Measurement of the radiative decay width Γ[Λ(1520) --> Λγ] with the SPHINX spectrometer

dc.creatorAntipov, Yu. M.
dc.creatorArtamonov, A. V.
dc.creatorBatarin, V. A.
dc.creatorVavilov, D. V.
dc.creatorVictorov, V. A.
dc.creatorEroshin, O. V.
dc.creatorGolovkin, S. V.
dc.creatorGorin, Yu. P.
dc.creatorKolganov, V. Z.
dc.creatorKozhevnikov, A. P.
dc.creatorKonstantinov, A. S.
dc.creatorKubarovsky, V. P.
dc.creatorKurshetsov, V. F.
dc.creatorLandsberg, L. G.
dc.creatorLeontiev, V. M.
dc.creatorLomkatsi, G. S.
dc.creatorMolchanov, V. V.
dc.creatorMukhin, V. A.
dc.creatorNilov, A. F.
dc.creatorPatalakha, D. I.
dc.creatorPetrenko, S. V.
dc.creatorSmolyankin, V. T.
dc.date2004-06-15
dc.date2004-10-27
dc.date.accessioned2026-07-07T10:28:26Z
dc.date.available2026-07-07T10:28:26Z
dc.descriptionThe radiative decay Λ(1520) --> Λγwas measured directly in the study of exclusive diffractive-like reaction p + N --> Λ(1520) K^+ + N, Λ(1520) --> Λγwith the SPHINX spectrometer. The values of the branching and partial width of this radiative decay were obtained: BR[Λ(1520) --> Λγ] = (1.02+/-0.21(stat)+/-0.15(syst))x10^{-2} and Γ[Λ(1520) --> Λγ] = 159+/-33(stat)+/-26(syst) keV.
dc.descriptionMore detailed treatment of systematical uncertainties, minor clarifications and corrections, significant improvements in English. 18 pages, 6 figures, accepted by Phys.Lett.B
dc.identifierhttps://arxiv.org/abs/hep-ex/0406039
dc.identifierhttp://arxiv.org/abs/hep-ex/0406039
dc.identifierPhys.Lett.B604:22-30,2004
dc.identifierdoi:10.1016/j.physletb.2004.10.050
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/177446
dc.subjectHigh Energy Physics - Experiment
dc.titleMeasurement of the radiative decay width Γ[Λ(1520) --> Λγ] with the SPHINX spectrometer
dc.typetext

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