distribution of young star clusters (YSCs) in four nearby star forming galaxies (NGC 628, NGC 4449, M51, and M83) in order to investigate their underlying hierarchical structuring. Using newly constructed catalogs of YSCs in the emerging phase (eYSCs),...

💬 0 commentsarXiv:2601.11434v1PDF
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Posted in cond-mat.soft · 2026-01-16 · G. C. Antunes, C. Obst, H. Stark

Confinement-induced motion of ciliates

The time dynamics of flagellar and ciliary beating is often neglected in theories of microswimmers, with the most common models prescribing a time-constant actuation of the surrounding fluid. By explicitly introducing a metachronal wave, coarse-grained to a sinusoidal surface slip velocity, we show that a spatial resonance between the...

💬 0 commentsarXiv:2601.11424v2PDF
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Posted in quant-ph · 2026-01-16 · Amit S. Patel, Himanshukumar R. Patel, Bikash K. Behera

Noisy-QSMOTE: Robustness Analysis of Quantum SMOTE under Quantum-Inspired Noise for Condition Monitoring and Fault Classification in Industrial and Energy Systems

Imbalanced datasets remain a major challenge in industrial condition monitoring and fault diagnosis, often causing machine-learning models to favor majority classes while underrepresenting minority fault conditions. This work investigates the Quantum Synthetic Minority Oversampling Technique (QSMOTE) through three stages: (i) baseline...

💬 0 commentsarXiv:2601.11423v2PDF
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Posted in quant-ph · 2026-01-16 · Mostafa Atallah, Alvin Gonzales, Daniel Dilley, Igor Gaidai, Zain H. Saleem, Rebekah Herrman

A matching decomposition algorithm for simulating quantum walk Hamiltonians

In this work, we present a new algorithm for generating quantum circuits that efficiently implement continuous time quantum walks on arbitrary simple sparse graphs. The algorithm, called matching decomposition, works by decomposing a continuous-time quantum walk Hamiltonian into a collection of exactly implementable Hamiltonians...

💬 0 commentsarXiv:2601.11418v3PDF
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Posted in physics.optics · 2026-01-16 · Sergey A. Ponomarenko, Morteza Hajati

Wigner picture of partially coherent accelerating beams

We advance a phase-space theory of partially coherent accelerating, non-diffracting beams employing the Wigner distribution function (WDF). We derive a general expression for the WDF of any accelerating, diffraction-free beam of arbitrary degree of spatial coherence and find an elegant closed-form expression for the WDF of such beam...

💬 0 commentsarXiv:2601.11416v1PDF
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Posted in astro-ph.IM · 2026-01-16 · Jose Sánchez Andreu

Zero-Shot Detection of Elastic Transient Morphology Across Physical Systems

We test whether a representation learned from interferometric strain transients in gravitational-wave observatories can act as a frozen morphology-sensitive operator for unseen sensors, provided the target signals preserve coherent elastic transient structure. Using a neural encoder trained exclusively on non-Gaussian instrumental...

💬 0 commentsarXiv:2601.11415v1PDF
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Posted in quant-ph · 2026-01-16 · Laia Domingo, Christine Johnson

Quantum-enhanced optimization for patient stratification in clinical trials

Clinical trials are notorious for their high failure rates and steep costs, leading to wasted time and resources spend, prolonged development timelines, and delayed patient access to new therapies. A key contributor to these failures is biological uncertainty, which complicates trial design and weakens the ability to detect true...

💬 0 commentsarXiv:2601.11413v1PDF
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Posted in physics.optics · 2026-01-16 · Igor Kuzmenko, Y. B. Band, Yshai Avishai, Marek Trippenbach

Hysteresis in the complex nonlinear refractive index of a homogeneous and isotropic medium

We calculate the permittivity, $ε(ω)$, for a medium with a quadratic electro-optic effect, modeling it as a Duffing oscillator. The nonlinear refractive index $n(ω, E(ω))$ and the nonlinear absorption coefficient $α(ω, E(ω))$ exhibit hysteresis when the light intensity is varied [here $E(ω)$ is the electric field strength at angular...

💬 0 commentsarXiv:2601.11411v1PDF
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Posted in physics.optics · 2026-01-16 · An Aloysius Wang, Yuxi Cai, Yifei Ma, Patrick S Salter, Chao He

Resolving topological obstructions to vectorial structured field control

The use of structured matter, such as optical retarders, for vectorial control is a well-established and widely employed technique in modern optics, and has driven continued advances in the manipulation of complex, spatially varying vectorial fields. However, achieving arbitrary field conversion typically requires the use of cascaded...

