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D. Besson

Publications and source records attributed to D. Besson.

92 records · Page 6Linked to original sources

Observation of a Narrow Resonance of Mass 2.46 GeV/c^2 in the D_s^*+π^0 Final State, and Confirmation of the D_sJ^*(2317)

Using 13.5 fb^{-1} of e^+e^- annihilation data collected with the CLEO-II detector, we have observed a new narrow resonance in the D_s^*π^0 final state, with a mass near 2.46 GeV/c^2. The search for such a state was motivated by the recent discovery by the BaBar Collaboration of a narrow state at 2.32 GeV/c^2, the D_{sJ}^*(2317)^+, that decays to D_sπ^0. Reconstructing the D_sπ^0 and D_s^*π^0 final states in CLEO data, we observe a peak in each of the corresponding reconstructed mass difference distributions, ΔM_{D_sπ^0} = M(D_sπ^0) - M(D_s) and ΔM_{D_s^*π^0} = M(D_s^*π^0) - M(D_s^*), both of them at values around 350 MeV/c^2. These peaks constitute statistically significant evidence for two distinct states, at 2.32 and 2.46 GeV/c^2, taking into account the background source that each state comprises for the other in light of the nearly identical values of ΔM observed for the two peaks. We have measured the mean mass differences ΔM_{D_sπ^0} = 350.4 \pm 1.2[stat.] \pm 1.0 [syst.] MeV/c^2 for the $D_{sJ}^*(2317)^+$ state, and ΔM_{D_s^*π^0} = 351.6 \pm 1.7[stat.] \pm 1.0 [syst.] MeV/c^2 for the new state at 2.46 GeV/c^2. We have also searched, but find no evidence, for decays of D_{sJ}^*(2317) into the alternate final states D_s^*γ, D_sγ, and D_sπ^+π^-. The observations of the two states at 2.32 and 2.46 GeV/c^2, in the D_sπ^0 and D_s^*π^0 decay channels respectively, are consistent with their possible interpretations as c s-bar mesons with orbital angular momentum L=1, and spin-parity J^P = 0^+ and 1^+.

hep-ex

Status of Radio Ice Cherenkov Experiment (RICE)

RICE is designed to detect ultrahigh energy (>100 TeV) neutrinos from astrophysical sources. It will consist of an array of compact radio (100 to 1000 MHz) receivers buried in ice at the South Pole. During the 1995-96 and 1996-97 austral summers, several receivers transmitters were deployed in bore holes drilled for the AMANDA project, at depths of 141 to 260 m. This was the first in situ test of radio receivers in deep ice for neutrino astronomy.

astro-ph