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arXiv preprints from January 1, 2026 through September 11, 2026 — 12:10:18 EST

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Posted in quant-ph · 2026-01-05 · A. S. Usoltsev, L. V. Gerasimov, A. D. Manukhova, S. P. Kulik, D. V. Kupriyanov

Optical nonlinearity of cold atomic ensemble driven by strong coherent field in a saturation regime

We present a microscopic analysis and evaluation of the dielectric susceptibility of a dielectric medium consisting of vector-type two-energy-level atoms responding on a weak probe mode when the atoms are driven by a strong coherent field. Each atom, in an environment of others, exists as a quasiparticle further structuring a bulk...

💬 0 commentsarXiv:2601.02152v1PDF
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Posted in quant-ph · 2026-01-05 · Arisa Ikeda, Akitada Sakurai, Kae Nemoto, Mayu Muramatsu

Quantum Extreme Reservoir Computing for Phase Classification of Polymer Alloy Microstructures

Quantum machine learning (QML) is expected to offer new opportunities to process high-dimensional data efficiently by exploiting the exponentially large state space of quantum systems. In this work, we apply quantum extreme reservoir computing (QERC) to the classification of microstructure images of polymer alloys generated using...

💬 0 commentsarXiv:2601.02150v2PDF
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Posted in cond-mat.mes-hall · 2026-01-05 · Mateusz Krawczyk, Jarosław Pawłowski

AI-enhanced tuning of quantum dot Hamiltonians toward Majorana modes

We propose a neural network-based model capable of learning the broad landscape of working regimes in quantum dot simulators, and using this knowledge to autotune these devices - based on transport measurements - toward obtaining Majorana modes in the structure. The model is trained in an unsupervised manner on synthetic data in the...

💬 0 commentsarXiv:2601.02149v4PDF
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Posted in physics.ao-ph · 2026-01-05 · Béatrice Lessard-Hamel, Marcel Babin, Simon Thibault

Microscopy system for in situ sea ice structure and biology observations

Sea ice harbours a rich community of well-adapted microorganisms that inhabit liquid micro-spaces where extreme conditions prevail. Currently at risk under climate change, the sea-ice microbiome holds mysteries about evolution of life on Earth and possibly elsewhere, which require methodological innovation to be unravelled. Gaining...

💬 0 commentsarXiv:2601.02328v3PDF
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Posted in cond-mat.mtrl-sci · 2026-01-05 · Brian H. Lee, Chunyu Li, Aidan Pantoya, James P. Larentzos, John K. Brennan, Alejandro Strachan

Multi-Fidelity Predictive Model for Shock Response of Energetic Materials Using Conditional U-Net

Mapping microstructure to properties is central to materials science. Perhaps most famously, the Hall-Petch relationship relates average grain size to strength. More challenging has been deriving relationships for properties that depend on subtle microstructural features and not average properties. One such example is the initiation...

💬 0 commentsarXiv:2601.02327v1PDF
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Posted in astro-ph.EP · 2026-01-05 · Alexander Roman, Emilie Panek, Roy T. Forestano, Eyup B. Unlu, Katia Matcheva, Konstantin T. Matchev

Hunting for "Oddballs" with Machine Learning: Detecting Anomalous Exoplanets Using a Deep-Learned Low-Dimensional Representation of Transit Spectra with Autoencoders

This study explores the application of autoencoder-based machine learning techniques for anomaly detection to identify exoplanet atmospheres with unconventional chemical signatures using a low-dimensional data representation. We use the Atmospheric Big Challenge (ABC) database, a publicly available dataset with over 100,000 simulated...

💬 0 commentsarXiv:2601.02324v1PDF
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Posted in astro-ph.HE · 2026-01-05 · Pierre Sikivie, Yuxin Zhao

Axions explain the formation of supermassive black holes at cosmic dawn

In a recent paper we pointed out that supermassive black holes, with masses ranging from $10^5$ to $10^{10} M_\odot$ form naturally at cosmic dawn if the dark matter is QCD axions or axion-like particles with mass $m > 10^{-16}\, \mathrm{eV}/c^2$. No additional assumptions are required. Here we answer in detail the most commonly...

💬 0 commentsarXiv:2601.02321v1PDF
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Posted in cond-mat.stat-mech · 2026-01-05 · Soumyabrata Saha, Sandeep Jangid, Thibaut Arnoulx de Pirey, Juliane U. Klamser, Tridib Sadhu

A bottom-up approach to fluctuating hydrodynamics: Coarse-graining of stochastic lattice gases and the Dean-Kawasaki equation

Fluctuating hydrodynamics provides a quantitative, large-scale description of many-body systems in terms of smooth variables, with microscopic details entering only through a small set of transport coefficients. Although this framework has been highly successful in characterizing macroscopic fluctuations and correlations, a systematic...

