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arXiv preprints from January 1, 2026 through July 28, 2026 — 13:04:33 EST

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Posted in physics.chem-ph · 2026-01-01 · Li Chen, Leonardo Medrano Sandonas, Shirong Huang, Alexander Croy, Gianaurelio Cuniberti

Interpretable Machine Learning for Quantum-Informed Property Predictions in Artificial Sensing Materials

Digital sensing faces challenges in developing sustainable methods to extend the applicability of customized e-noses to complex body odor volatilome (BOV). To address this challenge, we developed MORE-ML, a computational framework that integrates quantum-mechanical (QM) property data of e-nose molecular building blocks with machine...

💬 0 commentsarXiv:2601.00503v1PDF
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Posted in astro-ph.HE · 2026-01-01 · Joseph O'Leary, Liam Dunn, Andrew Melatos

Discovering pulsars in compact binaries with a hidden Markov model

Discovering radio pulsars in compact binaries, whose orbital periods $P_{\rm b}$ satisfy $P_{\rm b} \lesssim 1 \, \rm{day}$, is computationally challenging, because the time-dependent pulse frequency $f_{\rm p}(t)$ is strongly Doppler modulated by the binary motion. Here we present a new, fast, semi-coherent detection scheme based on...

💬 0 commentsarXiv:2601.00500v1PDF
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Posted in astro-ph.CO · 2026-01-01 · Muhammad Yarahmadi, Amin Salehi

Late-Time Resolution of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks

We present a comprehensive Bayesian analysis of the Hubble constant within the framework of Physics-Informed Neural Networks (PINNs), focusing on the standard $Λ$CDM model and its dynamical dark energy extensions described by the Chevallier-Polarski-Linder (CPL) parametrization, both with and without massive neutrinos. By embedding...

💬 0 commentsarXiv:2601.00495v1PDF
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Posted in cond-mat.mtrl-sci · 2026-01-01 · Amirhossein Abedini, Behzad Mehrafrooz, Iyad Alabd Alhafez, Arash Kardani

Thermal History-Dependent Coalescence Mechanisms and Sintering Dynamics in Al-6.8%Cu Nanopowders

Aluminum-Copper (Al-Cu) alloys are essential materials for weight reduction critical structures in the aerospace and automotive industries, yet achieving their maximum ultrahigh-strength potential remains limited by nanoscale defect control during powder metallurgy processing. We employ large-scale molecular dynamics simulations on...

💬 0 commentsarXiv:2601.00492v1PDF
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Posted in physics.ins-det · 2026-01-01 · J. Sumaya-Martinez, E. Torres-Garcia

Fisher-Information-Driven Adaptive Acquisition for Photon-Efficient FLIM: A Dual-Implementation Framework for TCSPC and Programmable Time-Gating

We present a Fisher-information (FI) framework for photon-efficient fluorescence lifetime imaging microscopy (FLIM) that treats temporal sampling as a controllable design variable under a fixed photon (dose) budget. Starting from a Poisson photon-counting model for bi-exponential fluorescence decays convolved with a finite instrument...

💬 0 commentsarXiv:2601.00490v1PDF
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Posted in quant-ph · 2026-01-01 · Modi Ke, Dai-Nam Le, Lilia M. Woods

Casimir interactions between two parallel graphene sheets carrying steady-state drift currents

We investigate the fluctuation-induced Casimir interactions between two parallel graphene sheets carrying steady-state drift currents. The graphene properties are modeled based on the shifted Fermi disk model to capture the non-equilibrium optical response of the system. We find that the drift current introduces a repulsive correction...

💬 0 commentsarXiv:2601.00489v2PDF
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Posted in quant-ph · 2026-01-01 · Wenxuan Xie, John C Schotland

Non-Hermitian Band Topology and Edge States in Atomic Lattices

We investigate the band structure and topological phases of one- and two-dimensional bipartite atomic lattices mediated by long-range dissipative radiative coupling. By deriving an effective non-Hermitian Hamiltonian for the single-excitation sector, we demonstrate that the low-energy dynamics of the system are governed by a Dirac...

💬 0 commentsarXiv:2601.00487v1PDF
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Posted in nlin.CG · 2026-01-01 · Henryk Fukś

Ternary cellular automata induced by semigroups of order 3 are solvable

The minimal number of inputs in the local function of a non-trivial cellular automaton is two. Such a function can be viewed as as a kind of binary operation. If this operation is associative, it forms, together with the set of states, a semigroup. There are 18 semigroups of order 3 up to equivalence, and they define 18 cellular...

