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Physics

arXiv preprints from January 1, 2026 through July 20, 2026 — 17:57:40 EST

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Posted in astro-ph.HE · 2026-01-07 · David A. Coulter, Conor Larison, Justin D. R. Pierel, Seiji Fujimoto, Vasily Kokorev, Joseph F. V. Allingham, Takashi J. Moriya, Matthew Siebert, Yoshihisa Asada, Rachel Bezanson, Maruša Bradač, Gabriel Brammer, John Chisholm, Dan Coe, Pratika Dayal, Michael Engesser, Steven L. Finkelstein, Ori D. Fox, Lukas J. Furtak, Anton M. Koekemoer, Thomas Moore, Minami Nakane, Masami Ouchi, Richard Pan, Robert Quimby, Armin Rest, Johan Richard, Luke Robbins, Louis-Gregory Strolger, Fengwu Sun, Tommaso Treu, Hiroto Yanagisawa, Abdurro'uf, Aadya Agrawal, Ricardo Amorín, Joseph P. Anderson, Rodrigo Angulo, Hakim Atek, Franz E. Bauer, Larry D. Bradley, Volker Bromm, Mateusz Bronikowski, Christopher J. Conselice, Christa DeCoursey, James M. DerKacy, Guillaume Desprez, Suhail Dhawan, Jose M. Diego, Eiichi Egami, Andreas Faisst, Brenda Frye, Sebastian Gomez, Mauro González-Otero, Massimo Griggio, Yuichi Harikane, Kohei Inayoshi, Saurabh W. Jha, Yolanda Jiménez-Teja, Jeyhan S. Kartaltepe, Patrick L. Kelly, Lindsey A. Kwok, Zachary G. Lane, Xiaolong Li, Ivo Lobbe, Paulo A. A. Lopes, Ray A. Lucas, Georgios E. Magdis, Nicholas S. Martis, Jorryt Matthee, Ashish K. Meena, Rohan P. Naidu, Gaël Noirot, Masamune Oguri, Estefania Padilla Gonzalez, Massimo Pascale, Tanja Petrushevska, Massimo Ricotti, Daniel Schaerer, Stefan Schuldt, Melissa Shahbandeh, William Sheu, Koji Shukawa, Akiyoshi Tsujita, Eros Vanzella, Qinan Wang, John Weaver, Robert Williams, Rogier Windhorst, Yi Xu, Yossef Zenati, Adi Zitrin

A spectroscopically confirmed, strongly lensed, metal-poor Type II supernova at z = 5.13

Observing supernovae (SNe) in the early Universe (z > 3) provides a window into how both galaxies and individual stars have evolved over cosmic time, yet a detailed study of high-redshift stars and SNe has remained difficult due to their extreme distances and cosmological redshifting. To overcome the former, searches for...

💬 0 commentsarXiv:2601.04156v2PDF
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Posted in cond-mat.dis-nn · 2026-01-07 · Dafne Prado Bandeira, Marco Tarzia

Anderson Localization on Husimi Trees and its implications for Many-Body localization

Motivated by the analogy between many-body localization (MBL) and single-particle Anderson localization on hierarchical graphs, we study localization on the Husimi tree, a generalization of the Bethe lattice with a finite density of local loops of arbitrary but finite length. The exact solution of the model provides a transparent and...

💬 0 commentsarXiv:2601.04155v3PDF
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Posted in cond-mat.soft · 2026-01-07 · Nolan A. Miller, Laura C. Bradley, Alfred J. Crosby

Modulus and confinement effects on self-repeating, power-amplified snapping of soft, swollen beams

Latch-mediated Spring Actuation (LaMSA) is a mechanism found in nature, employed by organisms that generate the highest levels of power density through repeatable, rapid energy release. While LaMSA has been used in engineered systems like archery bows, catapults, and jumping robots, most such technologies require external power for...

💬 0 commentsarXiv:2601.04154v1PDF
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Posted in gr-qc · 2026-01-07 · Kanabar Jay, Kharanshu N. Solanki, Pankaj S. Joshi

Obstructions to global visibility of singularities in asymptotically flat spacetimes

Consider an $(N+1)$-dimensional asymptotically flat spacetime and a future-directed, affinely parametrized outgoing null generator $γ$ of an achronal boundary $\partial J^+(S_\varepsilon)$, where $\{S_\varepsilon\}$ is a nested family of smooth compact codimension $2$ surfaces approaching a singular boundary set $S$ in the past. In...