💬 0 commentsarXiv:2601.02319v1PDF
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Posted in physics.optics · 2026-01-05 · Galy Yang, Eric Ashallay, Zhiming Wang, Abolfazl Bayat, Arup Neogi

Mechanisms and Opportunities for Tunable High-Purity Single Photon Emitters: A Review of Hybrid Perovskites and Prospects for Bright Squeezed Vacuum

Single-photon emitters (SPEs) are central to quantum communication, computing, and metrology, yet their development remains constrained by trade-offs in purity, indistinguishability, and tunability. This review presents a mechanism-based classification of SPEs, offering a physics-oriented framework to clarify the performance...

💬 0 commentsarXiv:2601.02317v1PDF
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Posted in cond-mat.str-el · 2026-01-05 · K. Gofryk, S. Zhou, N. Poudel, N. Dice, D. Murray, T. Pavlov, C. Marianetti

Electronic correlations and topology in Kondo insulator PuB$_6$

Utilizing a combination of dynamical mean field theory and density functional theory (DMFT/DFT), it has been theoretically proposed that PuB$_6$ is a strongly correlated topological insulator characterized by nontrivial $\mathbf{Z}_{2}$ topological invariants and metallic surface states (\textit{X. Deng et al., Phys. Rev. Lett. 111,...

💬 0 commentsarXiv:2601.02312v1PDF
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Posted in astro-ph.IM · 2026-01-05 · Scott Shambaugh

Validation of Satellite Lifetime Predictions at Leonid Space

We validate Leonid Space's satellite lifetime prediction pipeline through comprehensive backtesting against 934 non-maneuvering satellites that deorbited from LEO between 1961 and 2024. This represents the first large-scale validation of lifetime prediction tooling using forecasted space weather conditions rather than historical...

💬 0 commentsarXiv:2601.02453v2PDF
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Posted in hep-ph · 2026-01-05 · Brian P. Dolan

Fixed points of the renormalisation group running of quark and fermion mixing matrices in the Standard Model and beyond

The renormalisation group running of fermion mixing matrices in the Standard model and beyond is studied. For the massless 1-loop running with three generations six fixed points are found. Their associated anomalous dimension matrices are calculated and the nature of each fixed point, whether attractive, repulsive or mixed, is...

💬 0 commentsarXiv:2601.02452v3PDF
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Posted in physics.soc-ph · 2026-01-05 · Arturo Tozzi

Low-Dimensional Interaction Spaces Impose Geometric Constraints On Collective Organization

Collective organization in physical, biophysical, and biological systems often emerges from many weak, local interactions, yet the resulting global structures display striking regularities and apparent limits in diversity. Existing theoretical approaches typically emphasize specific mechanisms, detailed dynamics, or energetic...

💬 0 commentsarXiv:2601.11592v1PDF
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Posted in hep-ph · 2026-01-05 · F. Mahmoudi, D. Mishra

$Λ_b \to Λ$ Form Factors from Light-Cone Sum Rules with $Λ$-Baryon Distribution Amplitudes

We compute the $Λ_b \to Λ$ transition form factors using light-cone sum rules based on $Λ$-baryon distribution amplitudes, including contributions up to twist--6. The analysis is performed for pseudoscalar, vector, and axial-vector $b\to s$ currents and for different choices of the $Λ_b$ interpolating current. We find that only the...

💬 0 commentsarXiv:2601.02302v1PDF
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Posted in physics.atom-ph · 2026-01-05 · Gordon Baym, Glennys Farrar

Resolution of the hyperfine puzzle and its significance for two fermion Dirac atoms

The hyperfine interaction in the ground state of a hydrogen atom of assumed radius $R$ is proportional to $-1/R^3$, raising the question of why the hyperfine interaction does not lead to collapse of hydrogen, or positronium. We approach the problem in terms of a minimax variational calculation based on the exact Gordon solution of the...

💬 0 commentsarXiv:2601.02300v2PDF
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Posted in astro-ph.GA · 2026-01-05 · Nora Salem, Dylan M. Paré, Paulo Cortes, Mark R. Morris, Valentin J. M. Le Gouellec

The Polarization and Magnetic Field of the Radio Arc as Observed by ALMA at 100 GHz

The unique Galactic Center non-thermal filaments (NTFs) have been a focus of investigations for over 40 years. The most prominent manifestation of the NTFs is a bundle of parallel filaments known as the Radio Arc. Radio polarimetric observations made with the Very Large Array (VLA) at 10 GHz have revealed an alternating magnetic field...

💬 0 commentsarXiv:2601.02297v2PDF
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Posted in astro-ph.IM · 2026-01-05 · Lily L. Zhao, Debra A. Fischer, Andrew E. Szymkowiak, John M. Brewer, Joe Llama

Uncovering Hidden Systematics in Extreme-Precision Radial Velocity Measurements

We identify and correct for small but coherent instrumental drifts in seven years of radial velocity data from the EXtreme PREcision Spectrograph (EXPRES). The systematics are most notable for the six months before and after 2022 January, when EXPRES experienced larger temperature variations, and we see a systematic trough-to-peak...