💬 0 commentsarXiv:2601.00486v1PDF
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Posted in astro-ph.IM · 2026-01-01 · Nicolas De Angelis, Abhay Kumar, Sergio Fabiani, Ettore Del Monte, Enrico Costa, Giovanni Lombardi, Alda Rubini, Paolo Soffitta, Andrea Alimenti, Riccardo Campana, Mauro Centrone, Giovanni De Cesare, Sergio Di Cosimo, Giuseppe Di Persio, Alessandro Lacerenza, Pasqualino Loffredo, Gabriele Minervini, Fabio Muleri, Paolo Romano, Emanuele Scalise, Enrico Silva, Davide Albanesi, Ilaria Baffo, Daniele Brienza, Valerio Campomaggiore, Giovanni Cucinella, Andrea Curatolo, Giulia de Iulis, Andrea Del Re, Vito Di Bari, Simone Di Filippo, Immacolata Donnarumma, Pierluigi Fanelli, Nicolas Gagliardi, Paolo Leonetti, Matteo Mergè, Dario Modenini, Andrea Negri, Daniele Pecorella, Massimo Perelli, Alice Ponti, Francesca Sbop, Paolo Tortora, Alessandro Turchi, Valerio Vagelli, Emanuele Zaccagnino, Alessandro Zambardi, Costantino Zazza

Spectral performance of single-channel plastic and GAGG scintillator bars of the CUbesat Solar Polarimeter (CUSP)

Our Sun is the closest X-ray astrophysical source to Earth. As such, it makes a formidable case study to better understand astrophysical processes. Solar flares are in particular very interesting as they are linked to coronal mass ejections as well as magnetic field reconnection sites in the solar atmosphere. Flares can therefore...

💬 0 commentsarXiv:2601.00485v1PDF
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Posted in quant-ph · 2026-01-01 · Ali Al-Bayaty, Marek Perkowski

A Geometrical Design Tool for Building Cost-Effective Layout-Aware n-Bit Quantum Gates Using the Bloch Sphere Approach

The conventional design technique of any n-bit quantum gate is mainly achieved using unitary matrices multiplication, where n >= 2 and 1 <= m <= n-1 for m target qubits and n-m control qubits. These matrices represent quantum rotations by an n-bit quantum gate. For a quantum designer, such a conventional technique requires extensive...

💬 0 commentsarXiv:2601.00484v1PDF
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Posted in quant-ph · 2026-01-01 · Long Ma, Larissa Inácio, Dai-Nam Le, Lilia M. Woods, Mathias Boström

Prediction of a measurable sign change in the Casimir force using a magnetic fluid

We demonstrate quantum levitation controlled by Casimir forces acting between a polystyrene surface and a Teflon-coated metallic substrate immersed in a mixture of Toluene and magnetite particles. This system experiences repulsion-attraction transitions in the Casimir interaction for distances where the effect is measurable. This...

💬 0 commentsarXiv:2601.00483v1PDF
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Posted in cond-mat.soft · 2026-01-01 · Aritra K. Mukhopadhyay, Ran Niu, Linhui Fu, Kai Feng, Christopher Fujta, Qiang Zhao, Jinping Qu, Benno Liebchen

Automated decision-making by chemical echolocation in active droplets

Motile microorganisms, like bacteria and algae, unify abilities like self-propulsion, autonomous navigation, and decision-making on the micron scale. While recent breakthroughs have led to the creation of synthetic microswimmers and nanoagents that can also self-propel, they still lack the functionality and sophistication of their...

💬 0 commentsarXiv:2601.00480v1PDF
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Posted in nlin.CG · 2026-01-01 · Henryk Fukś, Yucen Jin

Approximating dynamics of a number-conserving cellular automaton by a finite-dimensional dynamical system

The local structure theory for cellular automata (CA) can be viewed as an finite-dimensional approximation of infinitely-dimensional system. While it is well known that this approximation works surprisingly well for some cellular automata, it is still not clear why it is the case, and which CA rules have this property. In order to...

💬 0 commentsarXiv:2601.00479v1PDF
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Posted in astro-ph.SR · 2026-01-01 · Andrea K. Dupree, Paul I. Cristofari, Morgan MacLeod, Kateryna Kravchenko

Betelgeuse: Detection of the Expanding Wake of the Companion Star

Recent analyses conclude that Betelgeuse, a red supergiant star (HD 39801), likely has a companion object with a period of about 2000 days orbiting at only 2.3 stellar radii, deep in the chromosphere of the supergiant. A probable detection of such a companion, named Siwarha, has just occurred from speckle imaging. This study finds...

💬 0 commentsarXiv:2601.00470v1PDF
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Posted in physics.ins-det · 2026-01-01 · Farhad Hakimi, Hosain Hakimi

Terrestrial Test of Shapiro Time Delay: Forth test of Einstein General Theory of Relativity

The Shapiro time delay is one of the four classical tests of Einstein general theory of relativity and is commonly interpreted as a constrain on the parametrized post Newtonian (PPN) parameter gamma, which is exactly unity in general relativity. To date all measurement of the Shapiro time delay have been confined to astrophysical and...

💬 0 commentsarXiv:2601.00468v2PDF
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Posted in astro-ph.SR · 2026-01-01 · Hodari-Sadiki Hubbard-James, Sebastian Carrazco-Gaxiola, Todd J. Henry, Leonardo A. Paredes, Azmain H. Nizak, Xavier Lesley-Saldaña, Wei-Chun Jao, Abigail Arbogast

The Solar Neighborhood LV: Spectral Characterization of an Equatorial Sample of 580 K Dwarfs

We present a spectroscopic characterization of 580 K dwarfs within 33 pc, observed with the CHIRON echelle spectrograph (R=80,000) on the SMARTS 1.5m telescope. This volume-limited sample is part of the RKSTAR survey of $\sim$4400 K dwarf primaries within 50 pc. Using Empirical SpecMatch and the diagnostic lines H-alpha (6562.8...

