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000003103 0247_ $$2DOI$$a10.1103/PhysRevLett.100.052003
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000003103 037__ $$aPreJuSER-3103
000003103 041__ $$aeng
000003103 082__ $$a550
000003103 084__ $$2WoS$$aPhysics, Multidisciplinary
000003103 1001_ $$0P:(DE-Juel1)VDB73164$$aDöring, M.$$b0$$uFZJ
000003103 245__ $$aSimultaneous Photoproduction of eta and pi0 Mesons on the Proton
000003103 260__ $$aCollege Park, Md.$$bAPS$$c2008
000003103 300__ $$a052003
000003103 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article
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000003103 440_0 $$04925$$aPhysical Review Letters$$v100$$x0031-9007
000003103 500__ $$aRecord converted from VDB: 12.11.2012
000003103 520__ $$aThe analysis of the gamma p ->eta pi(0)p reaction has been performed using data from the GRAAL experiment. The total and differential cross sections and the beam asymmetry have been obtained from threshold up to 1.5 GeV of beam energy. The two resonances S-11(1535) and Delta(1700) are expected to be excited in the intermediate states of this reaction. The results are used to test predictions based on the assumption that both resonances are dynamically generated from the meson-baryon interaction provided by chiral Lagrangians. The term involving the Delta(1700) excitation, followed by the decay into eta Delta(1232), is found to be dominant.
000003103 536__ $$0G:(DE-Juel1)FUEK413$$2G:(DE-HGF)$$aPhysik der Hadronen und Kerne$$cP53$$x0
000003103 588__ $$aDataset connected to Web of Science
000003103 650_7 $$2INSPIRE$$aeffective Lagrangian: chiral
000003103 650_7 $$2INSPIRE$$aphoton p: interaction
000003103 650_7 $$2INSPIRE$$aphoton: polarized beam
000003103 650_7 $$2INSPIRE$$aeta: photoproduction
000003103 650_7 $$2INSPIRE$$api0: associated production
000003103 650_7 $$2INSPIRE$$anucleon resonance: intermediate boson
000003103 650_7 $$2INSPIRE$$aN(1535)
000003103 650_7 $$2INSPIRE$$aDelta(1700)
000003103 650_7 $$2INSPIRE$$across section
000003103 650_7 $$2INSPIRE$$apolarization: asymmetry
000003103 650_7 $$2INSPIRE$$aenergy dependence
000003103 650_7 $$2INSPIRE$$anumerical calculations
000003103 650_7 $$2INSPIRE$$ainterpretation of experiments: Grenoble ESRF
000003103 650_7 $$2INSPIRE$$aphoton p --> p eta pi0
000003103 650_7 $$2INSPIRE$$a< 1.5 GeV: (1))
000003103 7001_ $$0P:(DE-HGF)0$$aAjaka, J.$$b1
000003103 7001_ $$0P:(DE-HGF)0$$aAssafiri, Y.$$b2
000003103 7001_ $$0P:(DE-HGF)0$$aBartalini, O.$$b3
000003103 7001_ $$0P:(DE-HGF)0$$aBellini, V.$$b4
000003103 7001_ $$0P:(DE-HGF)0$$aBouchigny, S.$$b5
000003103 7001_ $$0P:(DE-HGF)0$$aCastoldi, M.$$b6
000003103 7001_ $$0P:(DE-HGF)0$$aD`Angelo, A.$$b7
000003103 7001_ $$0P:(DE-HGF)0$$aDidelez, J. P.$$b8
000003103 7001_ $$0P:(DE-HGF)0$$aDi Salvo, R.$$b9
000003103 7001_ $$0P:(DE-HGF)0$$aFantini, A.$$b10
000003103 7001_ $$0P:(DE-HGF)0$$aFichen, L.$$b11
000003103 7001_ $$0P:(DE-HGF)0$$aGervino, G.$$b12
000003103 7001_ $$0P:(DE-HGF)0$$aGhio, F.$$b13
000003103 7001_ $$0P:(DE-HGF)0$$aGirolami, B.$$b14
000003103 7001_ $$0P:(DE-HGF)0$$aGiusa, A.$$b15
000003103 7001_ $$0P:(DE-HGF)0$$aGuidal, M.$$b16
000003103 7001_ $$0P:(DE-HGF)0$$aHourany, E.$$b17
000003103 7001_ $$0P:(DE-HGF)0$$aKunne, R.$$b18
000003103 7001_ $$0P:(DE-HGF)0$$aLapik, A.$$b19
000003103 7001_ $$0P:(DE-HGF)0$$aSandri, P. L.$$b20
000003103 7001_ $$0P:(DE-HGF)0$$aMoricciani, D.$$b21
000003103 7001_ $$0P:(DE-HGF)0$$aMuskarenkov, A.$$b22
000003103 7001_ $$0P:(DE-HGF)0$$aNedorezov, V.$$b23
000003103 7001_ $$0P:(DE-HGF)0$$aOset, E.$$b24
000003103 7001_ $$0P:(DE-HGF)0$$aRandieri, C.$$b25
000003103 7001_ $$0P:(DE-HGF)0$$aRudnev, N.$$b26
000003103 7001_ $$0P:(DE-HGF)0$$aRusso, G.$$b27
000003103 7001_ $$0P:(DE-HGF)0$$aSchaerf, C.$$b28
000003103 7001_ $$0P:(DE-HGF)0$$aSperduto, M.$$b29
000003103 7001_ $$0P:(DE-HGF)0$$aSutera, M.$$b30
000003103 7001_ $$0P:(DE-HGF)0$$aTuringe, A.$$b31
000003103 773__ $$0PERI:(DE-600)1472655-5$$a10.1103/PhysRevLett.100.052003$$gVol. 100, p. 052003$$p052003$$q100<052003$$tPhysical review letters$$v100$$x0031-9007$$y2008
000003103 8567_ $$uhttp://dx.doi.org/10.1103/PhysRevLett.100.052003
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