Qwen Councils
arXiv could not process that search. Try a simpler keyword search or an arXiv field query such as all:quantum.
Showing downloaded papers while arXiv is unavailable.

Physics

arXiv preprints from January 1, 2026 through July 20, 2026 — 17:24:35 EST

0

Posted in math-ph · 2026-01-13 · Luisiana X. Cundin

Newell-Whitehead-Segel equation,A Simpler Proof

Previous analysis of the Newell-Whitehead-Segel equation proved the best solution is null; although, the method of solution generated complex nested integrals, therefore, difficult to analyze \cite{NWSgen,NWS2020}. Recent insights into the properties of the convolution integral enable considerable simplification of the solution in the...

💬 0 commentsarXiv:2601.08965v1PDF
0

Posted in astro-ph.EP · 2026-01-13 · Peter L. Olson, Zachary D. Sharp, Susmita Garai

Depletion of moderately volatile elements by pebble accretion in Earth-like planets

Protoplanets growing by pebble accretion capture massive hydrogen-helium atmospheres from the surrounding nebula. Pebbles settling through such atmospheres continuously release gravitational potential energy, heating both the atmosphere and the pebbles. Under these conditions, atmosphere temperatures above large protoplanets are...

💬 0 commentsarXiv:2601.08958v1PDF
0

Posted in astro-ph.EP · 2026-01-13 · S. I. Ipatov

Formation and evolution of planetary systems

Various problems of the formation and evolution of planetary systems are studied. Most of the studies are devoted to the Solar System. The collapse of the presolar cloud and the accumulation of planets are studied. The author considers the formation of the Earth-Moon system, binary trans-Neptunian objects, and the axial rotations of...

💬 0 commentsarXiv:2601.08952v1PDF
0

Posted in astro-ph.SR · 2026-01-13 · Shih-Ying Hsu, Nadia M. Murillo, Chin-Fei Lee, Doug Johnstone, Tien-Hao Hsieh, Naomi Hirano, Leonardo Bronfman, Yo-Ling Chuang, David J. Eden, Shanghuo Li, Sheng-Jun Lin, Mark G. Rawlings, Ken'ichi Tatematsu, Sheng-Yuan Liu, Huei-Ru Vivien Chen, Kee-Tae Kim, Yi-Jehng Kuan, Woojin Kwon, Chang Won Lee, Jeong-Eun Lee, Tie Liu, Qiuyi Luo, Patricio Sanhueza, Hsien Shang

HOPS-288: A Laboratory for Complex Organics in Proto-multiple Systems

Complex organic molecules (COMs) in young stellar objects (YSOs) have attracted significant attention in recent years due to their potential connection to pre-biotic chemistry and their utility as tracers of warm or shocked gas components. Proto-binary and multiple systems with close separations are particularly valuable targets for...

💬 0 commentsarXiv:2601.08948v1PDF
0

Posted in cond-mat.str-el · 2026-01-13 · Matt Boswell, Mingyu Xu, Haozhe Wang, Mouyang Cheng, N. Li, X. F. Sun, Haidong Zhou, Huibo Cao, Mingda Li, Weiwei Xie

Frustrated Magnetism in FeGe$_3$O$_4$ with a Chiral Trillium Network

The discovery of new magnetic ground states in geometrically frustrated lattices remains a central challenge in materials science. Here, we report the synthesis, structural characterization, and frustrated magnetic properties of FeGe$_3$O$_4$, a newly identified compound that crystallizes in the noncentrosymmetric cubic space group...

💬 0 commentsarXiv:2601.08947v1PDF
0

Posted in quant-ph · 2026-01-13 · P. A. Stuermer, D. Wirtitsch, T. Steidl, R. Wörnle, J. Körber, W. Schustereder, C. Zmoelnig, P. Urlesberger, F. Chiapolino, S. Meinardi, K. Edelmann, M. Kern, J. Anders, S. Krainer, H. Heiss, M. Trupke, J. Wrachtrup

Demonstration Of A Quantum Magnetometer Chip Based On Proprietary And Scalable 4H-Silicon Carbide Technology

This work presents an industrially scalable, power-efficient and high-performance quantum magnetometer chip based on proprietary 4H-silicon carbide (SiC) technology, leveraging wafer-scale fabrication techniques to optimize V2 silicon vacancy color centers for highly reproducible, industry-grade fabrication with precise control of...