💬 0 commentsarXiv:2601.00462v1PDF
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Posted in physics.soc-ph · 2026-01-01 · Jnanajyoti Bhaumik, Naoki Masuda

Non-dilemmatic social dynamics promote cooperation in multilayer networks

Various theoretical and empirical studies have accounted for why humans cooperate in competitive environments. Although prior work has revealed that network structure and multiplex interactions can promote cooperation, most theory assumes that individuals play similar dilemma games in all social contexts. However, real-world agents...

💬 0 commentsarXiv:2601.00460v1PDF
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Posted in cond-mat.stat-mech · 2026-01-01 · Rik S. Breebaart, Peter G. Bolhuis

Combining multiple interface set path ensembles with MBAR reweighting

We introduce a method to compute the reweighted path ensemble by combining transition interface sampling simulations conditioned on different collective variables. The approach is based on the Multistate Bennett Acceptance Ratio (MBAR) methodology applied to entire trajectories. Illustrating the technique with simple 2D potential...

💬 0 commentsarXiv:2601.00458v1PDF
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Posted in hep-th · 2026-01-01 · Giacomo Cacciapaglia, Wanda Isnard, Roman Pasechnik, Anca Preda

One loop renormalization of 5D gauge-Yukawa theories

The common lore dictates that extra dimensional theories loose predictive power at energies just above the compatification scale, due to the power-law running of bulk coupling. We show that five-dimensional gauge-Yukawa theories can be valid up to arbitrarily high scales, provided: 1) A finite number of terms are required to absorb...

💬 0 commentsarXiv:2601.00453v1PDF
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Posted in astro-ph.CO · 2026-01-01 · V. Kamali, R. Brandenberger

Late Time Magnetogenesis from Ultralight Scalar Dark Matter

Assuming that Dark Matter is an ultralight scalar field which is coupled to electromagnetism via a gauge-kinetic function and which at the time of recombination is oscillating coherently over a Hubble patch, we show that there is a tachyonic instability for the gauge field modes which leads to the generation of magnetic fields on...

💬 0 commentsarXiv:2601.00443v1PDF
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Posted in hep-th · 2026-01-01 · Xi Dong, Donald Marolf, Pratik Rath

The JLMS formula in a large code with approximate error correction

Gauge/gravity duality is often described as a quantum error correcting code. However, as seen in the Jafferis-Lewkowycz-Maldacena-Suh (JLMS) formula, exact quantum error correction with complementary recovery (and thus entanglement wedge reconstruction) emerges only in the limit $G \to 0$. As a result, precise arguments controlling...

💬 0 commentsarXiv:2601.00442v1PDF
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Posted in astro-ph.HE · 2026-01-01 · Konstantinos N. Gourgouliatos

Magnetic plasmoid explosions in the context of magnetar giant flares and fast radio bursts

Magnetar flares are highly energetic and rare events in which intense X and γ-ray emission is released from strongly magnetised neutron stars. The events are also accompanied by mass ejection from the neutron star. Fast radio bursts are short and intense pulses of coherent radio emission. Their large dispersion measures support an...

💬 0 commentsarXiv:2601.00441v2PDF
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Posted in physics.soc-ph · 2026-01-01 · Fredrik Jansson

The dynamics of cultural systems

Culture is not just traits but a dynamic system of interdependent beliefs, practices and artefacts embedded in cognitive, social and material structures. Culture evolves as these entities interact, generating path dependence, attractor states and tension, with long-term stability punctuated by rapid systemic transformations. Cultural...

💬 0 commentsarXiv:2601.00440v1PDF
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Posted in astro-ph.SR · 2026-01-01 · Cheyanne Shariat, Kareem El-Badry

A global view of post-interaction white dwarf-main sequence binaries

Common-envelope evolution (CEE) is among the most uncertain phases in binary evolution. To empirically constrain CEE, we construct a uniformly selected sample of eclipsing post--common-envelope binaries (PCEBs). Starting from an unresolved white dwarf-main-sequence (WDMS) candidate sample within 200 pc selected from the Gaia...

💬 0 commentsarXiv:2601.00439v3PDF
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Posted in astro-ph.CO · 2026-01-01 · Kaili Cao, David H. Weinberg, Vivian Miranda, Nihar Dalal, Tim Eifler, Jiachuan Xu, Haley Bowden

Fisher Forecasts for Cosmological Yields from $3\!\times\!2$pt Analysis of the Roman Space Telescope High Latitude Imaging Survey

The High Latitude Imaging Survey (HLIS) of NASA's Nancy Grace Roman Space Telescope will provide powerful tests of cosmological models through sensitive measurements of cosmic shear, galaxy-galaxy lensing (GGL), and galaxy clustering. As part of the HLIS Project Infrastructure Team's Data Challenge 1 (DC1), we carry out Fisher...

💬 0 commentsarXiv:2601.00438v1PDF