💬 0 commentsarXiv:2601.04152v1PDF
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Posted in hep-lat · 2026-01-07 · Stephen R. Sharpe

Three-particle scattering amplitudes from lattice QCD

I review recent progress in calculating scattering amplitudes and resonance properties involving three particles using results from lattice QCD. The necessary input is the finite-volume spectrum, and the outputs -- via solutions of integral equations -- are scattering amplitudes that can be continued into the complex plane to search...

💬 0 commentsarXiv:2601.04147v2PDF
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Posted in gr-qc · 2026-01-07 · Stephon Alexander, Lawrence Edmond, Cooper Niu

Parity-violating Dark Photon Halos

We propose a mechanism for the generation of gravitationally bound dark photon halos during the matter-dominated era. Coupled to an ultralight axion field through a parity-violating Chern-Simons term, dark photons can be produced by the tachyonic instability of axion coherent oscillation. The dark photons with a net helicity lead to a...

💬 0 commentsarXiv:2601.04145v1PDF
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Posted in gr-qc · 2026-01-07 · Jibril Ben Achour, Etera Livine, Vincent Vennin

Symmetries of cosmological perturbations: The residual low-multipole ambiguity

In cosmology, long-wavelength modes are related to large-gauge transformations (LGT), i.e. changes of coordinates that modify the physical geometry of the cosmological patch. These LGTs stand as bona-fide symmetries of cosmological perturbation theory with various applications, from consistency relations constraining cosmological...

💬 0 commentsarXiv:2601.04144v2PDF
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Posted in hep-ph · 2026-01-07 · Michael Fucilla, Jean-Philippe Lansberg, Maxim Nefedov, Lech Szymanowski, Samuel Wallon

Complete NLO BFKL impact factors for quarkonium hadroproduction in NRQCD: the case of ${}^1S_0^{[1]}$, ${}^1S_0^{[8]}$, and ${}^3S_1^{[8]}$ states

We present the first complete next-to-leading-order calculation of the impact factors for hadroproduction of the ${}^1S_0^{[1]}$, ${}^1S_0^{[8]}$, and ${}^3S_1^{[8]}$ NRQCD states within the BFKL formalism. We complete the recent virtual-correction computation presented in JHEP 12 (2024) 129 by that of the real-emission contributions....

💬 0 commentsarXiv:2601.04142v4PDF
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Posted in astro-ph.HE · 2026-01-07 · Keigo Fukumura, Alessandro Peca, Roberto Serafinelli, Mauro Dadina

Implications of Non-equatorial Relativistic Accretion Flows for Ultra-Fast Inflows in AGNs

Motivated by a number of X-ray observations of active galactic nuclei (AGNs) that exhibit a potential signature of ultra-fast inflows (UFIs), we consider in this work a scenario that UFIs can be physically identified as weakly-magnetized hydrodynamic accretion flows that is guided and channeled by poloidal magnetic field into...

💬 0 commentsarXiv:2601.04141v1PDF
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Posted in astro-ph.EP · 2026-01-07 · Luke B. Handley, Konstantin Batygin

Secular Excitation of Polar Neptune Orbits in Pure Disk-Planet Systems

The stellar spin-orbit angles of Neptune-sized planets present a primordial yet puzzling view of the planetary formation epoch. The striking dichotomy of aligned and perpendicular orbital configurations are suggestive of obliquity excitation through secular resonance -- a process where the precession of a hot Neptune becomes locked...

💬 0 commentsarXiv:2601.04140v1PDF
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Posted in quant-ph · 2026-01-07 · Cristofero Oglialoro, Gerard J. Machado, Felix Farsch, Daniel F. Urrego, Alejandra A. Padilla, Raj B. Patel, Ian A. Walmsley, Markus Gräfe, Juan P. Torres, Enno Giese

Below-shot-noise capacity in phase estimation using nonlinear interferometers

Over the past decade, several schemes for imaging and sensing based on nonlinear interferometers have been proposed and demonstrated experimentally. These interferometers exhibit two main advantages. First, they enable probing a sample at a chosen wavelength while detecting light at a different wavelength with high efficiency (bicolor...