💬 0 commentsarXiv:2601.08945v1PDF
0

Posted in astro-ph.CO · 2026-01-13 · Axel de la Macorra, Jose Agustin Lozano Torres

Bound Dark Energy: Particle Physics model in alignment with recent DESI cosmological measurements

We present observational constraints on the Bound Dark Energy Cold Dark Matter (BDE-CDM) model using DESI DR2 baryon acoustic oscillation measurements combined with Planck CMB data and Type Ia supernovae compilations (PantheonPlus, Union3, DESY5). In BDE-CDM, dark energy originates from the lightest meson field within a supersymmetric...

💬 0 commentsarXiv:2601.08943v1PDF
0

Posted in astro-ph.GA · 2026-01-13 · S. Katsioli, E. M. Xilouris, F. Galliano, R. Adam, P. Ade, H. Ajeddig, S. Amarantidis, P. André, H. Aussel, M. Baes, A. Beelen, A. Benoît, S. Berta, A. Bongiovanni, J. Bounmy, O. Bourrion, M. Calvo, A. Catalano, D. Chérouvrier, I. De Looze, M. De Petris, F. -X. Désert, S. Doyle, E. F. C. Driessen, G. Ejlali, A. Ferragamo, A. Gomez, J. Goupy, C. Hanser, A. Hughes, A. P. Jones, F. Kéruzoré, C. Kramer, B. Ladjelate, G. Lagache, S. Leclercq, J. -F. Lestrade, J. F. Macías-Pérez, S. C. Madden, A. Maury, F. Mayet, A. Monfardini, A. Moyer-Anin, M. Muñoz-Echeverría, I. Myserlis, A. Nersesian, A. Paliwal, L. Pantoni, D. Paradis, L. Perotto, G. Pisano, N. Ponthieu, V. Revéret, A. J. Rigby, A. Ritacco, H. Roussel, F. Ruppin, M. Sánchez-Portal, S. Savorgnano, K. Schuster, A. Sievers, M. W. L. Smith, F. Tabatabaei, J. Tedros, C. Tucker, N. Ysard, R. Zylka

Resolved ISM properties and scaling relations in the barred galaxy NGC 3627: constraints from NIKA2 observations

We investigate the interplay between star formation, interstellar medium (ISM) components, and dust properties in NGC 3627 using new NIKA2 1.15 and 2 mm observations from the IMEGIN Large Program. Our goal is to analyze dust and radio emission, decompose contributions in the millimeter-centimeter regime, and explore ISM properties...

💬 0 commentsarXiv:2601.08941v1PDF
0

Posted in astro-ph.GA · 2026-01-13 · B. Agís-González, D. Hutsemékers, I. Liodakis, S. Cazzoli, D. Sluse, G. Miniutti, I. Márquez, J. Masegosa, F. Marin, J. A. Acosta-Pulido, C. Ramos Almeida

Polarization echoes from past nuclear activity in the quasi-periodic eruption source GSN 069

Context. X-ray quasi-periodic eruptions (QPEs) are repeating, high-amplitude, soft X-ray bursts observed from the nuclei of a dozen nearby low-mass galaxies. Their origin remains a puzzle in the physics of accretion variability. Observational data indicate that X-ray and/or optical tidal disruption events (TDEs) may precede QPE...

💬 0 commentsarXiv:2601.08940v1PDF
0

Posted in astro-ph.GA · 2026-01-13 · Bianca Moreschini, Francesco Belfiore, Alessandro Marconi, Elisa Cataldi, Mirko Curti, Amirnezam Amiri, Anna Feltre, Filippo Mannucci, Elena Bertola, Caterina Bracci, Matteo Ceci, Avinanda Chakraborty, Giovanni Cresci, Quirino D'Amato, Enrico di Teodoro, Michele Ginolfi, Isabella Lamperti, Cosimo Marconcini, Martina Scialpi, Lorenzo Ulivi, Maria Vittoria Zanchettin

One cloud is not enough: extreme conditions bias chemical abundances in high-redshift galaxies

Since its launch, JWST has opened an unprecedented opportunity to characterise the ionised ISM of high-redshift galaxies using well-established rest-frame UV/optical diagnostics from the local Universe. At the same time, these observations challenge the validity of such classical methods when applied to the extreme environments...

💬 0 commentsarXiv:2601.08939v1PDF
0

Posted in astro-ph.EP · 2026-01-13 · Michael L. Weber, Barbara Ercolano, Giovanni Picogna

Can photoevaporation open gaps in protoplanetary discs?

We investigate whether photoevaporation alone can open and sustain gaps in protoplanetary discs by coupling the evolving disc structure with the photoevaporative flow in two dimensional radiation hydrodynamical simulations. Our results show that once a density depression forms, the local mass-loss rate decreases sharply, suppressing...

