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Physics

arXiv preprints from January 1, 2026 through July 20, 2026 — 16:00:10 EST

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Posted in hep-th · 2026-01-05 · Evan Budd, Adrien Florio, David Frenklakh, Swagato Mukherjee

Quantum dynamics of cosmological particle production: interacting quantum field theories with matrix product states

Understanding real-time dynamics of interacting quantum fields in curved spacetime remains a major theoretical challenge. We employ tensor network methods to study such dynamics using interacting scalar and gauge theories in 1+1 spacetime dimensions, subject to a quench modeling a homogeneously expanding gravitational background. The...

💬 0 commentsarXiv:2601.02331v2PDF
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Posted in physics.soc-ph · 2026-01-05 · Alec Kirkley, Helcio Felippe, Federico Battiston

Structural reducibility of hypergraphs

Higher-order interactions provide a nuanced understanding of the relational structure of complex systems beyond traditional pairwise interactions. However, higher-order network analyses also incur more cumbersome interpretations and greater computational demands than their pairwise counterparts. Here we present an...

💬 0 commentsarXiv:2601.02603v1PDF
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Posted in physics.soc-ph · 2026-01-05 · A. Y. Klimenko, A. Rozycki, Y. Lu

From Agent-Based Markov Dynamics to Hierarchical Closures on Networks: Emergent Complexity and Epidemic Applications

We explore a rigorous formulation of agent-based SIR epidemic dynamics as a discrete-state Markov process, capturing the stochastic propagation of infection or an invading agent on networks. Using indicator functions and corresponding marginal probabilities, we derive a hierarchy of evolution equations that resembles the classical...

💬 0 commentsarXiv:2601.07844v1PDF
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Posted in astro-ph.HE · 2026-01-05 · Ruocheng Zhai, David Radice, Fabio Magistrelli, Sebastiano Bernuzzi, Albino Perego

Exploring Composition Mixing in Kilonova Ejecta with Ray-by-ray Simulations

Binary neutron star merger (BNSM) ejecta are considered a primary repository of $r$-process nucleosynthesis and a source of the observed heavy-element abundances. We implement composition mixing into ray-by-ray radiation-hydrodynamic simulations of BNSM ejecta, coupled with an online nuclear network (NN). We model mixing via a...

💬 0 commentsarXiv:2601.02600v2PDF
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Posted in astro-ph.EP · 2026-01-05 · Vitalii Kuksenko, Juraj Tóth

Meteor observations as a tool to constrain cosmogonic models of the Solar System

Recent observations of small bodies of the Solar System showed evidence of the presence of refractory (asteroidal) material in the Oort cloud. Different models of the origin of the Solar System predict different numbers of rocky objects in the Oort cloud, meaning that measurement of this population can be used as an observational...

💬 0 commentsarXiv:2601.02599v1PDF
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Posted in physics.ins-det · 2026-01-05 · K. Amini, T. C. H. de Raadt, J. G. H. Franssen, B. Siwick, O. J. Luiten, A. Ryabov

High-throughput, high-brightness, ultrashort 90 keV electrons at 40 kHz

Radiofrequency-compressed keV electron sources for ultrafast electron diffraction (UED) face competing demands: short pulses require low charge, yet weak scatterers demand high flux; high repetition rates enable signal averaging, yet most systems operate $\lesssim$1 kHz with low detection efficiency. Here, we demonstrate a 90 keV...

💬 0 commentsarXiv:2601.02597v1PDF
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Posted in gr-qc · 2026-01-05 · Mariano Cadoni, Leonardo de Lima, Mirko Pitzalis, Davi C. Rodrigues, Andrea P. Sanna

Cosmologically Coupled Black Holes with Regular Horizons

We present the most general and exact solution of Einstein's gravity sourced by an anisotropic fluid describing the cosmological embedding (CE) of a static and spherically-symmetric object, including black holes (BHs) or exotic compact objects, without radial energy influx and in an arbitrary Friedmann-Lemaître-Robertson-Walker (FLRW)...

💬 0 commentsarXiv:2601.03296v2PDF
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Posted in astro-ph.EP · 2026-01-05 · Chunhua Qi, David J. Wilner, Catherine C. Espaillat

Isotopic Ratios in the Disk of HD 163296

Isotopic abundance ratios in protoplanetary disks are critical for understanding volatile inheritance and chemical evolution in planet-forming environments. We present Atacama Large Millimeter/submillimeter Array observations of the rare isotopologue 13C18O(2-1) at approximately 0.3 arcsec resolution from the disk around the Herbig Ae...