💬 0 commentsarXiv:2601.02296v1PDF
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Posted in physics.chem-ph · 2026-01-05 · Aditya Barman, Gregory H. Jones, Kaila E. Weflen, Margarita Shepelenko, Jan M. L. Martin

Coupling between thermochemical contributions of subvalence correlation and of higher-order post-CCSD(T) correlation effects -- a step toward `W5 theory'

We consider the thermochemical impact of post-CCSD(T) contributions to the total atomization energy (TAE, the sum of all bond energies) of first- and second-row molecules, and specifically their coupling with the subvalence correlation contribution. In particular, we find large contributions from (Q) when there are several neighboring...

💬 0 commentsarXiv:2601.02294v5PDF
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Posted in hep-th · 2026-01-05 · Pinak Banerjee

M5 brane to D4 brane via cyclification of rational relative 3-cohomotopy

In this article, we start by re-deriving the equations of motion and Bianchi identities for the abelian D4 brane worldvolume. Noting that the 4-flux in M-Theory is rationally flux quantized in a non-abelian cohomology theory called 4-cohomotopy, and the three-flux on the M5 brane worldvolume in rational (twisted) 3-cohomotopy, we...

💬 0 commentsarXiv:2601.02293v2PDF
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Posted in cond-mat.soft · 2026-01-05 · Jesús Fernández, Loïc Vanel, Antoine Bérut

Colloidal Suspensions can have Non-Zero Angles of Repose below the Minimal Value for Athermal Frictionless Particles

We investigate the angle of repose $θ_r$ of dense suspensions of colloidal silica particles ($d = 2$ $μm$ to $7$ $μm$) in water-filled microfluidic rotating drum experiments, to probe the crossover between the thermal (colloidal) and athermal (granular) regimes. For the smallest particles, thermal agitation promotes slow creep flows,...

💬 0 commentsarXiv:2601.02291v3PDF
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Posted in astro-ph.HE · 2026-01-05 · Peggy Varniere, Fabien Casse, Fabrice Dodu

Looking for observational signatures of early binary black hole systems

Context. A lot of recent studies have focused on the observables associated with near merger binary black-holes (BBHs) embedded in a circumbinary disk (CBD) but we still we lack knowledge of observables of BBHs in their early stage. In that stage the separation between the two black holes is so large that both black holes could...

💬 0 commentsarXiv:2601.02288v1PDF
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Posted in astro-ph.HE · 2026-01-05 · Yue Zhao, Poshak Gandhi, Christian Knigge, Phil Charles, Daniel Stern, Peter Boorman, Pornisara Nuchvanichakul, Cordelia Dashwood Brown, David A. H. Buckley

A comprehensive search for high-velocity X-ray sources: New compact object binary candidates in the Gaia era

We perform a comprehensive search for high-velocity X-ray sources with large X-ray/optical flux ratios ($F_\mathrm{X}/F_\mathrm{G}$), identifying candidates for interacting black hole or neutron star binaries potentially accelerated by supernova natal kicks. We cross-match X-ray points sources from a variety of catalogues (Chandra,...

💬 0 commentsarXiv:2601.02287v1PDF
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Posted in astro-ph.CO · 2026-01-05 · Phusuda Thanankullaphong, Prasanta Sahoo, Prajwal Hassan Puttasiddappa, Nandan Roy

Quintom Dark Energy: Future Attractor and Phantom Crossing in Light of DESI DR2 Observation

We study the late-time cosmological dynamics of a two-field dark energy model consisting of a canonical quintessence scalar field and a phantom scalar field in a spatially flat FLRW universe. The fields are minimally coupled to gravity and uncoupled at the level of the potential, with the quintessence sector governed by an exponential...

💬 0 commentsarXiv:2601.02284v2PDF
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Posted in quant-ph · 2026-01-05 · Alfonso García-Velo, Alberto Ibort

Schwarz maps with symmetry

The theory of symmetry of quantum mechanical systems is applied to study the structure and properties of several classes of relevant maps in quantum information theory: CPTP, PPT and Schwarz maps. First, we develop the general structure that equivariant maps $Φ:\mathcal A \to \mathcal B$ between $C^\ast$-algebras satisfy. Then, we...

💬 0 commentsarXiv:2601.02282v1PDF
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Posted in cond-mat.supr-con · 2026-01-05 · Devi Vijayan Ambika, Qing-Ping Ding, Corey E. Frank, Sheng Ran, Nicholas P. Butch, Yuji Furukawa

Enhancement of antiferromagnetic spin fluctuations in UTe$_2$ under pressure revealed by $^{125}$Te NMR

Characterizing magnetic fluctuations is one of the keys to understanding the origin of superconductivity in the spin-triplet superconductor UTe$_2$ which exhibits two superconducting (SC) phases (SC1 and SC2) under pressure: SC1 where a superconducting transition temperature of $T_{\rm c}$ decreases with pressure while $T_{\rm c}$ of...

💬 0 commentsarXiv:2601.02280v1PDF