Radiative decay of the K*-(890)

D. Berg; C. Chandlee; S. Cihangir; T. Ferbel; J. Huston; T. Jensen; F. Lobkowicz; C. A. Nelson; T. Oshima; P. Slattery; P. Thompson; J. Biel; T. Droege; A. Jonckheere; P. F. Koehler; S. Heppelmann; T. Joyce; Y. Makdisi; M. Marshak; E. Peterson; K. Ruddick; T. Walsh

doi:10.1016/0370-2693(81)90380-4

Radiative decay of the K^*-(890)

D. Berg
, C. Chandlee
, S. Cihangir
, T. Ferbel
, J. Huston
, T. Jensen
, F. Lobkowicz
, C. A. Nelson
, T. Oshima
, P. Slattery
, P. Thompson
, J. Biel
, T. Droege
, A. Jonckheere
, P. F. Koehler
, S. Heppelmann
, T. Joyce
, Y. Makdisi
, M. Marshak
, E. Peterson

K. Ruddick, T. Walsh

Physics and Astronomy (Twin Cities)

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

13 Scopus citations

Abstract

We report a measurement of the radiative decay of the K^*- (890). The width for the transition K^*- → K^- γ is 62 ± 14 keV. The resulting ratio of decay probabilities (K^*0 → K⁰γ)/(K^*- → K^-γ), while consistent with predictions of certain quark models, does not agree with expectations from unbroken SU(3) symmetry.

Original language	English (US)
Pages (from-to)	119-122
Number of pages	4
Journal	Physics Letters B
Volume	98
Issue number	1-2
DOIs	https://doi.org/10.1016/0370-2693(81)90380-4
State	Published - Jan 1 1981

Bibliographical note

Funding Information:
Radiative decay transitions between meson states provide some of the most straight-forward tests of SU(3) and of the quark model. Predictions for K *f (890) ~ K-+7, p ~ rt7 and K*0(890) ~ K07 decays are independent of assumptions concerning mixing between the singlet and octet members of the vector and pseudoscalar meson nonets. In addition, the small mass differences between K *0 and K*-+, and between K 0 and K +-, make the ratio of the radiative widths P(K* 0 -~ K07)/F(K * ~ -~ K~7) essentially independent of any phase-space factors. In the simple quark model, this ratio can be expressed, using quark magnetic moments/~q, as Research supported by the US Department of Energy, The National Science Foundation and by funds from the Uni-versities of Minnesota and Rochester.

Publisher link

10.1016/0370-2693(81)90380-4

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Berg, D., Chandlee, C., Cihangir, S., Ferbel, T., Huston, J., Jensen, T., Lobkowicz, F., Nelson, C. A., Oshima, T., Slattery, P., Thompson, P., Biel, J., Droege, T., Jonckheere, A., Koehler, P. F., Heppelmann, S., Joyce, T., Makdisi, Y., Marshak, M., ... Walsh, T. (1981). Radiative decay of the K^*-(890). Physics Letters B, 98(1-2), 119-122. https://doi.org/10.1016/0370-2693(81)90380-4

Berg, D, Chandlee, C, Cihangir, S, Ferbel, T, Huston, J, Jensen, T, Lobkowicz, F, Nelson, CA, Oshima, T, Slattery, P, Thompson, P, Biel, J, Droege, T, Jonckheere, A, Koehler, PF, Heppelmann, S, Joyce, T, Makdisi, Y, Marshak, M, Peterson, E, Ruddick, K & Walsh, T 1981, 'Radiative decay of the K^*-(890)', Physics Letters B, vol. 98, no. 1-2, pp. 119-122. https://doi.org/10.1016/0370-2693(81)90380-4