💬 0 commentsarXiv:2601.11410v1PDF
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Posted in astro-ph.EP · 2026-01-16 · Bennet Outland, Gretchen Noble, Andrew W. Smith, Jack J. Lissauer

Orbital Stability of Closely-Spaced Four-planet Systems

We investigate the orbital dynamics of four-planet systems consisting of Earth-mass planets on initially-circular, coplanar orbits around a star of one solar mass. In our simulations, the innermost planet's semimajor axis is set at 1 AU, with subsequent semimajor axes spaced equally in terms of planets' mutual Hill radii. Several sets...

💬 0 commentsarXiv:2601.11692v2PDF
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Posted in physics.optics · 2026-01-16 · An Aloysius Wang, Yuxi Cai, Zhenglin Li, Ruofu Liu, Yifei Ma, Patrick S Salter, Chao He

General in situ feedback control of cascaded liquid crystal spatial light modulators for structured field generation

Cascaded liquid crystal spatial light modulators provide a versatile strategy for the generation of structured light and matter fields, with applications including optical communications, photonic computing, and topological field engineering. However, experimental imperfections, such as temperature-dependent liquid crystal response,...

💬 0 commentsarXiv:2601.11405v1PDF
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Posted in physics.soc-ph · 2026-01-16 · Ixandra Achitouv, David Chavalarias, Raphael Fournier-S'niehotta

D-MODD: A Diffusion Model of Opinion Dynamics Derived from Online Data

We present the first empirical derivation of a continuous-time stochastic model for real-world opinion dynamics. Using longitudinal social-media data to infer users opinion on a binary climate-change topic, we reconstruct the underlying drift and diffusion functions governing individual opinion updates. We show that the observed...

💬 0 commentsarXiv:2601.16226v2PDF
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Posted in hep-ph · 2026-01-16 · Michael I. Eides, Vladimir A. Yerokhin

Energy levels of multiscale bound states from QED energy-momentum trace

Energy levels of QED bound states, which depend on a number of independent mass parameters, can be calculated as matrix elements of the QED energy-momentum tensor trace. As an example of such system we consider muonic hydrogen. The leading one-loop corrections to its energy levels depend on the electron and muon masses. These...

💬 0 commentsarXiv:2601.11403v2PDF
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Posted in astro-ph.GA · 2026-01-16 · Ortiz-Gómez S., Torres-Flores S., Monachesi A., Montaguth G. P., Véliz Astudillo S., Mendes de Oliveira C., Olave-Rojas D. E., Lima-Dias C., Demarco R., Pallero D., Lopes A. R., Cortesi A., Telles E., Kanaan A., Ribeiro T., Schoenell W

Star-forming compact groups: Tracing the early evolutionary stages of compact group environments

In the context of pre-processing -- a scenario in which galaxies quench their star formation within substructures before falling into clusters -- we investigate the impact of environment on the physical and morphological properties of galaxies in Compact Groups (CGs), focusing specifically on a sample of Star-Forming Compact Groups...

💬 0 commentsarXiv:2601.11399v1PDF
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Posted in cond-mat.soft · 2026-01-16 · Sleeba Varghese, Sobin Alosious, Jesper Schmidt Hansen, Billy Dean Todd

NAVIS: A LAMMPS-Python framework for efficient computation of nanochannel velocity and thermal interfacial slip

We present NAVIS (NAnochannel Velocity and thermal Interfacial Slip), a LAMMPS-Python scripted toolkit for computing the Navier (hydrodynamic) friction coefficient and Kapitza (thermal) resistance at arbitrary solid-fluid interfaces. NAVIS is based on equilibrium molecular dynamics (EMD) methods for calculating the linear response...

💬 0 commentsarXiv:2601.11391v2PDF
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Posted in nucl-ex · 2026-01-16 · A. Filippi

The unfinished picture of low-energy antineutron interactions: open issues and hints for future research possibilities

This report examines the open questions that remain unsolved following the measurements with antineutrons ($\bar n$) as probes conducted up to the 1990s at the LEAR facility at CERN. It also presents suggestions for possible new experiments at a future, upgraded AD complex, which can potentially provide access to new areas of physics.

💬 0 commentsarXiv:2601.11390v1PDF
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Posted in cond-mat.mtrl-sci · 2026-01-16 · Martí Raya-Moreno, Alexander Buccheri, Noah Alexy Dasch, Nasrin Farahani, Ignacio Gonzalez Oliva, Andris Gulans, Manoar Hossain, Hannah Kleine, Martin Kuban, Sven Lubeck, Benedikt Maurer, Pasquale Pavone, Fabian Peschel, Daria Popova-Gorelova, Lu Qiao, Elias Richter, Santiago Rigamonti, Ronaldo Rodrigues Pela, Maximilian Schebek, Kshitij Sinha, Daniel T. Speckhard, Jan Stutz, Sebastian Tillack, Dmitry Tumakov, Seokhyun Hong, Jānis Užulis, Mara Voiculescu, Cecilia Vona, Mao Yang, Claudia Draxl

An exciting approach to theoretical spectroscopy

Theoretical spectroscopy, and more generally, electronic-structure theory, are powerful concepts for describing the complex many-body interactions in materials. They comprise a variety of methods that can capture all aspects, from ground-state properties to lattice excitations to different types of light-matter interaction, including...

