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Study of η and η' Photoproduction at MAMI.
Kashevarov, V L; Ott, P; Prakhov, S; Adlarson, P; Afzal, F; Ahmed, Z; Akondi, C S; Annand, J R M; Arends, H J; Beck, R; Braghieri, A; Briscoe, W J; Cividini, F; Codling, R; Collicott, C; Costanza, S; Denig, A; Downie, E J; Dieterle, M; Ferretti Bondy, M I; Fil'kov, L V; Fix, A; Gardner, S; Garni, S; Glazier, D I; Glowa, D; Gradl, W; Gurevich, G; Hamilton, D J; Hornidge, D; Howdle, D; Huber, G M; Käser, A; Kay, S; Keshelashvili, I; Kondratiev, R; Korolija, M; Krusche, B; Linturi, J; Lisin, V; Livingston, K; MacGregor, I J D; MacRae, R; Mancell, J; Manley, D M; Martel, P P; McGeorge, J C; McNicol, E; Middleton, D G; Miskimen, R.
Afiliación
  • Kashevarov VL; Institut für Kernphysik, Johannes Gutenberg-Universität Mainz, D-55099 Mainz, Germany.
  • Ott P; Lebedev Physical Institute, 119991 Moscow, Russia.
  • Prakhov S; Institut für Kernphysik, Johannes Gutenberg-Universität Mainz, D-55099 Mainz, Germany.
  • Adlarson P; Institut für Kernphysik, Johannes Gutenberg-Universität Mainz, D-55099 Mainz, Germany.
  • Afzal F; The George Washington University, Washington, D.C. 20052-0001, USA.
  • Ahmed Z; University of California Los Angeles, Los Angeles, California 90095-1547, USA.
  • Akondi CS; Institut für Kernphysik, Johannes Gutenberg-Universität Mainz, D-55099 Mainz, Germany.
  • Annand JRM; Helmholtz-Institut für Strahlen- und Kernphysik, Universität Bonn, D-53115 Bonn, Germany.
  • Arends HJ; University of Regina, Regina, Saskatchewan S4S 0A2, Canada.
  • Beck R; Kent State University, Kent, Ohio 44242-0001, USA.
  • Braghieri A; SUPA School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom.
  • Briscoe WJ; Institut für Kernphysik, Johannes Gutenberg-Universität Mainz, D-55099 Mainz, Germany.
  • Cividini F; Helmholtz-Institut für Strahlen- und Kernphysik, Universität Bonn, D-53115 Bonn, Germany.
  • Codling R; INFN Sezione di Pavia, I-27100 Pavia, Italy.
  • Collicott C; The George Washington University, Washington, D.C. 20052-0001, USA.
  • Costanza S; Institut für Kernphysik, Johannes Gutenberg-Universität Mainz, D-55099 Mainz, Germany.
  • Denig A; SUPA School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom.
  • Downie EJ; Dalhousie University, Halifax, Nova Scotia B3H 4R2, Canada.
  • Dieterle M; Department of Astronomy and Physics, Saint Mary's University, Halifax, Nova Scotia B3H 3C3, Canada.
  • Ferretti Bondy MI; INFN Sezione di Pavia, I-27100 Pavia, Italy.
  • Fil'kov LV; Dipartimento di Fisica, Università di Pavia, I-27100 Pavia, Italy.
  • Fix A; Institut für Kernphysik, Johannes Gutenberg-Universität Mainz, D-55099 Mainz, Germany.
  • Gardner S; Institut für Kernphysik, Johannes Gutenberg-Universität Mainz, D-55099 Mainz, Germany.
  • Garni S; The George Washington University, Washington, D.C. 20052-0001, USA.
  • Glazier DI; Departement für Physik, Universität Basel, CH-4056 Basel, Switzerland.
  • Glowa D; Institut für Kernphysik, Johannes Gutenberg-Universität Mainz, D-55099 Mainz, Germany.
  • Gradl W; Lebedev Physical Institute, 119991 Moscow, Russia.
  • Gurevich G; Laboratory of Mathematical Physics, Tomsk Polytechnic University, 634034 Tomsk, Russia.
  • Hamilton DJ; SUPA School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom.
  • Hornidge D; Departement für Physik, Universität Basel, CH-4056 Basel, Switzerland.
  • Howdle D; SUPA School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom.
  • Huber GM; SUPA School of Physics, University of Edinburgh, Edinburgh EH9 3JZ, United Kingdom.
  • Käser A; SUPA School of Physics, University of Edinburgh, Edinburgh EH9 3JZ, United Kingdom.
  • Kay S; Institut für Kernphysik, Johannes Gutenberg-Universität Mainz, D-55099 Mainz, Germany.
  • Keshelashvili I; Institute for Nuclear Research, 125047 Moscow, Russia.
  • Kondratiev R; SUPA School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom.
  • Korolija M; Mount Allison University, Sackville, New Brunswick E4L 1E6, Canada.
  • Krusche B; SUPA School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom.
  • Linturi J; University of Regina, Regina, Saskatchewan S4S 0A2, Canada.
  • Lisin V; Departement für Physik, Universität Basel, CH-4056 Basel, Switzerland.
  • Livingston K; SUPA School of Physics, University of Edinburgh, Edinburgh EH9 3JZ, United Kingdom.
  • MacGregor IJD; Departement für Physik, Universität Basel, CH-4056 Basel, Switzerland.
  • MacRae R; Institute for Nuclear Research, 125047 Moscow, Russia.
  • Mancell J; Rudjer Boskovic Institute, HR-10000 Zagreb, Croatia.
  • Manley DM; Departement für Physik, Universität Basel, CH-4056 Basel, Switzerland.
  • Martel PP; Institut für Kernphysik, Johannes Gutenberg-Universität Mainz, D-55099 Mainz, Germany.
  • McGeorge JC; Institute for Nuclear Research, 125047 Moscow, Russia.
  • McNicol E; SUPA School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom.
  • Middleton DG; SUPA School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom.
  • Miskimen R; SUPA School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom.
Phys Rev Lett ; 118(21): 212001, 2017 May 26.
Article en En | MEDLINE | ID: mdl-28598665
The reactions γp→ηp and γp→η^{'}p are measured from their thresholds up to the center-of-mass energy W=1.96 GeV with the tagged-photon facilities at the Mainz Microtron, MAMI. Differential cross sections are obtained with unprecedented statistical accuracy, providing fine energy binning and full production-angle coverage. A strong cusp is observed in the total cross section for η photoproduction at the energies in the vicinity of the η^{'} threshold, W=1896 MeV (E_{γ}=1447 MeV). Within the framework of a revised ηMAID isobar model, the cusp, in connection with a steep rise of the η^{'} total cross section from its threshold, can only be explained by a strong coupling of the poorly known N(1895)1/2^{-} state to both ηp and η^{'}p. Including the new high-accuracy results in the ηMAID fit to available η and η^{'} photoproduction data allows the determination of the N(1895)1/2^{-} properties.

Texto completo: 1 Colección: 01-internacional Banco de datos: MEDLINE Idioma: En Revista: Phys Rev Lett Año: 2017 Tipo del documento: Article País de afiliación: Alemania

Texto completo: 1 Colección: 01-internacional Banco de datos: MEDLINE Idioma: En Revista: Phys Rev Lett Año: 2017 Tipo del documento: Article País de afiliación: Alemania