💬 0 commentsarXiv:2601.02593v1PDF
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Posted in cond-mat.str-el · 2026-01-05 · Loïc Herviou, Elodie Campan, Pierre Nataf

$\mathbb{Z}_L$ symmetry breaking in SU(N) Fermi-Hubbard dots at zero and finite temperature

We address the SU(N) Fermi-Hubbard model on a chain, with $N$ the number of degenerate orbitals, or colors, for each fermion. In the limit of both large number of colors $N$ and particles, and small number of sites $L \geq 2$, the model is proved to undergo a $\mathbb{Z}_L$ symmetry breaking for attractive local interaction amplitude...

💬 0 commentsarXiv:2601.02590v1PDF
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Posted in physics.plasm-ph · 2026-01-05 · B. Z. Djordjević, D. J. Strozzi, G. B. Zimmerman, S. A. MacLaren, C. R. Weber, D. D. -M. Ho, L. S. Leal, C. A. Walsh, J. D. Moody

Integrated Radiation-Magneto-Hydrodynamic Simulations of Magnetized Burning Plasmas. I. Magnetizing Ignition-Class Designs

Motivated by breakthroughs in inertial confinement fusion (ICF), first achieving ignition conditions in National Ignition Facility (NIF) shot N210808 and then laser energy breakeven in N221204, modeling efforts here investigate the effect of imposed magnetic fields on integrated hohlraum simulations of igniting systems. Previous NIF...

💬 0 commentsarXiv:2601.02588v2PDF
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Posted in physics.bio-ph · 2026-01-05 · Enso O. Torres Alegre

Evolutionary tuning of TAM receptor-ligand interfaces highlights electrostatic features associated with regenerative phagocytic signaling

Efficient resolution of neuroinflammation and debris clearance is a key determinant of successful central nervous system regeneration. Regenerative vertebrates such as Danio rerio often exhibit faster immune resolution and debris clearance than mammals, yet the molecular determinants underlying these differences remain incompletely...

💬 0 commentsarXiv:2601.08855v1PDF
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Posted in hep-ph · 2026-01-05 · Yang Yu, Peng Cheng, Hui-Yu Xing, Daniele Binosi, Craig D. Roberts

Helicity Dependent Distribution Functions of the Proton and $Λ$ and $Σ^0$ Baryons

Using continuum Schwinger function methods, a coherent set of predictions for proton, $Λ$ and $Σ^0$ distribution functions (DFs) has been made available -- both helicity dependent and unpolarised. The results and comparisons between them reveal impacts of diquark correlations and SU$(3)$-flavour symmetry breaking, some of which are...

💬 0 commentsarXiv:2601.02587v1PDF
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Posted in nlin.CD · 2026-01-05 · Zhenwei Xu, Ulrich Kuhl, Nicolas Noiray

Dynamic Synchronization of Driven Self-Oscillators: Modeling and Experiment

Synchronization of self-sustained oscillators under fixed-frequency and amplitude forcing is well understood, but how time-varying forcing mangles phase locking has been much less explored. Theory predicts that slow, deterministic modulation of the drive amplitude or frequency can lead to a peculiar synchronization regime...

💬 0 commentsarXiv:2601.02584v1PDF
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Posted in physics.app-ph · 2026-01-05 · Caroline M. Barotta, Jack-William Barotta

The physics of cranberry bogs

The common New England sight of a cranberry bog presents a rich tapestry of fluid dynamics and soft matter phenomena. Here, we present four connected problems exploring the behavior of cranberries in their stages of harvest: the buoyant rise of a cranberry in a flooded bog, the stable floating configuration of a cranberry on the...

💬 0 commentsarXiv:2601.11593v1PDF
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Posted in astro-ph.GA · 2026-01-05 · Seneca K. H. Bahr, Aleksandr V. Mosenkov, Jacob A. Guerrette, Isaac H. Jensen, Jonah X. George, Thea E. Spigarelli, Ryan P. Smith, Brandon T. Burton, Kevan W. Beckstead, Jonah D. Seguine, Harrison K. Casper, Nefi Pineda, Michael Holland

COUGS-DESI: A Catalog of Unusual Galaxies with Polar Structures in the DESI Legacy Imaging Surveys

Polar-structure galaxies (PSGs) host photometrically and kinematically decoupled components oriented at large angles to one another. These systems, which include polar rings, polar disks, polar halos, polar bulges, polar dust lanes, and polar tidal structures, provide valuable insights into galaxy formation and evolution, although...

