Showing 261–280 of 1,256 results
/ Date/ Name
Mar 4, 2022A Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino PhysicsFeb 28, 2022Experimental study of the $^{40,48}$Ca+ $^{40,48}$Ca reactions at 35 MeV/nucleonFeb 22, 2022Implications of the first evidence for coherent elastic scattering of reactor neutrinosFeb 17, 2022Final results on the $0νββ$ decay half-life limit of $^{100}$Mo from the CUPID-Mo experimentFeb 13, 2022Angular distribution of $γ$ rays from the p-wave resonance of $^{118}$SnFeb 11, 2022Multi-channel experimental and theoretical constraints for the $^{116}$Cd($^{20}$Ne,$^{20}$F)$^{116}$In charge exchange reaction at 306 MeVFeb 11, 2022Border of the Island of Inversion: Unbound states in $^{29}$NeFeb 7, 2022A First Glimpse at the Shell Structure beyond $^{54}$Ca: Spectroscopy of $^{55}$K, $^{55}$Ca, and $^{57}$CaJan 25, 2022Activation cross section measurement of the 14N(p,gamma)15O astrophysical key reactionJan 12, 2022Development of a $^{127}$Xe calibration source for nEXODec 31, 2021First Determination of the 27Al Neutron Distribution Radius from a Parity-Violating Electron Scattering MeasurementDec 10, 2021First application of mass measurement with the Rare-RI Ring reveals the solar r-process abundance trend at A=122 and A=123Dec 6, 2021Nuclear Charge Radii of the Nickel Isotopes $^{58-68,70}$NiDec 1, 2021Measurements of Proton High Order Cumulants in 3 GeV Au+Au Collisions and Implications for the QCD Critical PointNov 29, 2021Evidence of Mass Ordering of Charm and Bottom Quark Energy Loss in Au+Au Collisions at RHICNov 25, 2021Accessing ground state and excited states energies in many-body system after symmetry restoration using quantum computersNov 19, 2021Charge radii, moments and masses of mercury isotopes across the N = 126 shell closureNov 15, 2021Enhanced production of $^{8}$Be nuclei in relativistic nuclei fragmentationNov 8, 2021New Measurements of the Beam-Normal Single Spin Asymmetry in Elastic Electron Scattering Over a Range of Spin-0 NucleiOct 27, 2021Improved Nuclear Physics Near $A=61$ Refines Urca Neutrino Luminosities in Accreted Neutron Star Crusts