💬 0 commentsarXiv:2601.08938v1PDF
0

Posted in astro-ph.GA · 2026-01-12 · Rafael Bertolotto-Stefanelli, Juan José Downes, Genaro Suárez, Cecilia Mateu, Jonathan Gagné, Carlos Román Zúñiga

The stellar initial mass function of nearby young moving groups

The solar neighbourhood is populated by nearby, young moving groups (NYMGs) of stars that are candidates to be remnants of individual stellar clusters and associations, currently dispersing in the galactic disc. To derive the initial mass function (IMF) of a large sample of NYMGs, we developed and applied an algorithm that uses...

💬 0 commentsarXiv:2601.07184v1PDF
0

Posted in gr-qc · 2026-01-12 · Haorong Wu, Xilong Fan

Chiroptical effect induced by gravitational waves

We propose the gravitational analog of the chiroptical effect for the first time, demonstrating that gravitational waves (GWs) can induce a reversal of photon chirality through the exchange of angular momentum, namely the spin-2-gravitation chiroptical effect. By analyzing the interaction between photon spin angular momentum (SAM) and...

💬 0 commentsarXiv:2601.07179v1PDF
0

Posted in astro-ph.HE · 2026-01-12 · Zhipeng Huang, Zhen Yan, Zhiqiang Shen, Hao Tong, Mingyu Ge, Zhifu Gao, Yajun Wu, Rongbing Zhao, Jie Liu, Rui Wang, Xiaowei Wang, Fan Yang, Chuyuan Zhang, Zhenlong Liao, Yangyang Lin

Does the radio-active phase of XTE~J1810$-$197 recur following the same evolutionary pattern?

Magnetars are the most strongly magnetized compact objects known in the Universe and are regarded as one of the primary engines powering a variety of enigmatic, high-energy transients. However, our understanding of magnetars remains highly limited, constrained by observational sample size and radiative variability. XTE~J1810$-$197,...

💬 0 commentsarXiv:2601.07173v1PDF
0

Posted in astro-ph.GA · 2026-01-12 · Shaobo Zhang, Xianhuan Lei, Hui Zhu, Xueying Hu, Xiaohong Cui, Wenwu Tian, Haiyan Zhang, Dan Wu

A Study Revealing Physical Attributes of Supernova Remnant in G321.3-3.9

We present a radio analysis of the recently identified supernova remnant G321.3-3.9 using archival multi-wavelength data spanning 88-2304 MHz. The source exhibits an elliptical shell-like morphology (1.3 deg x 1.7 deg) and a relatively flat non-thermal spectral index of alpha = -0.40 +/- 0.03. The distance is estimated using both the...

💬 0 commentsarXiv:2601.07170v1PDF
0

Posted in physics.plasm-ph · 2026-01-12 · Tian Shuang, Zhang Han, Zhang Xi, Zhang Xuexue, Li Qing, Li Xuecehng, Run Junxia

Discharge characteristics and parameter diagnosis of dielectric barrier discharge patterns in double-gap configuration

Pattern discharge is a common mode in dielectric barrier discharge (DBD) and has broad application prospects in various industrial fields, such as material surface treatment, environmental monitoring, and biomedical applications. In this work, a mixed gas of 75% argon and 25% air is used to generate a pattern discharge. A double-gap...

💬 0 commentsarXiv:2601.07167v1PDF
0

Posted in physics.flu-dyn · 2026-01-12 · Jun Wang, Shanhe Pang, Zhiyuan Che, Chang Liu, Zhongxia Du, Xilai Hu, Yanyong Li, Bo Wang, Lei Shi, Konstantin Y. Bliokh, Y. Shen

Dynamic Water-Wave Tweezers

Following a recent demonstration of stable trapping of floating particles by stationary (monochromatic) structured water waves [Nature 638, 394 (2025)], we report dynamic water-wave tweezers that enable controllable transport of trapped particles along arbitrary trajectories on the water surface. We employ a triangular lattice formed...

💬 0 commentsarXiv:2601.07166v1PDF
0

Posted in hep-ph · 2026-01-12 · Anthony G. Williams

Perspectives on QCD, Topology and the Strong CP Problem

On the basis of allowed local gauge symmetries, the QCD Lagrangian admits a CP-violating term proportional to the topological charge density, commonly referred to as the $θ$ term. A priori, any value of $θ$ is consistent with the local symmetries of the theory, while current experimental limits constrain $θ\lesssim 10^{-10}$. The...

