Showing 221–240 of 945 results
/ Date/ Name
Aug 18, 2021An Improved Measurement of Neutrino Oscillation Parameters by the NOvA ExperimentAug 2, 2021Probing Strangeness Canonical Ensemble with $K^{-}$, $φ(1020)$ and $Ξ^{-}$ Production in Au+Au Collisions at ${\sqrt{s_{\rm NN}} = \rm{3\,GeV}}$Aug 2, 2021Disappearance of partonic collectivity in $\sqrt{s_{NN}}$ = 3 GeV Au+Au collisions at RHICJul 30, 2021Global $Λ$-hyperon polarization in Au+Au collisions at $\sqrt{s_\mathrm{NN}}=3$ GeVJul 30, 2021Magnetohydrodynamics and electro-electron interaction of massless Dirac fermionsJul 30, 2021Constraining the 21cm brightness temperature of the IGM at $z$=6.6 around LAEs with the Murchison Widefield ArrayJul 29, 2021All-sky search for long-duration gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo runJul 23, 2021LEGEND-1000 Preconceptual Design ReportJul 19, 2021Searching for solar KDAR with DUNEJul 12, 2021The Impact of Mixing Treatments on Cloud Modelling in 3D Simulations of Hot JupitersJul 6, 2021Measurement of the $^{239}$Pu(n,f)/$^{235}$U(n,f) Cross-Section Ratio with the NIFFTE fission Time Projection ChamberJun 25, 2021Rediscovery of $B^0\to J\mskip 1mu / ψ\mskip 2mu K^0_{\scriptscriptstyle L}$ at Belle IIJun 23, 2021Fermi Large Area Telescope Performance After 10 Years Of OperationJun 10, 2021Performance of the MICE diagnostic systemJun 10, 2021Investigation of the correlation patterns and the Compton dominance variability of Mrk 421 in 2017Jun 7, 2021Measurements of branching fractions and direct CP asymmetries in $B^{0}\to K^{+} π^{-}$, $B^+ \to K_{\rm S}^0π^+$ and $B^0 \to π^+π^-$ using 2019 and 2020 dataJun 1, 2021Search for dark matter annihilation signals from unidentified Fermi-LAT objects with H.E.S.SJun 1, 2021Measurement of the time-integrated mixing probability $χ_d$ with a semileptonic double-tagging strategy and $34.6 {\rm fb}^{-1}$ of Belle II collision dataMay 27, 2021Constraints on dark photon dark matter using data from LIGO's and Virgo's third observing runMay 27, 2021A new MWA limit on the 21 cm Power Spectrum at Redshifts $\sim$ 13 $-$ 17