💬 0 commentsarXiv:2601.11388v2PDF
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Posted in nlin.SI · 2026-01-16 · Graham Hesketh

Complete Weierstrass elliptic function solutions and canonical coordinates for four-wave mixing in nonlinear optical fibres

Complete analytic solutions to quasi-continuous-wave four-wave mixing in nonlinear optical fibres are presented in terms of Weierstrass elliptic $\wp$, $ζ$, and $σ$ functions, providing the full complex envelopes for all four waves under arbitrary initial conditions. A sequence of coordinate transformations reveals a canonical form...

💬 0 commentsarXiv:2601.11740v2PDF
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Posted in astro-ph.SR · 2026-01-16 · Jamila Taaki, Lia Corrales, Alfred O. Hero

Using Astrometry to Break Degeneracies in Stellar Surface Mapping

Astrometric jitter noise arises when starspots on a rotating stellar surface move in and out of view, shifting the photocenter. This noise may limit our ability to detect and weigh small, sub-Neptune-sized planets around active stars. By deriving a linear forward model for the astrometric jitter signal of a rotating star in a...

💬 0 commentsarXiv:2601.11737v2PDF
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Posted in hep-th · 2026-01-16 · Dmitry Galakhov, Alexei Gavshin, Alexei Morozov

Weyl Mutations in Quiver Yangians

The problem of solving non-linear equations would be considerably simplified by a possibility to convert known solutions into the new ones. This could seem an element of art, but in the context of ADHM-like equations describing quiver varieties there is a systematic approach. In this note we study moduli spaces and dualities of quiver...

💬 0 commentsarXiv:2601.11736v2PDF
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Posted in physics.optics · 2026-01-16 · Mohamed A. Mousa, Leif Bauer, Daien He, Sakshi Gupta, Shubhankar Jape, Utkarsh Singh, Bhagwati Prasad, Partha P. Mukherjee, Angshuman Deka, Zubin Jacob

Ultra-broadband Mid to Long-wave Infrared Spintronic Poisson Bolometer

Infrared detectors have traditionally been divided into two fundamental classes, mid-wave (MWIR, 3-5 um) and long-wave (LWIR, 8-14 um). Integrating MWIR and LWIR within a single device is challenging due to distinct materials, cooling needs, and detection mechanisms, while such integration is critical for improved object recognition,...

💬 0 commentsarXiv:2601.11733v1PDF
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Posted in astro-ph.EP · 2026-01-16 · M. R. Jankovic, N. Pawellek, J. Zander, T. Löhne, A. V. Krivov, J. Olofsson, A. Brennan, J. Milli, M. Bonduelle, M. C. Wyatt, A. A. Sefilian, T. Pearce, S. Mac Manamon, Y. Han, S. Marino, L. Matrá, A. Moór, M. Booth, E. Chiang, E. Mansell, P. Weber, A. M. Hughes, D. J. Wilner, P. Luppe, B. Zawadzki, C. del Burgo, Á. Kóspál, S. Pérez, J. M. Carpenter, Th. Henning

The ALMA survey to Resolve exoKuiper belt Substructures (ARKS). X. Interpreting the peculiar dust rings around HD 131835

Dusty discs detected around main-sequence stars are thought to be signs of planetesimal belts in which the dust distribution is shaped by collisional and dynamical processes, including interactions with gas if present. The debris disc around the young A-type star HD 131835 is composed of two dust rings at ~65 au and ~100 au, a third...

💬 0 commentsarXiv:2601.11732v1PDF
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Posted in physics.med-ph · 2026-01-16 · Jingyuan Chen, Zeliang Ma, Meiyun Cao, Robert W. Gao, Yunze Yang, Yuzhen Ding, Nicholas B. Remmes, Jiasen Ma, Kimberly S. Corbin, Dean A. Shumway, Robert W. Mutter, Wei Liu

Dose-LET Interactions Predict Capsular Contracture After Proton Postmastectomy Radiation Therapy

Pencil beam scanning (PBS) proton therapy provides highly conformal dose distributions that are increasingly leveraged for postmastectomy radiation therapy (PMRT) to reduce cardiopulmonary exposure. However, implant-based reconstruction in the setting of PMRT remains vulnerable to capsular contracture, and biological mechanisms of...

💬 0 commentsarXiv:2601.11731v1PDF