Limit on the radiative width of the K0/emph>(1430)

D. Carlsmith; R. H. Bernstein; G. Bock; D. Coupal; G. D. Gollin; K. Nishikawa; H. Norton; B. Winstein; B. Peyaud; R. Turlay; A. Zylberstejn

doi:10.1103/PhysRevD.36.3502

Limit on the radiative width of the K0/emph>(1430)

D. Carlsmith, R. H. Bernstein, G. Bock, D. Coupal, G. D. Gollin, K. Nishikawa, H. Norton, B. Winstein, B. Peyaud, R. Turlay, A. Zylberstejn

Research output: Contribution to journal › Article › peer-review

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	https://doi.org/10.1103/PhysRevD.36.3502
State	Published - 1987
Externally published	Yes

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Physics and Astronomy (miscellaneous)

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10.1103/PhysRevD.36.3502

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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.",

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doi = "10.1103/PhysRevD.36.3502",

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T1 - Limit on the radiative width of the K0/emph>(1430)

AU - Carlsmith, D.

AU - Bernstein, R. H.

AU - Bock, G.

AU - Coupal, D.

AU - Gollin, G. D.

AU - Nishikawa, K.

AU - Norton, H.

AU - Winstein, B.

AU - Peyaud, B.

AU - Turlay, R.

AU - Zylberstejn, A.

PY - 1987

Y1 - 1987

N2 - 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.

AB - 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.

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ER -

Limit on the radiative width of the K0/emph>(1430)

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