Showing 401–420 of 6,054 results
/ Date/ Name
Apr 9, 2025Kernpiler: Compiler Optimization for Quantum Hamiltonian Simulation with Partial TrotterizationApr 7, 2025The UV Legacy Library of Young Stars as Essential Standards (ULLYSES) Large Director's Discretionary Program with Hubble. I. Goals, Design, and Initial ResultsApr 4, 2025Constraints on dark matter boosted by supernova shock within the effective field theory framework from the CDEX-10 experimentApr 3, 2025Stellar CoRGI in MaNGA: Stellar Counterrotating Galaxies Identified in the MaNGA SurveyApr 3, 2025Detection of Deuterated Hydrocarbon Nanoparticles in the Whirlpool Galaxy, M51Apr 3, 2025Measurement of the transverse energy density in Au+Au collisions at $\sqrt{s_{NN}} = 200$ GeV with the sPHENIX detectorApr 3, 2025Measurement of charged hadron multiplicity in Au+Au collisions at $\sqrt{\text{s}_{\text{NN}}} = 200$ GeV with the sPHENIX detectorApr 2, 2025Studying stellar populations in Omega Centauri with phylogeneticsApr 1, 2025Study of Ultra-High-Energy Gamma-Ray Source 1LHAASO J0056+6346u and Its Possible OriginsApr 1, 2025LEP3: A High-Luminosity e+e- Higgs and ElectroweakFactory in the LHC TunnelMar 31, 2025The International Axion Observatory (IAXO): case, status and plans. Input to the European Strategy for Particle PhysicsMar 31, 2025Quasinormal modes and excitation factors of Kerr black holesMar 31, 2025European Contributions to Fermilab Accelerator Upgrades and Facilities for the DUNE ExperimentMar 31, 2025DUNE Software and Computing Research and DevelopmentMar 30, 2025The DUNE Phase II DetectorsMar 30, 2025The DUNE Science ProgramMar 29, 2025Interpretable Graph Kolmogorov-Arnold Networks for Multi-Cancer Classification and Biomarker Identification using Multi-Omics DataMar 28, 2025Diffraction around caustics in gravitational wave lensingMar 28, 2025Multiplicity and net-electric charge fluctuations in central Ar+Sc interactions at 13A, 19A, 30A, 40A, 75A, and 150A GeV/c beam momenta measured by NA61/SHINE at the CERN SPSMar 27, 2025Binarity at LOw Metallicity (BLOeM): Enhanced multiplicity of early B-type dwarfs and giants at $Z=0.2\,{\rm Z}_\odot$