Inclusive [Formula Presented] production from the [Formula Presented]

M. Artuso; C. Boulahouache; S. Blusk; K. Bukin; E. Dambasuren; R. Mountain; H. Muramatsu; R. Nandakumar; T. Skwarnicki; S. Stone; J. C. Wang; B. Gittelman; S. W. Gray; D. L. Hartill; B. K. Heltsley; L. Hsu; C. D. Jones; J. Kandaswamy; D. L. Kreinick; A. Magerkurth; H. Mahlke-Krüger; T. O. Meyer; N. B. Mistry; J. R. Patterson; D. Peterson; J. Pivarski; S. J. Richichi; D. Riley; A. J. Sadoff; H. Schwarthoff; M. R. Shepherd; J. G. Thayer; D. Urner; T. Wilksen; A. Warburton; M. Weinberger

doi:10.1103/PhysRevD.67.052003

Inclusive [Formula Presented] production from the [Formula Presented]

M. Artuso, C. Boulahouache, S. Blusk, K. Bukin, E. Dambasuren, R. Mountain, H. Muramatsu, R. Nandakumar, T. Skwarnicki, S. Stone, J. C. Wang, B. Gittelman, S. W. Gray, D. L. Hartill, B. K. Heltsley, L. Hsu, C. D. Jones, J. Kandaswamy, D. L. Kreinick, A. MagerkurthH. Mahlke-Krüger, T. O. Meyer, N. B. Mistry, J. R. Patterson, D. Peterson, J. Pivarski, S. J. Richichi, D. Riley, A. J. Sadoff, H. Schwarthoff, M. R. Shepherd, J. G. Thayer, D. Urner, T. Wilksen, A. Warburton, M. Weinberger

Department of Physics

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

Abstract

Using the CLEO II detector at CESR, we measure the (Formula presented) energy spectra in (Formula presented) decays that we compare with models of the (Formula presented) form factor. This form factor, especially at large (Formula presented) energies, may provide an explanation of the large rate for (Formula presented) Our data do not support a large anomalous coupling at higher (Formula presented) and thus the large (Formula presented) rate remains a mystery, possibly requiring a non-standard-model explanation.

Original language	English (US)
Journal	Physical Review D - Particles, Fields, Gravitation and Cosmology
Volume	67
Issue number	5
DOIs	https://doi.org/10.1103/PhysRevD.67.052003
State	Published - 2003

ASJC Scopus subject areas

Nuclear and High Energy Physics
Physics and Astronomy (miscellaneous)

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10.1103/PhysRevD.67.052003

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Artuso, M., Boulahouache, C., Blusk, S., Bukin, K., Dambasuren, E., Mountain, R., Muramatsu, H., Nandakumar, R., Skwarnicki, T., Stone, S., Wang, J. C., Gittelman, B., Gray, S. W., Hartill, D. L., Heltsley, B. K., Hsu, L., Jones, C. D., Kandaswamy, J., Kreinick, D. L., ... Weinberger, M. (2003). Inclusive [Formula Presented] production from the [Formula Presented]. Physical Review D - Particles, Fields, Gravitation and Cosmology, 67(5). https://doi.org/10.1103/PhysRevD.67.052003

Artuso, M, Boulahouache, C, Blusk, S, Bukin, K, Dambasuren, E, Mountain, R, Muramatsu, H, Nandakumar, R, Skwarnicki, T, Stone, S, Wang, JC, Gittelman, B, Gray, SW, Hartill, DL, Heltsley, BK, Hsu, L, Jones, CD, Kandaswamy, J, Kreinick, DL, Magerkurth, A, Mahlke-Krüger, H, Meyer, TO, Mistry, NB, Patterson, JR, Peterson, D, Pivarski, J, Richichi, SJ, Riley, D, Sadoff, AJ, Schwarthoff, H, Shepherd, MR, Thayer, JG, Urner, D, Wilksen, T, Warburton, A & Weinberger, M 2003, 'Inclusive [Formula Presented] production from the [Formula Presented]', Physical Review D - Particles, Fields, Gravitation and Cosmology, vol. 67, no. 5. https://doi.org/10.1103/PhysRevD.67.052003

