Showing 101–120 of 6,168 results
/ Date/ Name
Jan 27, 2026POEMMA-Balloon with Radio: A multi-messenger, multi-detector balloon payloadJan 23, 2026Longitudinal Dynamics of Large and Small Systems from a 3D Bayesian Calibration of RHIC Top-energy Collision DataJan 22, 2026Large-scale real-time signal processing in physics experiments: The ALICE TPC FPGA pipelineJan 20, 2026Gilbert Damping Parameters of Epitaxially-Stabilized Iron Gallium Thin Films from Ferromagnetic ResonanceJan 20, 2026The JEM-EUSO Collaboration: Contributions to the 39th International Cosmic Ray Conference (ICRC2025)Jan 20, 2026Optimising gravitational-wave sky maps for pulsar timing arraysJan 19, 2026Locating the missing large-scale emission in the jet of M87* with short EHT baselinesJan 16, 2026Study of the anisotropy of cosmic expansion on ZTF type Iasupernovae simulationsJan 13, 2026Fractional-Monolayer 2D-GaN/AlN Structures: Growth Kinetics and UVC-emitter ApplicationsJan 13, 2026RotCurves: A PYTHON package for efficient modelling and fitting of galactic rotation curves at high-zJan 8, 2026QCD Crossover at Low Temperatures from Lee-Yang Edge SingularityJan 7, 2026Detector characterization for a new $^{12}$C+$^{12}$C reaction study at LUNAJan 6, 2026Differential cross sections for ${{^{12}\mathrm{C}(n,α_{0})}}$, ${{^{16}\mathrm{O}(n,α_{0})}}$ and ${{^{16}\mathrm{O}(n,α_{1,2,3})}}$ between ${E_n}$ = 7.2 and 10 MeV with an active-target Time Projection ChamberJan 5, 2026Gas rotation and turbulence in the galaxy cluster Abell 2029Jan 5, 2026Lévy walkers inside spherical shells with absorbing boundaries: Towards settling the optimal Lévy walk strategy for random searchesJan 5, 2026A 500 pc volume-limited sample of hot subluminous stars II. Atmospheric parameters, mass distribution, and kinematicsJan 4, 2026Hilbert space signatures of non-ergodic glassy dynamicsJan 2, 2026High-Temperature Deformation Behavior of Co-Free Non-Equiatomic CrMnFeNi AlloyDec 24, 2025Observation of disorder-induced superfluidityDec 23, 2025Alfvénic solar wind intervals observed by Solar Orbiter: Exploiting the capability of the SWA plasma suite and source region investigation