💬 0 commentsarXiv:2601.07165v2PDF
0

Posted in astro-ph.GA · 2026-01-12 · Yan Gong, Jiaqiang Zhong, Yuan Ren, Yilong Zhang, Daizhong Liu, Yiping Ao, Qijun Yao, Wen Zhang, Wei Miao, Zhenhui Lin, Wenying Duan, Dong Liu, Kangmin Zhou, Jie Liu, Zheng Wang, Junda Jin, Kun Zhang, Feng Wu, Jinpeng Li, Boliang Liu, Xuan Zhang, Zhengheng Luo, Jiameng Wang, Huiqian Hao, Xingming Lu, Shaoming Xie, Jia Quan, Yanjie Liu, Jingtao Liang, Xianjin Deng, Jun Jiang, Li Li, Liang Guo, Tuo Ji, Peng Jiang, Yi Zhang, Chenggang Shu, Sudeep Neupane, Ruiqing Mao, Shengcai Shi, Jing Li

First Submillimeter Lights from Dome A: Tracing the Carbon Cycle in the Feedback of Massive Stars

The cycling of carbon between its ionized, atomic, and molecular phases shapes the chemical compositions and physical conditions of the interstellar medium (ISM). However, ground-based studies of the full carbon cycle have been limited by atmospheric absorption. Dome~A, the most promising site for submillimeter astronomy, has long...

💬 0 commentsarXiv:2601.07162v1PDF
0

Posted in astro-ph.EP · 2026-01-12 · Jacob Haqq-Misra

Limit cycles and the climate history of Mars

Evidence for fluvial features and standing liquid water indicate that Mars was a warmer and wetter place in its past; however, climate models have historically been unable to produce conditions to yield a warm early Mars under the faint young sun. Some models invoke thick greenhouse atmospheres to produce continuously warm conditions,...

💬 0 commentsarXiv:2601.07159v2PDF
0

Posted in quant-ph · 2026-01-12 · Qianlong Wang, Sven Ahrens, Baifei Shen

Strong coupling of virtual negative states in the Kapitza-Dirac effect

Negative states are an intrinsic property of relativistic quantum theory and related to anti-particles in the context of the Dirac sea concept. We show that negative states can dominantly contribute to the diffraction amplitude in the quantum dynamics of the two-photon Kapitza-Dirac effect. We draw our conclusion by investigating...

💬 0 commentsarXiv:2601.07157v2PDF
0

Posted in astro-ph.IM · 2026-01-12 · Sathwik Narkedimilli, Satvik Raghav, Om Mishra, Mohan Kumar, Aswath Babu H, Tereza Jerabkova, Manish M, Sai Prashanth Mallellu

Explainable Galaxy Interaction Prediction with Hybrid Attention Mechanisms

Galaxy interaction classification remains challenging due to complex morphological patterns and the limited interpretability of deep learning models. We propose an attentive neural ensemble that combines AG-XCaps, H-SNN, and ResNet-GRU architectures, trained on the Galaxy Zoo DESI dataset and enhanced with LIME to enable explainable...

💬 0 commentsarXiv:2601.08872v1PDF
0

Posted in astro-ph.SR · 2026-01-12 · Umberto Battino, Claudia Lederer-Woods, Claudia Travaglio, Friedrich Konrad Röpke, Brad Gibson

Slow White Dwarf Mergers as a New Galactic Source of Trans-Iron Elements

The astrophysical origins of the heaviest stable elements that we observe today in the Solar System are still not fully understood. Recent studies have demonstrated that H-accreting white dwarfs (WDs) in a binary sys- tem exploding as type Ia supernovae could be an efficient p-process source beyond iron. However, both observational...

💬 0 commentsarXiv:2601.07151v1PDF
0

Posted in physics.soc-ph · 2026-01-12 · Yuxin Geng, Wolfram Barfuss, Feng Fu, Xingru Chen

Dynamics of Multi-Agent Actor-Critic Learning in Stochastic Games: from Multistability and Chaos to Stable Cooperation

Achieving robust coordination and cooperation is a central challenge in multi-agent reinforcement learning (MARL). Uncovering the mechanisms underlying such emergent behaviors calls for a dynamical understanding of learn processes. In this work, we investigate the dynamics of actor-critic agents in stochastic games, focusing on the...

💬 0 commentsarXiv:2601.07142v1PDF
0

Posted in cond-mat.str-el · 2026-01-12 · Qiong Qin, Toshihiro Sato, Marcin Raczkowski, Jeroen van den Brink, Congjun Wu, Fakher F. Assaad

Revealing altermagnetic Fermi surfaces with two Kondo impurities

Motivated by recent advances in the study of altermagnetism, or unconventional magnetism, and in the realization and manipulation of two-impurity Kondo physics in real materials, we propose a phase-sensitive method to explore unconventional magnetic symmetries. Our method can be implemented with spin-resolved scanning tunneling...

💬 0 commentsarXiv:2601.07138v1PDF