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. 2017 May 26;118(21):212001.
doi: 10.1103/PhysRevLett.118.212001. Epub 2017 May 26.

Study of η and η' Photoproduction at MAMI

V L Kashevarov  1   2 P Ott  1 S Prakhov  1   3   4 P Adlarson  1 F Afzal  5 Z Ahmed  6 C S Akondi  7 J R M Annand  8 H J Arends  1 R Beck  5 A Braghieri  9 W J Briscoe  3 F Cividini  1 R Codling  8 C Collicott  10   11 S Costanza  9   12 A Denig  1 E J Downie  1   3 M Dieterle  13 M I Ferretti Bondy  1 L V Fil'kov  2 A Fix  14 S Gardner  8 S Garni  13 D I Glazier  8   15 D Glowa  15 W Gradl  1 G Gurevich  16 D J Hamilton  8 D Hornidge  17 D Howdle  8 G M Huber  6 A Käser  13 S Kay  15 I Keshelashvili  13 R Kondratiev  16 M Korolija  18 B Krusche  13 J Linturi  1 V Lisin  16 K Livingston  8 I J D MacGregor  8 R MacRae  8 J Mancell  8 D M Manley  7 P P Martel  1   17 J C McGeorge  8 E McNicol  8 D G Middleton  1   17 R Miskimen  19 E Mornacchi  1 C Mullen  8 A Mushkarenkov  9   19 A Neiser  1 M Oberle  13 M Ostrick  1 P B Otte  1 B Oussena  1   3 D Paudyal  6 P Pedroni  9 V V Polyanski  2 A Rajabi  19 G Reicherz  20 J Robinson  8 G Rosner  8 T Rostomyan  13 A Sarty  11 D M Schott  3 S Schumann  1 C Sfienti  1 V Sokhoyan  1   3 K Spieker  5 O Steffen  1 B Strandberg  8 I I Strakovsky  3 Th Strub  13 I Supek  18 M F Taragin  3 A Thiel  5 M Thiel  1 L Tiator  1 A Thomas  1 M Unverzagt  1 S Wagner  1 D P Watts  15 D Werthmüller  8   13 J Wettig  1 L Witthauer  13 M Wolfes  1 R L Workman  3 L Zana  15 A2 Collaboration at MAMI
Affiliations

Study of η and η' Photoproduction at MAMI

V L Kashevarov et al. Phys Rev Lett. .

Abstract

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.

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