💬 0 commentsarXiv:2601.04139v1PDF
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Posted in astro-ph.GA · 2026-01-07 · David Vizgan, Joaquin D. Vieira, Justin S. Spilker, Simon Birrer, Nan Zhang, Manuel Aravena, Melanie A. Archipley, Jack E. Birkin, Jared Cathey, Scott C. Chapman, Veronica J. Dike, Anthony H. Gonzalez, Thomas R. Greve, Gayathri Gururajan, Ryley Hill, Matthew A. Malkan, Desika Narayanan, Kedar A. Phadke, Vismaya Pillai, Ana C. Posses, Manuel Solimano, Nikolaus Sulzenauer, Dazhi Zhou

A census of star-formation and gas mass tracers in two lensed $z \sim 4$ dusty star-forming galaxies

We present new and archival Atacama Large Millimeter/submillimeter Array (ALMA) observations of two strongly lensed dusty star-forming galaxies (DSFGs) selected from the South Pole Telescope survey, SPT0418-47 $(z = 4.225)$ and SPT2147-50 $(z = 3.760)$. We study the [C II], CO(7-6), [C I](2-1), and, in SPT0418-47, $p$-H$_2$O emission,...

💬 0 commentsarXiv:2601.04133v1PDF
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Posted in astro-ph.HE · 2026-01-07 · Pietro Monti-Guarnieri, Gianfranco Paternò, Alexei Sytov, Elisabetta Cavazzuti, Luigi Costamante, Sara Cutini, Matteo Duranti, Pierluigi Fedeli, Richard J. Gaitskell, Vincenzo Guidi, Viktar Haurylavets, Savvas M. Koushiappas, Francesco Longo, Sofia Mangiacavalli, Andrea Mazzolari, Michela Prest, Marco Romagnoni, Alessia Selmi, Mattia Soldani, Victor Tikhomirov, Valerio Vagelli, Erik Vallazza, Laura Bandiera

Satellite-borne $γ$-ray astrophysics from coherent interactions in oriented crystals

High-density and high-Z crystals are key elements of most space-borne $γ$-ray telescopes operating at gigaelectronvolt energies (such as Fermi-LAT). The lattice structure is usually neglected in the development of a crystalline detector, although its effects on the energy deposit development should be taken into account, since the...

💬 0 commentsarXiv:2601.04129v2PDF
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Posted in physics.optics · 2026-01-07 · Clément Ferise, Pierre Granier, Antton Goïcoechea, François Sarrazin, Philippe Besnier, Matthieu Davy

Backscatter Communication Through Disordered Media Enabled by a Programmable Leaky Cavity

Retrieving information through disordered scattering systems remains a major challenge in wireless communication and sensing due to the severe distortion and attenuation caused by multiple scattering. Here, we demonstrate robust focusing through random media using a leaky cavity made programmable by reconfigurable metasurfaces. We...

💬 0 commentsarXiv:2601.04128v1PDF
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Posted in cond-mat.stat-mech · 2026-01-07 · J. L. Cardoso, V. G. Ibarra-Sierra, J. C. Sandoval-Santana, A. Kunold

The thermodynamics of liquid-vapor coexistence for a van der Waals fluid. Analytical solution of the Clausius-Clapeyron equation

This work presents a pedagogical derivation of the thermodynamics of a van der Waals fluid by explicitly incorporating pairwise molecular interactions and the finite size of particles into the statistical-mechanical description. Starting from the Lennard-Jones potential, we evaluate the second virial coefficient to infer the virial...

💬 0 commentsarXiv:2601.04296v1PDF
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Posted in cond-mat.stat-mech · 2026-01-07 · Johannes Schmidt, Žiga Krajnik, Vladislav Popkov

Universality in driven systems with a multiply-degenerate umbilic point

We investigate a driven particle system, a multilane asymmetric exclusion process, where the particle number in every lane is conserved, and stationary state is fully uncorrelated. The phase space has, starting from three lanes and more, an umbilic manifold where characteristic velocities of all the modes but one coincide, thus...

💬 0 commentsarXiv:2601.04116v2PDF
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Posted in hep-th · 2026-01-07 · M. M. Sheikh-Jabbari, V. Taghiloo

Freelance Fluid/Gravity Correspondence, 3d Analysis

Freelance holography program is an extension of gauge/gravity correspondence, where the gravity theory is defined on a portion of AdS with an arbitrary timelike boundary, with any desired boundary conditions. It is also known that gauge/gravity correspondence admits a fluid/gravity correspondence limit, where the gauge theory side is...

