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000052234 0247_ $$2DOI$$a10.1103/PhysRevLett.96.242301
000052234 0247_ $$2WOS$$aWOS:000238487900013
000052234 0247_ $$2arXiv$$aarXiv:hep-ex/0604010$$chep-ex
000052234 0247_ $$2arXiv$$aarXiv:oai:arXiv.org:hep-ex/0604010
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000052234 035__ $$9arXiv$$ahep-ex/0604010$$chep-ex
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000052234 035__ $$9DESY$$zD06-09033
000052234 035__ $$9SPIRESTeX$$zHartmann:2006zc
000052234 041__ $$aeng
000052234 082__ $$a550
000052234 084__ $$2WoS$$aPhysics, Multidisciplinary
000052234 084__ $$2PACS$$a25.40.Ve
000052234 084__ $$2PACS$$a13.75.Cs
000052234 084__ $$2PACS$$a25.10.+s
000052234 084__ $$2PACS$$a99.10.Fg
000052234 1001_ $$0P:(DE-Juel1)131183$$aHartmann, M.$$b0$$uFZJ
000052234 245__ $$aNear-Threshold Production Phi Mesons in pp Collisions
000052234 260__ $$aCollege Park, Md.$$bAPS$$c2006
000052234 300__ $$a242301
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000052234 440_0 $$04925$$aPhysical Review Letters$$v96$$x0031-9007
000052234 500__ $$aRecord converted from VDB: 12.11.2012
000052234 500__ $$9arXiv$$a4 Pages, 3 Figures, 1 Table, submitted to Phys. Rev. Lett
000052234 520__ $$aThe pp -> pp phi reaction has been studied at the Cooler Synchrotron COSY-Julich, using the internal beam and ANKE facility. Total cross sections have been determined at three excess energies epsilon near the production threshold. The differential cross section closest to threshold at epsilon=18.5 MeV exhibits a clear S wave dominance as well as a noticeable effect due to the proton-proton final-state interaction. Taken together with data for pp omega production, a significant enhancement of the phi/omega ratio of a factor 8 is found compared to predictions based on the Okubo-Zweig-Iizuka rule.
000052234 536__ $$0G:(DE-Juel1)FUEK413$$2G:(DE-HGF)$$aPhysik der Hadronen und Kerne$$cP53$$x0
000052234 588__ $$aDataset connected to Web of Science
000052234 650_7 $$2INSPIRE$$ap p: inelastic scattering
000052234 650_7 $$2INSPIRE$$aPhi(1020): hadroproduction
000052234 650_7 $$2INSPIRE$$athreshold
000052234 650_7 $$2INSPIRE$$amass spectrum: (K+ K-)
000052234 650_7 $$2INSPIRE$$achannel cross section: energy dependence
000052234 650_7 $$2INSPIRE$$adifferential cross section: momentum dependence
000052234 650_7 $$2INSPIRE$$aangular distribution
000052234 650_7 $$2INSPIRE$$aamplitude analysis: partial wave
000052234 650_7 $$2INSPIRE$$ap p: final-state interaction
000052234 650_7 $$2INSPIRE$$ayield: (Phi(1020) omega(783))
000052234 650_7 $$2INSPIRE$$aIizuka-Okubo-Zweig rule
000052234 650_7 $$2INSPIRE$$amagnetic spectrometer: experimental results
000052234 650_7 $$2INSPIRE$$aJuelich COSY PS
000052234 650_7 $$2INSPIRE$$ap p --> Phi(1020) 2p
000052234 7001_ $$0P:(DE-Juel1)VDB12182$$aMaeda, Y.$$b1$$uFZJ
000052234 7001_ $$0P:(DE-Juel1)VDB43804$$aKeshelashvili, I.$$b2$$uFZJ
000052234 7001_ $$0P:(DE-Juel1)VDB788$$aKoch, H. R.$$b3$$uFZJ
000052234 7001_ $$0P:(DE-HGF)0$$aMikirtytchiants, S.$$b4
000052234 7001_ $$0P:(DE-HGF)0$$aBarsov, S.$$b5
000052234 7001_ $$0P:(DE-Juel1)VDB147$$aBorgs, W.$$b6$$uFZJ
000052234 7001_ $$0P:(DE-Juel1)131108$$aBüscher, M.$$b7$$uFZJ
000052234 7001_ $$0P:(DE-HGF)0$$aDimitrov, V. I.$$b8
000052234 7001_ $$0P:(DE-HGF)0$$aDymov, S.$$b9
000052234 7001_ $$0P:(DE-Juel1)131187$$aHejny, V.$$b10$$uFZJ
000052234 7001_ $$0P:(DE-HGF)0$$aKleber, V.$$b11
000052234 7001_ $$0P:(DE-HGF)0$$aKoptev, V.$$b12
000052234 7001_ $$0P:(DE-Juel1)VDB4141$$aKulessa, P.$$b13$$uFZJ
000052234 7001_ $$0P:(DE-HGF)0$$aMersmann, T.$$b14
000052234 7001_ $$0P:(DE-HGF)0$$aMerzliakov, S.$$b15
000052234 7001_ $$0P:(DE-Juel1)VDB21644$$aMussgiller, A.$$b16$$uFZJ
000052234 7001_ $$0P:(DE-Juel1)VDB1136$$aNekipelov, M.$$b17$$uFZJ
000052234 7001_ $$0P:(DE-HGF)0$$aNioradze, M.$$b18
000052234 7001_ $$0P:(DE-Juel1)VDB1188$$aOhm, H.$$b19$$uFZJ
000052234 7001_ $$0P:(DE-Juel1)VDB1299$$aPysz, K.$$b20$$uFZJ
000052234 7001_ $$0P:(DE-Juel1)VDB1419$$aSchleichert, R.$$b21$$uFZJ
000052234 7001_ $$0P:(DE-Juel1)131344$$aStein, H. J.$$b22$$uFZJ
000052234 7001_ $$0P:(DE-Juel1)131349$$aStröher, H.$$b23$$uFZJ
000052234 7001_ $$0P:(DE-Juel1)VDB12183$$aWatzlawik, K.-H.$$b24$$uFZJ
000052234 7001_ $$0P:(DE-Juel1)133959$$aWüstner, P.$$b25$$uFZJ
000052234 773__ $$0PERI:(DE-600)1472655-5$$a10.1103/PhysRevLett.96.242301$$gVol. 96, p. 242301$$p242301$$q96<242301$$tPhysical review letters$$v96$$x0031-9007$$y2006
000052234 8567_ $$uhttp://hdl.handle.net/2128/1638$$uhttp://dx.doi.org/10.1103/PhysRevLett.96.242301
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