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Observation of the radiative transition ψ → γE(1420)
- Scharre, DL;
- Trilling, GH;
- Abrams, GS;
- Alam, MS;
- Blocker, CA;
- Blondel, A;
- Boyarski, AM;
- Breidenbach, M;
- Burke, DL;
- Carithers, WC;
- Chinowsky, W;
- Coles, MW;
- Cooper, S;
- Dieterle, WE;
- Dillon, JB;
- Dorenbosch, J;
- Dorfan, JM;
- Eaton, MW;
- Feldman, GJ;
- Franklin, MEB;
- Gidal, G;
- Goldhaber, G;
- Hanson, G;
- Hayes, KG;
- Himel, T;
- Hitlin, DG;
- Hollebeek, RJ;
- Innes, WR;
- Jaros, JA;
- Jenni, P;
- Johnson, AD;
- Kadyk, JA;
- Lankford, AJ;
- Larsen, RR;
- Lüth, V;
- Millikan, RE;
- Nelson, ME;
- Pang, CY;
- Patrick, JF;
- Perl, ML;
- Richter, B;
- Roussarie, A;
- Schindler, RH;
- Schwitters, RF;
- Siegrist, JL;
- Strait, J;
- Taureg, H;
- Tonutti, M;
- Vella, EN;
- Vidal, RA;
- Videau, I;
- Weiss, JM;
- Zaccone, H
Published Web Location
https://doi.org/10.1016/0370-2693(80)90612-7Abstract
We have observed a radiative transition from the ψ to a state decaying into KSK±π∓, with mass M = 1.44-0.015+0.01 GeV/c2 and width Γ = 0.05-0.02+0.03 GeV/c2. We tentatively identify this state as the E(1420). Assuming that this state is an isospin singlet, we have determined the branching fraction product B(ψ → γE) × B(E × KKπ) = (3.6 ± 1.4) × 10-3. © 1980.
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