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arXiv preprints from January 1, 2026 through September 13, 2026 — 07:29:39 EST

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Posted in quant-ph · 2026-01-21 · Johannes Jakob Meyer, Jacopo Rizzo, Asad Raza, Lorenzo Leone, Sofiene Jerbi, Jens Eisert

The computational two-way quantum capacity

Quantum channel capacities are fundamental to quantum information theory. Their definition, however, does not limit the computational resources of sender and receiver. In this work, we initiate the study of computational quantum capacities. These quantify how much information can be reliably transmitted when imposing the natural...

💬 0 commentsarXiv:2601.15393v1PDF
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Posted in cs.AI · 2026-01-21 · Francesca Pia Panaccione, Carlo Sgaravatti, Pietro Pinoli

GeMM-GAN: A Multimodal Generative Model Conditioned on Histopathology Images and Clinical Descriptions for Gene Expression Profile Generation

Biomedical research increasingly relies on integrating diverse data modalities, including gene expression profiles, medical images, and clinical metadata. While medical images and clinical metadata are routinely collected in clinical practice, gene expression data presents unique challenges for widespread research use, mainly due to...

💬 0 commentsarXiv:2601.15392v1PDF
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Posted in physics.plasm-ph · 2026-01-21 · T. Adkins, I. G. Abel, M. Barnes, S. Buller, W. Dorland, P. G. Ivanov, R. Meyrand, F. I. Parra, A. A. Schekochihin, J. Squire

Asymptotic scaling theory of electrostatic turbulent transport in magnetised fusion plasmas

Turbulent transport remains one of the principal obstacles to achieving efficient magnetic confinement in fusion devices. Two of the dominant drivers of the turbulence are microscale instabilities fuelled by electron- and ion-temperature gradients (ETG and ITG), whose nonlinear saturation determines the cross-field transport of...

💬 0 commentsarXiv:2601.15391v1PDF
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Posted in cs.LG · 2026-01-21 · Zhaolong Su, Leheng Zhao, Xiaoying Wu, Ziyue Xu, Jindong Wang

FedUMM: A General Framework for Federated Learning with Unified Multimodal Models

Unified multimodal models (UMMs) are emerging as strong foundation models that can do both generation and understanding tasks in a single architecture. However, they are typically trained in centralized settings where all training and downstream datasets are gathered in a central server, limiting the deployment in privacy-sensitive...

💬 0 commentsarXiv:2601.15390v1PDF
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Posted in math.CO · 2026-01-21 · Hin Chung Henry Tsang

Maximal Green Sequences for Cluster Algebras Associated to Closed Orbifolds

It is known that the existence of a maximal green sequence for a quiver associated to surfaces is equivalent to the equality of the cluster algebra and upper cluster algebra generated by the quiver. This paper makes the first steps in investigating this behavior in the generalised case of cluster algebras from orbifolds; determining...

💬 0 commentsarXiv:2601.15389v1PDF
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Posted in q-bio.PE · 2026-01-21 · Alison M. V. D. L. Melo, Matheus C. Santos

Final size of a structured SIRD Model with active-population force of infection

We consider a SIRD epidemic model for a population composed of two groups of individuals with asymmetric interactions, where the force of infection depends on the active (alive) population in each group, rather than on the total population, as in the classical formulation. We prove that the final state for susceptible individuals is...

💬 0 commentsarXiv:2601.15388v1PDF
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Posted in astro-ph.SR · 2026-01-21 · Daisuke Taniguchi, Patrick de Laverny, Alejandra Recio-Blanco, Takuji Tsujimoto, Pedro A. Palicio

Solar twins in Gaia DR3 GSP-Spec I. Building a large catalog of Solar twins with ages

[Abbreviated] Context. Solar twins, stars whose stellar parameters (Teff, log g, and [M/H]) are very close to the Solar ones, offer a unique opportunity to investigate Galactic archaeology with very high accuracy and precision. However, most previous catalogs of Solar twins contain only a small number of objects (typically a few...

💬 0 commentsarXiv:2601.15387v1PDF
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Posted in cond-mat.str-el · 2026-01-21 · Misha Yutushui, David F. Mross

Theory of Next-Generation Even-Denominator States

Even-denominator quantum Hall states are leading candidates for realizing non-Abelian topological orders, with the $ν=\frac{5}{2}$ plateau in GaAs the first and most-studied example. Recent experiments in GaAs and bilayer graphene (BLG) have observed many `next-generation' even-denominator states at filling factors such as...

💬 0 commentsarXiv:2601.15386v1PDF
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Posted in cs.HC · 2026-01-21 · Marko Hostnik, Rauf Kurbanov, Yaroslav Sokolov, Artem Trofimov

VegaChat: A Robust Framework for LLM-Based Chart Generation and Assessment

Natural-language-to-visualization (NL2VIS) systems based on large language models (LLMs) have substantially improved the accessibility of data visualization. However, their further adoption is hindered by two coupled challenges: (i) the absence of standardized evaluation metrics makes it difficult to assess progress in the field and...