💬 0 commentsarXiv:2601.02579v3PDF
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Posted in astro-ph.IM · 2026-01-05 · David Rousso, Moritz Bjoern Kristiansson Kunze, Christoph Reinhardt

Optomechanical platform for high-frequency gravitational wave and vector dark matter detection

We present a proposal for a nanomechanical membrane resonator integrated into a moderate-finesse ($\mathcal{F}\sim 10$) optical cavity as a versatile platform for detecting high-frequency gravitational waves and vector dark matter. Gravitational-wave sensitivity arises from cavity-length modulation, which resonantly drives membrane...

💬 0 commentsarXiv:2601.02576v1PDF
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Posted in physics.geo-ph · 2026-01-05 · Valeria Villa, Robert W. Clayton, Patricia Persaud

Receiver Functions in the San Fernando Valley, California: Graph-Regularized Bayesian Approach for Gravity-Informed Mapping

The San Fernando Valley (SFV) in Southern California is a complex sedimentary basin whose shape strongly influences ground shaking. We develop a fully quantitative, probabilistic graph-regularized inference model that integrates both gravity and receiver function (RF) constraints and evaluate its ability to determine the basin's...

💬 0 commentsarXiv:2601.02575v1PDF
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Posted in physics.optics · 2026-01-05 · Xiangjun Kong, Qingkang Bao, Tibebe Yalew, Gerardo Adesso, Samanta Piano

Deep Learning-based Single-Shot Composite Fringe Projection Profilometry with Pixel-Wise Uncertainty Quantification

Driven by the growing demand for high-speed 3D measurement in advanced manufacturing, optical metrology algorithms must deliver high accuracy and robustness under dynamic conditions. Fringe projection profilometry (FPP) offers high precision, yet the 2pi ambiguity of the wrapped phase means that conventional absolute phase recovery...

💬 0 commentsarXiv:2601.02572v1PDF
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Posted in cond-mat.mtrl-sci · 2026-01-05 · Thiago S. Arnaud, Ryan W. Spangler, Johnathan D. Georgaras, Jonah B. Haber, Daniel Hirt, Maximilian Obst, Gonzalo Álvarez-Pérez, Mackey Long, Felix G. Kaps, Jakob Wetzel, Courtney Ragle, John E. Buchner, Youngji Kim, Aditha S. Senarath, Richarda Niemann, Mingze He, Giulia Carini, Unai Arregui-Leon, Akash C. Behera, Ramachandra Bangari, Nihar Sahoo, Niels C. Brumby, J. Michael Klopf, Martin Wolf, Lukas M. Eng, Susanne C. Kehr, Thomas G. Folland, Alexander Paarmann, Patrick E. Hopkins, Felipe Jornada, Jon-Paul Maria, Joshua D. Caldwell

Tailoring phonon-driven responses in α-MoO3 through isotopic enrichment

The implementation of polaritonic materials into nanoscale devices requires selective tuning of parameters to realize desired spectral or thermal responses. One robust material is α-MoO3, which as an orthorhombic crystal boasts three distinct phonon dispersions, providing three polaritonic dispersions of hyperbolic phonon polaritons...

💬 0 commentsarXiv:2601.02570v1PDF
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Posted in gr-qc · 2026-01-05 · G. G. Luciano, A. Paliathanasis, G. Leon, A. Sheykhi, M. Motaghi

Hints Beyond $Λ$CDM from Barrow and Tsallis Holographic Dark Energy with GO cutoff

Barrow and Tsallis Holographic Dark Energy (HDE) are two recent extensions of the standard HDE framework, obtained by introducing generalized entropy corrections through the Barrow and Tsallis formalisms. In this work, we examine the cosmological consequences of Barrow and Tsallis HDE implemented with the Granda-Oliveros (GO) infrared...

💬 0 commentsarXiv:2601.02567v1PDF
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Posted in quant-ph · 2026-01-05 · Walter O. Krawec

Further Improving the Decoy State Quantum Key Distribution Protocol with Advantage Distillation

In this paper, we revisit the application of classical advantage distillation (CAD) to the decoy-state BB84 protocol. Prior work has shown that CAD can greatly improve maximal distances and noise tolerances of the practical decoy state protocol. However, past work in deriving key-rate bounds for this protocol with CAD have assumed a...