@article{610abe184d28471cb5e7c77ed3a765ea,

title = "Radiative decay of the K*-(890)",

abstract = "We report a measurement of the radiative decay of the K*- (890). The width for the transition K*- → K- γ is 62 ± 14 keV. The resulting ratio of decay probabilities (K*0 → K0γ)/(K*- → K-γ), while consistent with predictions of certain quark models, does not agree with expectations from unbroken SU(3) symmetry.",

author = "D. Berg and C. Chandlee and S. Cihangir and T. Ferbel and J. Huston and T. Jensen and F. Lobkowicz and Nelson, \{C. A.\} and T. Oshima and P. Slattery and P. Thompson and J. Biel and T. Droege and A. Jonckheere and Koehler, \{P. F.\} and S. Heppelmann and T. Joyce and Y. Makdisi and M. Marshak and E. Peterson and K. Ruddick and T. Walsh",

note = "Funding Information: Radiative decay transitions between meson states provide some of the most straight-forward tests of SU(3) and of the quark model. Predictions for K *f (890) \textasciitilde{} K-+7, p \textasciitilde{} rt7 and K*0(890) \textasciitilde{} K07 decays are independent of assumptions concerning mixing between the singlet and octet members of the vector and pseudoscalar meson nonets. In addition, the small mass differences between K *0 and K*-+, and between K 0 and K +-, make the ratio of the radiative widths P(K* 0 -\textasciitilde{} K07)/F(K * \textasciitilde{} -\textasciitilde{} K\textasciitilde{}7) essentially independent of any phase-space factors. In the simple quark model, this ratio can be expressed, using quark magnetic moments/\textasciitilde{}q, as Research supported by the US Department of Energy, The National Science Foundation and by funds from the Uni-versities of Minnesota and Rochester.",

year = "1981",

month = jan,

day = "1",

doi = "10.1016/0370-2693(81)90380-4",

language = "English (US)",

volume = "98",

pages = "119--122",

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TY - JOUR

T1 - Radiative decay of the K*-(890)

AU - Berg, D.

AU - Chandlee, C.

AU - Cihangir, S.

AU - Ferbel, T.

AU - Huston, J.

AU - Jensen, T.

AU - Lobkowicz, F.

AU - Nelson, C. A.

AU - Oshima, T.

AU - Slattery, P.

AU - Thompson, P.

AU - Biel, J.

AU - Droege, T.

AU - Jonckheere, A.

AU - Koehler, P. F.

AU - Heppelmann, S.

AU - Joyce, T.

AU - Makdisi, Y.

AU - Marshak, M.

AU - Peterson, E.

AU - Ruddick, K.

AU - Walsh, T.

N1 - Funding Information: Radiative decay transitions between meson states provide some of the most straight-forward tests of SU(3) and of the quark model. Predictions for K *f (890) ~ K-+7, p ~ rt7 and K*0(890) ~ K07 decays are independent of assumptions concerning mixing between the singlet and octet members of the vector and pseudoscalar meson nonets. In addition, the small mass differences between K *0 and K*-+, and between K 0 and K +-, make the ratio of the radiative widths P(K* 0 -~ K07)/F(K * ~ -~ K~7) essentially independent of any phase-space factors. In the simple quark model, this ratio can be expressed, using quark magnetic moments/~q, as Research supported by the US Department of Energy, The National Science Foundation and by funds from the Uni-versities of Minnesota and Rochester.

PY - 1981/1/1

Y1 - 1981/1/1

N2 - We report a measurement of the radiative decay of the K*- (890). The width for the transition K*- → K- γ is 62 ± 14 keV. The resulting ratio of decay probabilities (K*0 → K0γ)/(K*- → K-γ), while consistent with predictions of certain quark models, does not agree with expectations from unbroken SU(3) symmetry.

AB - We report a measurement of the radiative decay of the K*- (890). The width for the transition K*- → K- γ is 62 ± 14 keV. The resulting ratio of decay probabilities (K*0 → K0γ)/(K*- → K-γ), while consistent with predictions of certain quark models, does not agree with expectations from unbroken SU(3) symmetry.

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U2 - 10.1016/0370-2693(81)90380-4

DO - 10.1016/0370-2693(81)90380-4

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AN - SCOPUS:0002157898

SN - 0370-2693

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SP - 119

EP - 122

JO - Physics Letters B

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