💬 0 commentsarXiv:2601.15385v1PDF
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Posted in astro-ph.GA · 2026-01-21 · Maura Kathleen Shea, D. Michael Crenshaw, Travis C. Fischer, Mitchell Revalski, Julia Falcone, Beena Meena, Zo Chapman, Jacob Tutterow, Madeline Davis, Kesha Patel

An Analysis of AGN Feedback in the Compact Galaxy Group Stephan's Quintet

Compact galaxy groups are ideal laboratories for studying the effects of interactions between AGN and multiple nearby galaxies. Recent JWST observations of the nearby compact group Stephan's Quintet highlight tidal flows between the interacting galaxies as well as outflows from the active galaxy NGC 7319. To study the kinematics on a...

💬 0 commentsarXiv:2601.15384v1PDF
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Posted in astro-ph.GA · 2026-01-21 · Krista Lynne Smith, Macon Magno, Michael Koss

An Investigation of 5-year Simultaneous X-ray and Radio Light Curves of the Dwarf Seyfert Galaxy UGC 6728

We present serendipitous simultaneous radio and X-ray light curves of the dwarf Seyfert galaxy UGC 6728 spanning 5 years. The X-ray light curve exhibits a flaring period, followed by a gradual rise and decline. Throughout these events, the X-ray hardness ratio and spectrum do not change significantly. The radio flux is constant, as...

💬 0 commentsarXiv:2601.15383v1PDF
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Posted in astro-ph.GA · 2026-01-21 · Salmoli Ghosh, P. Kharb, E. Costantini, J. Gallimore, D. Williams-Baldwin, M. Mehdipour

A Stratification in Magnetic Field Structures: The Radio Outflow in NGC 4151

The nature of radio outflows in radio-quiet AGN remains poorly understood. In this study, we present kpc-scale polarization observations of the Seyfert galaxy NGC\,4151 using the Karl G. Jansky Very Large Array (VLA) in B-array at 3 and 10 GHz. We find that the inferred magnetic (B-) field structures show a stratification: a...

💬 0 commentsarXiv:2601.15382v1PDF
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Posted in astro-ph.GA · 2026-01-21 · Nathan Secrest, Sebastien Lambert

Blazars define a stable celestial reference frame

Recent work has shown that optical-radio position offsets and radio position variability are inversely correlated with the photometric variability of active galactic nuclei (AGN). A key prediction of these findings is that a reference frame constructed using highly photometrically variable AGN should be more stable than a frame that...

💬 0 commentsarXiv:2601.15381v1PDF
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Posted in cs.LG · 2026-01-21 · Elon Litman, Gabe Guo

You Need Better Attention Priors

We generalize the attention mechanism by viewing it through the lens of Entropic Optimal Transport, revealing that standard attention corresponds to a transport problem regularized by an implicit uniform prior. We introduce Generalized Optimal transport Attention with Trainable priors (GOAT), a new attention mechanism that replaces...

💬 0 commentsarXiv:2601.15380v1PDF
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Posted in astro-ph.GA · 2026-01-21 · Sebastian Banaszak, Caitlin Witt, Adam Miller

Optimizing Optical Searches for Supermassive Black Hole Binaries in AGN Light Curves: Fourier versus Bayesian Periodicity Detection

Simulations predict that supermassive black hole binaries (SMBHBs) will exhibit periodic brightness variations that may exceed the stochastic variability intrinsic to active galactic nuclei (AGN). In this paper, we simulate SMBHBs with damped random walk (DRW) AGN variability and an added sinusoidal signal from the orbital motion, and...

💬 0 commentsarXiv:2601.15379v1PDF
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Posted in astro-ph.CO · 2026-01-21 · Simone Sartori, Sofia Contarini, Elena Sarpa, Giulia Degni, Federico Marulli, Stephanie Escoffier, Lauro Moscardini

The Back-in-time Void Finder: dynamical identification of cosmic voids through optimal transport reconstruction

Cosmic voids have increasingly emerged as a powerful cosmological probe. However, their large spatial extent and intrinsically underdense environments make their identification highly sensitive to shot noise, redshift-space distortions (RSD), and observational systematics, particularly for topological and density-based void...

💬 0 commentsarXiv:2601.15378v1PDF
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Posted in hep-ph · 2026-01-21 · Murshed Alam, Vedran Brdar, Dibya S. Chattopadhyay

Exploring Quantumness at Long-Baseline Neutrino Experiments

Violations of classicality can be probed through measurements performed on a system at different times, as proposed by Leggett and Garg. Specifically, violations of Leggett-Garg inequalities suggest the presence of quantum effects in macroscopic systems. Long-baseline neutrino experiments provide some of the longest available...

💬 0 commentsarXiv:2601.15375v1PDF
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Posted in hep-th · 2026-01-21 · Aritra Banerjee, Pulastya Parekh, Robin Raj

On $\sqrt{T\overline{T}}$ deformed pathways: CFT to CCFT

We discuss the marginal $\sqrt{T\overline{T}}$ deformation of massless scalar field theories in two dimensions from a dynamical perspective. The operator flow equations for such deformations induce a particular Legendre Transformation between flowed Lagrangians and flowed Hamiltonians. The marginal deformation does not change the...