💬 0 commentsarXiv:2601.02565v2PDF
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Posted in astro-ph.IM · 2026-01-05 · Arpita Roy, Stuart Feldman, Pete Klupar, John DiPalma, Saul Perlmutter, Ewan S. Douglas, Greg Aldering, Gabor Furesz, Patrick Ingraham, Gudmundur Stefansson, Douglas Kelly, Fan Yang Yang, Thomas Wevers, Nicole Arulanantham, James Lasker, Mickael Rigault, Everett Schlawin, Sander R. Zandbergen, S. Pete Worden, Ramya Anche, Heejoo Choi, Ian J. M. Crossfield, Kevin Derby, Jerry Edelstein, Mike Eiklenborg, Suvi Gezari, Paul Giuliano, Justin Hom, Taylor J. Hoyt, Hyukmo Kang, Daewook Kim, Keerthi Kunnumkai, Leander Lacroix, Jared R. Males, Thomas J. Maccarone, Kian Milani, Timothy N. Miller, Kelsey Lynn Miller, Pierre Nicolas, Antonella Palmese, Jason Pero, Laurent Pueyo, Stephanie Rinaldi, David J. Sand, Christian Schneider, Sanchit Sabhlok, Arfon Smith, Irina I. Stefan, Saraswathi Kalyani Subramanian, Kyle Van Gorkom, Andre F. Wong, Jaegun Yoo, Md Abdullah Al Zaman, the Lazuli Science Team

The Lazuli Space Observatory: Architecture & Capabilities

The Lazuli Space Observatory is a 3-meter aperture astronomical facility designed for rapid-response observations and precision astrophysics across visible to near-infrared wavelengths (400-1700 nm bandpass). An off-axis, freeform telescope delivers diffraction-limited image quality (Strehl $>$0.8 at 633 nm) to three instruments...

💬 0 commentsarXiv:2601.02556v1PDF
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Posted in cond-mat.str-el · 2026-01-05 · A. A. Aczel, B. R. Ortiz, Y. Luo, G. Pokharel, P. M. Sarte, C. dela Cruz, J. Liu, G. Sala, S. D. Wilson, B. A. Frandsen, J. A. M. Paddison

Influence of controlled disorder on the dipolar spin ice state of Ho-based pyrochlores

Pyrochlore magnets of the form $R_2B_2$O$_7$, in which rare-earth ions on the $R$-site form a three-dimensional network of corner-sharing tetrahedra, provide a canonical setting for geometrical frustration. Ho-based pyrochlores host a dipolar spin-ice ground state, characterized by Ising moments constrained by the ice rules and...

💬 0 commentsarXiv:2601.02555v2PDF
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Posted in astro-ph.IM · 2026-01-05 · Christopher. J. R. Clark, Roberto J. Avila, Alyssa Guzman, Norman A. Grogin

Using 23 Years of ACS/SBC Data to Understand Backgrounds: Significant Reductions in Expected Background Levels

We have used 23 years of Hubble Space Telescope ACS/SBC data to study what background levels are encountered in practice and how much they vary. The backgrounds vary considerably, with F115LP, F122M, F125LP, PR110L, and PR130L all showing over an order of magnitude of variation in background between observations, apparently due to...

💬 0 commentsarXiv:2601.02551v1PDF
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Posted in cond-mat.mtrl-sci · 2026-01-05 · Irene Festi, Antoine Cornet, Tomoki Fujita, Jens Moesggard, Alberto Ronca, Jie Shen, Michael Sprung, Shuai Wei, Fabian Westermeier, Raphael Escalier, Andrea Piarristeguy, Giacomo Baldi, Beatrice Ruta

X-ray photo-induced atomic motion in Phase Change Materials and conventional covalent chalcogenide glasses

X-ray Photon Correlation Spectroscopy (XPCS) enables direct access to atomic-scale dynamics in disordered materials, revealing both spontaneous and X-ray-induced relaxation processes. Here, we study two compositionally similar alloy glasses near their glass transition temperatures: the phase change material (PCM) Ge15Sb85 and the...

💬 0 commentsarXiv:2601.02550v1PDF