Showing 21–40 of 182 results
/ Date/ Name
Apr 19, 2024Determination of the CKM angle $φ_{3}$ from a combination of Belle and Belle II resultsApr 16, 2024Social Choice Should Guide AI Alignment in Dealing with Diverse Human FeedbackMar 30, 2024Angular analysis of $B \to K^* e^+ e^-$ in the low-$q^2$ region with new electron identification at BelleMar 15, 2024Measurement of the 1-jettiness event shape observable in deep-inelastic electron-proton scattering at HERAMar 13, 2024Observation and differential cross section measurement of neutral current DIS events with an empty hemisphere in the Breit frameJan 9, 2024Hydrogen Epoch of Reionization Array (HERA) Phase II Deployment and CommissioningDec 20, 2023Search for the $e^+e^-\toη_{b}(1S)ω$ and $e^+e^-\toχ_{b0}(1P)ω$ processes at $\sqrt{s}=10.745\,\mathrm{GeV}$Dec 6, 2023Bayesian estimation of cross-coupling and reflection systematics in 21cm array visibility dataNov 13, 2023First Measurement of $R(X_{τ/\ell})$ as an Inclusive Test of the $b \to c τν$ AnomalyOct 19, 2023Observation of the Antimatter Hypernucleus $^4_{\barΛ}\overline{\hbox{H}}$Oct 2, 2023The SOFIA FEEDBACK Legacy Survey: Rapid molecular cloud dispersal in RCW 79Aug 9, 2023Measurement of branching-fraction ratios and $CP$ asymmetries in $B^{\pm} \to D_{CP\pm}K^{\pm}$ decays at Belle and Belle IIJun 1, 2023Precise measurement of the $D^+_s$ lifetime at Belle IIMay 30, 2023Measurement of the $τ$-lepton mass with the Belle~II experimentMay 5, 2023A Race Track Trapped-Ion Quantum ProcessorMar 12, 2023Measurement of electrons from open heavy-flavor hadron decays in Au+Au collisions at $\sqrt{s_{\rm NN}}=200$ GeV with the STAR detectorJan 20, 2023Search for the decay $B^0_s \rightarrow π^0 π^0$ at BelleDec 1, 2022Hot and Cold QCD White Paper from ALICE-USA: Input for 2023 U.S. Long Range Plan for Nuclear ScienceOct 19, 2022Measurement of the photon-energy spectrum in inclusive $B\rightarrow X_{s}γ$ decays identified using hadronic decays of the recoil $B$ meson in 2019-2021 Belle II dataOct 10, 2022Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I Observations