💬 0 commentsarXiv:2601.15376v4PDF
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Posted in cond-mat.str-el · 2026-01-21 · Laura Shou, Jeet Shah, Matthew Lerner-Brecher, Amol Aggarwal, Alexei Borodin, Victor Galitski

Exactly Solvable Topological Phase Transition in a Quantum Dimer Model

We consider a family of generalized Rokhsar-Kivelson (RK) Hamiltonians, which are reverse-engineered to have an arbitrary edge-weighted superposition of dimer coverings as their exact ground state at the RK point. We focus on a quantum dimer model on the triangular lattice, with doubly-periodic edge weights. For simplicity we consider...

💬 0 commentsarXiv:2601.15377v3PDF
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Posted in astro-ph.GA · 2026-01-21 · David Chemaly, Elisabeth Sola, Vasily Belokurov, Sergey Koposov, GyuChul Meyong, HanYuan Zhang, Denis Erkal

Constraining the population of dark matter halo shapes using hierarchical inference with extragalactic stellar streams

Stellar streams, the debris of tidally disrupted satellites, trace their host's gravitational potential and thus probe dark matter halo structure. While six-dimensional phase-space data of Galactic streams enable precise dark matter halo modelling in the Milky Way, streams around external galaxies are typically available only as low...

💬 0 commentsarXiv:2601.15373v3PDF
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Posted in astro-ph.SR · 2026-01-21 · Fernando A. Olguin, Patricio Sanhueza, Yoko Oya, Adam Ginsburg, Maria T. Beltrán, Kaho Morii, Roberto Galván-Madrid, Huei-Ru Vivien Chen, Qiuyi Luo, Kei E. I. Tanaka, Suinan Zhang, Yu Cheng, Fumitaka Nakamura, Shanghuo Li, Kotomi Taniguchi, Guido Garay, Qizhou Zhang, Masao Saito, Takeshi Sakai, Xing Lu, Jixiang Weng, Andrés E. Guzmán

Digging into the Interior of Hot Cores with ALMA (DIHCA). VII. Disk candidates around high-mass stars and evidence of anisotropic infall

We study the kinematics of condensations in 30 fields forming high-mass stars with ALMA at a high-resolution of ~0.08'' on average (~230 au). The presence of disks is important for feeding high-mass stars without feedback halting growth as their masses increase. In the search for velocity gradients resembling rotation that can reveal...

💬 0 commentsarXiv:2601.15371v1PDF
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Posted in astro-ph.GA · 2026-01-21 · Shravya Shenoy, Daniel J. B. Smith, Sarah K. Biddle, Gülay Gürkan, Martin J. Hardcastle, Marina I. Arnaudova, Soumyadeep Das, Luke R. Holden, Gaoxiang Jin, Leah K. Morabito, Huub J. A. Röttgering

What factors shape the radio luminosity of star-forming galaxies? A new calibration from LoTSS-DR2

Radio observations offer a dust-unobscured view of galaxy star formation via the radio continuum-star formation rate (RC--SFR) relation. Emerging evidence of a stellar mass dependence in the RC--SFR relation raises the broader question of how other galaxy properties may influence this relation. In this work, we study the dependence of...

💬 0 commentsarXiv:2601.15374v1PDF
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Posted in hep-ph · 2026-01-21 · Damiano F. G. Fiorillo, Georg G. Raffelt

Single-wave solutions of the neutrino fast flavor system. Part I. Mechanical properties

A dense neutrino plasma can exhibit collective flavor evolution caused by neutrino--neutrino refraction. Recently, a new class of exact nonlinear inhomogeneous solutions was discovered: single-wave (SW) solutions of the fast flavor system. The key property is that the flavor occupation numbers remain homogeneous, whereas the field of...

💬 0 commentsarXiv:2601.15372v2PDF
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Posted in astro-ph.GA · 2026-01-21 · A. Ahmed, W. H. Elsanhoury, D. C. Çınar, S. Taşdemir, R. Canbay, A. A. Haroon, M. S. Alenazi

Tracing the Galactic Disk with Gaia DR3: A Deep Study of Berkeley 17, 18, and 39 Open Star Clusters

We report a detailed investigation of three intermediate-to-old age open clusters, Berkeley 17, Berkeley 18, and Berkeley 39, utilizing precise astrometric and photometric data from Gaia DR3. Cluster membership was robustly determined through a probabilistic proper-motion analysis, yielding statistically significant samples of 600,...

💬 0 commentsarXiv:2601.15289v1PDF
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Posted in cs.CV · 2026-01-21 · Jiwon Kang, Yeji Choi, JoungBin Lee, Wooseok Jang, Jinhyeok Choi, Taekeun Kang, Yongjae Park, Myungin Kim, Seungryong Kim

APPLE: Attribute-Preserving Pseudo-Labeling for Diffusion-Based Face Swapping

Face swapping aims to transfer the identity of a source face onto a target face while preserving target-specific attributes such as pose, expression, lighting, skin tone, and makeup. However, since real ground truth for face swapping is unavailable, achieving both accurate identity transfer and high-quality attribute preservation...

💬 0 commentsarXiv:2601.15288v2PDF