Showing 1–20 of 71 results
/ Date/ Name
Apr 24, 2026Quark Number Susceptibilities and Conserved Charge Fluctuations in $(2+1)$-flavor QCD with Möbius domain-wall fermions (MDWF)Apr 12, 2026First Observation of \boldmath{$D^+ \to a_0(980)ρ$ and $D^+ \to a_0(980)^+ f_0(500)$} in \boldmath{$D^+ \to π^+π^+π^-η$ and $D^+ \to π^+π^0π^0η$} DecaysJan 16, 2026ZPD Detector: Data Selection via Capability-Difficulty Alignment for Large Language ModelsJan 13, 2026AgriAgent: Contract-Driven Planning and Capability-Aware Tool Orchestration in Real-World AgricultureJan 6, 2026Generalized Bloch's Theorem for Cavity Exciton Polaron-PolaritonsNov 18, 2025First measurement of reactor neutrino oscillations at JUNONov 18, 2025Initial performance results of the JUNO detectorNov 17, 2025A Fractional Calculus Framework for Open Quantum Dynamics: From Liouville to Lindblad to Memory KernelsOct 8, 2025Design, waterproofing, and mass production of the 3-inch PMT frontend system of JUNOOct 1, 2025Serendipitous Discovery of an Optically-Dark Ultra-Luminous Infrared Galaxy at $z$ = 3.4Sep 20, 2025ADVEDM:Fine-grained Adversarial Attack against VLM-based Embodied AgentsAug 13, 2025Tight correlation of star formation with [Ci] and CO lines across cosmic timeAug 12, 2025AgriGPT: a Large Language Model Ecosystem for AgricultureJul 25, 2025RealisVSR: Detail-enhanced Diffusion for Real-World 4K Video Super-ResolutionJun 24, 2025A Perspective on Quantum Computing Applications in Quantum Chemistry using 25--100 Logical QubitsJun 18, 2025Dark Count Rate Stability of JUNO 20-inch PMTs in Mass TestingMay 12, 2025Why is the Star Formation Rate Proportional to Dense Gas Mass?Apr 14, 2025NTIRE 2025 Challenge on Cross-Domain Few-Shot Object Detection: Methods and ResultsApr 1, 2025Transfer learning empowers material Z classification with muon tomographyDec 5, 20244D SlingBAG: spatial-temporal coupled Gaussian ball for large-scale dynamic 3D photoacoustic iterative reconstruction