@article{8a30fcc012a14456b6d4793badfe51b4,

title = "Inclusive [Formula Presented] production from the [Formula Presented]",

abstract = "Using the CLEO II detector at CESR, we measure the (Formula presented) energy spectra in (Formula presented) decays that we compare with models of the (Formula presented) form factor. This form factor, especially at large (Formula presented) energies, may provide an explanation of the large rate for (Formula presented) Our data do not support a large anomalous coupling at higher (Formula presented) and thus the large (Formula presented) rate remains a mystery, possibly requiring a non-standard-model explanation.",

author = "M. Artuso and C. Boulahouache and S. Blusk and K. Bukin and E. Dambasuren and R. Mountain and H. Muramatsu and R. Nandakumar and T. Skwarnicki and S. Stone and Wang, {J. C.} and B. Gittelman and Gray, {S. W.} and Hartill, {D. L.} and Heltsley, {B. K.} and L. Hsu and Jones, {C. D.} and J. Kandaswamy and Kreinick, {D. L.} and A. Magerkurth and H. Mahlke-Kr{\"u}ger and Meyer, {T. O.} and Mistry, {N. B.} and Patterson, {J. R.} and D. Peterson and J. Pivarski and Richichi, {S. J.} and D. Riley and Sadoff, {A. J.} and H. Schwarthoff and Shepherd, {M. R.} and Thayer, {J. G.} and D. Urner and T. Wilksen and A. Warburton and M. Weinberger",

year = "2003",

doi = "10.1103/PhysRevD.67.052003",

language = "English (US)",

volume = "67",

journal = "Physical Review D - Particles, Fields, Gravitation and Cosmology",

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T1 - Inclusive [Formula Presented] production from the [Formula Presented]

AU - Artuso, M.

AU - Boulahouache, C.

AU - Blusk, S.

AU - Bukin, K.

AU - Dambasuren, E.

AU - Mountain, R.

AU - Muramatsu, H.

AU - Nandakumar, R.

AU - Skwarnicki, T.

AU - Stone, S.

AU - Wang, J. C.

AU - Gittelman, B.

AU - Gray, S. W.

AU - Hartill, D. L.

AU - Heltsley, B. K.

AU - Hsu, L.

AU - Jones, C. D.

AU - Kandaswamy, J.

AU - Kreinick, D. L.

AU - Magerkurth, A.

AU - Mahlke-Krüger, H.

AU - Meyer, T. O.

AU - Mistry, N. B.

AU - Patterson, J. R.

AU - Peterson, D.

AU - Pivarski, J.

AU - Richichi, S. J.

AU - Riley, D.

AU - Sadoff, A. J.

AU - Schwarthoff, H.

AU - Shepherd, M. R.

AU - Thayer, J. G.

AU - Urner, D.

AU - Wilksen, T.

AU - Warburton, A.

AU - Weinberger, M.

PY - 2003

Y1 - 2003

N2 - Using the CLEO II detector at CESR, we measure the (Formula presented) energy spectra in (Formula presented) decays that we compare with models of the (Formula presented) form factor. This form factor, especially at large (Formula presented) energies, may provide an explanation of the large rate for (Formula presented) Our data do not support a large anomalous coupling at higher (Formula presented) and thus the large (Formula presented) rate remains a mystery, possibly requiring a non-standard-model explanation.

AB - Using the CLEO II detector at CESR, we measure the (Formula presented) energy spectra in (Formula presented) decays that we compare with models of the (Formula presented) form factor. This form factor, especially at large (Formula presented) energies, may provide an explanation of the large rate for (Formula presented) Our data do not support a large anomalous coupling at higher (Formula presented) and thus the large (Formula presented) rate remains a mystery, possibly requiring a non-standard-model explanation.

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JO - Physical Review D - Particles, Fields, Gravitation and Cosmology

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ER -

Inclusive [Formula Presented] production from the [Formula Presented]

Abstract

ASJC Scopus subject areas

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