💬 0 commentsarXiv:2601.04115v1PDF
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Posted in physics.flu-dyn · 2026-01-07 · Sawyer Remillard, Bachir A. Abeid, Timothy L. Hall, Jonathan R. Sukovich, Jacob Baker, Jin Yang, Jonathan B. Estrada, Mauro Rodriguez

Microbubble surface instabilities in a strain stiffening viscoelastic material

Understanding the dynamics of instabilities along fluid-solid interfaces is critical for the efficacy of focused ultrasound therapy tools (e.g., histotripsy) and microcavitation rheometry techniques. Non-uniform pressure fields generated by either ultrasound or a focused laser can cause non-spherical microcavitation bubbles. Previous...

💬 0 commentsarXiv:2601.04113v1PDF
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Posted in hep-ph · 2026-01-07 · Emrys Peets

Compatibility of the Updated $(g-2)_μ$, $(g-2)_e$ and PADME-Favored Couplings with the Preferred Region of ATOMKI X17

We re-evaluate the viability of a kinetically mixed dark photon ($A^{\prime}$) as a solution to the muon anomalous magnetic moment $(g-2)μ$ discrepancy and the ATOMKI nuclear anomalies near 17~MeV, using the final FNAL measurement and the latest theory predictions (BMW21, WP25). For $m_{A^{\prime}} = 17$~MeV, the allowed kinetic...

💬 0 commentsarXiv:2601.05288v2PDF
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Posted in astro-ph.SR · 2026-01-07 · E. Artur de la Villarmois, V. V. Guzmán, M. L. van Gelder, E. F. van Dishoeck, E. A. Bergin, D. Harsono, N. Sakai, J. K. Jørgensen

Characterizing the physical and chemical properties of the Class I protostellar system Oph-IRS 44. Binarity, infalling streamers, and accretion shocks

(Abridged) In the low-mass star formation process, theoretical models predict that material from the infalling envelope could be shocked as it encounters the outer regions of the disk. Nevertheless, only a few protostars show evidence of these shocks at the disk-envelope interface, and the main formation path of shocked-related...

💬 0 commentsarXiv:2601.04108v1PDF
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Posted in hep-ph · 2026-01-07 · Laszlo Gyulai, Gabor Biro, Robert Vertesi, Gergely Gabor Barnafoldi

Effect of event classification on the Tsallis-thermometer

We analyze identified hadron spectra in pp collisions at $\sqrt{s} = 13$ TeV measured by ALICE within a non-extensive statistical framework. Spectra classified by multiplicity, flattenicity, and spherocity were fitted with the Tsallis-Pareto distribution, and the parameters were studied on the Tsallis-thermometer. Multiplicity and...

💬 0 commentsarXiv:2601.04106v1PDF
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Posted in cond-mat.str-el · 2026-01-07 · Yunhao Fan, Gia-Wei Chern

Equivariant Neural Networks for Force-Field Models of Lattice Systems

Machine-learning (ML) force fields enable large-scale simulations with near-first-principles accuracy at substantially reduced computational cost. Recent work has extended ML force-field approaches to adiabatic dynamical simulations of condensed-matter lattice models with coupled electronic and structural or magnetic degrees of...

💬 0 commentsarXiv:2601.04104v1PDF
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Posted in astro-ph.GA · 2026-01-07 · Alex N. Byrne, Christopher N. Shingledecker, Edwin A. Bergin, Martin S. Holdren, Gabi Wenzel, Ci Xue, Troy Van Voorhis, Brett A. McGuire

Modeling the Effect of C/O Ratio on Complex Carbon Chemistry in Cold Molecular Clouds

Elemental abundances, which are often depleted with respect to the solar values, are important input parameters for kinetic models of interstellar chemistry. In particular, the amount of carbon relative to oxygen is known to have a strong effect on modeled abundances of many species. While previous studies have focused on comparison...

💬 0 commentsarXiv:2601.04103v1PDF
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Posted in physics.plasm-ph · 2026-01-07 · Alexander Wieczorek, Nathan Rodkey, Jan Sommerhäuser, Jason Hattrick-Simpers, Sebastian Siol

Autonomous Sampling and SHAP Interpretation of Deposition-Rates in Bipolar HiPIMS

High-power impulse magnetron sputtering (HiPIMS) offers considerable control over ion energy and flux, making it invaluable for tailoring the microstructure and properties of advanced functional coatings. However, compared to conventional sputtering techniques, HiPIMS suffers from reduced deposition rates. Many groups have begun to...

💬 0 commentsarXiv:2601.05287v1PDF