Abstract
An upper limit (K0*(1430)K0)<84 keV (90% C.L.) has been derived from a search for Primakoff production of the K0*(1430) in the energy range 60200 GeV. The radiative width depends upon the values of the strange- and down-quark magnetic moments and is much smaller than the related radiative width of the K+*(1430). A naive quark-model calculation is presented which K+*(1430). A naive quark-model calculation is presented which explains this result.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 3502-3505 |
| Number of pages | 4 |
| Journal | Physical Review D |
| Volume | 36 |
| Issue number | 11 |
| DOIs | |
| State | Published - 1987 |
| Externally published | Yes |
ASJC Scopus subject areas
- Physics and Astronomy (miscellaneous)
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