The SciBooNE Collaboration has performed a search for charged current coherent pion production from muon neutrinos scattering on carbon, nu C-12(mu) -> mu C-12 pi+(,) with two distinct data samples. No evidence for coherent pion production is observed. We set 90% confidence level upper limits on the cross section ratio of charged current coherent pion production to the total charged current cross section at 0.67 X 10(-2) at mean neutrino energy 1.1 GeV and 1.36 X 10(-2) at mean neutrino energy 2.2 GeV.

Search for charged current coherent pion production on carbon in a few-GeV neutrino beam / K., H., J. L., A.A., S. J., B., L., B., J., C.P., G., C., J. M., C., Z., D., Dore, U., D. A., F., A. J., F., C., G., J. J., G.C., P., G., A., H., Y., H., G., J.M., G., K., T., K., Y. K., K., et al.. - In: PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. - ISSN 1550-7998. - 78:11(2008). [10.1103/physrevd.78.112004]

Search for charged current coherent pion production on carbon in a few-GeV neutrino beam

DORE, Ubaldo;LOVERRE, Pier Ferruccio;
2008

Abstract

The SciBooNE Collaboration has performed a search for charged current coherent pion production from muon neutrinos scattering on carbon, nu C-12(mu) -> mu C-12 pi+(,) with two distinct data samples. No evidence for coherent pion production is observed. We set 90% confidence level upper limits on the cross section ratio of charged current coherent pion production to the total charged current cross section at 0.67 X 10(-2) at mean neutrino energy 1.1 GeV and 1.36 X 10(-2) at mean neutrino energy 2.2 GeV.
2008
01 Pubblicazione su rivista::01a Articolo in rivista
Search for charged current coherent pion production on carbon in a few-GeV neutrino beam / K., H., J. L., A.A., S. J., B., L., B., J., C.P., G., C., J. M., C., Z., D., Dore, U., D. A., F., A. J., F., C., G., J. J., G.C., P., G., A., H., Y., H., G., J.M., G., K., T., K., Y. K., K., et al.. - In: PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. - ISSN 1550-7998. - 78:11(2008). [10.1103/physrevd.78.112004]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/90238
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