000026310 001__ 26310
000026310 005__ 20140130015401.0
000026310 037__ $$9arXiv$$anucl-ex/0301019$$cnucl-ex
000026310 035__ $$9arXiv$$zoai:arXiv.org:nucl-ex/0301019
000026310 035__ $$9DESY$$zD03-08296
000026310 035__ $$9SPIRESTeX$$zPatzold:2003tr
000026310 100__ $$aPatzold, J.$$uTubingen U.
000026310 245__ $$aStudy of the p p ---> p p pi+ pi- reaction in the low-energy tail of the Roper resonance
000026310 246__ $$9arXiv$$aStudy of the p p --> p p pi+ pi- reaction in the low-energy tail of the Roper resonance.
000026310 269__ $$c2003-01
000026310 300__ $$a5
000026310 520__ $$aExclusive measurements of the p p -> p p pi+ pi- reaction have been carried out at Tp = 775 MeV at CELSIUS using the PROMICE/WASA setup. Together with data obtained at lower energy they point to a dominance of the Roper excitation in this process. From the observed interference of its decay routes N* -> N sigma and N* -> Delta pi -> N sigma their energy-dependent relative branching ratio is determined.
000026310 65017 $$2INSPIRE$$aExperiment-Nucl
000026310 65017 $$2PACS$$a13.75.-n
000026310 65017 $$2PACS$$a14.20.Gk
000026310 65017 $$2PACS$$a25.40.Ve
000026310 690C_ $$2INSPIRE$$aPublished
000026310 693__ $$eCELSIUS-WASA
000026310 695__ $$2INSPIRE$$ap p: inelastic scattering
000026310 695__ $$2INSPIRE$$api: pair production
000026310 695__ $$2INSPIRE$$aN(1440): hadroproduction
000026310 695__ $$2INSPIRE$$achannel cross section: energy dependence
000026310 695__ $$2INSPIRE$$ap: angular distribution
000026310 695__ $$2INSPIRE$$amass spectrum
000026310 695__ $$2INSPIRE$$aangular distribution: two-pion
000026310 695__ $$2INSPIRE$$aexperimental results
000026310 695__ $$2INSPIRE$$aUppsala CELSIUS Stor
000026310 695__ $$2INSPIRE$$ap p --> 2p pi+ pi-
000026310 695__ $$2INSPIRE$$a0.775 GeV-cms
000026310 700__ $$aBashkanov, M.
000026310 700__ $$aBilger, R.
000026310 700__ $$aBrodowski, W.
000026310 700__ $$aCalen, H.
000026310 700__ $$aClement, H.
000026310 700__ $$aEkstrom, Curt
000026310 700__ $$aFransson, K.
000026310 700__ $$aGreiff, J.
000026310 700__ $$aHaggstrom, S.
000026310 700__ $$aHoistad, B.
000026310 700__ $$aJohanson, J.
000026310 700__ $$aJohansson, A.
000026310 700__ $$aJohansson, T.
000026310 700__ $$aKilian, K.
000026310 700__ $$aKullander, S.
000026310 700__ $$aKupsc, A.
000026310 700__ $$aMarciniewski, P.
000026310 700__ $$aMorosov, B.
000026310 700__ $$aOelert, W.
000026310 700__ $$aRuber, R.J.M.Y.
000026310 700__ $$aSchepkin, M.
000026310 700__ $$aScobel, W.
000026310 700__ $$aStepaniak, J.
000026310 700__ $$aSukhanov, A.
000026310 700__ $$aTurowiecki, A.
000026310 700__ $$aWagner, G.J.
000026310 700__ $$aWilhelmi, Z.
000026310 700__ $$aZabierowski, J.
000026310 700__ $$aZlomanczuk, J.
000026310 773__ $$a10.1103/PhysRevC.67.052202$$c052202$$pPhys.Rev.$$vC67$$y2003
000026310 8564_ $$uhttp://www.adsabs.harvard.edu/abs/2003PhRvC..67e2202P$$w2003PhRvC..67e2202P$$yADSABS
000026310 8564_ $$uhttp://dx.doi.org/10.1103/PhysRevC.67.052202$$w10.1103/PhysRevC.67.052202$$yDOI
000026310 8564_ $$uhttp://link.aps.org/abstract/PRC/V67/E052202/$$wV67/E052202/$$yPHRVA-C
000026310 902__ $$aTubingen U.
000026310 902__ $$aUppsala U.
000026310 902__ $$aHamburg U.
000026310 902__ $$aJulich, Forschungszentrum
000026310 902__ $$aDubna, JINR
000026310 902__ $$aMoscow, ITEP
000026310 902__ $$aWarsaw, Inst. Nucl. Studies
000026310 902__ $$aWarsaw U.
000026310 902__ $$aLodz, IPJ
000026310 909CO $$ooai:jdsweb.jinr.ru:26310$$pglobal
000026310 961__ $$x2003-02-03
000026310 961__ $$c2006-12-12
000026310 970__ $$aSPIRES-5464722
000026310 980__ $$aPublished
000026310 980__ $$aArxiv
000026310 980__ $$aCiteable
000026310 980__ $$aCORE
000026310 999C5 $$rnucl-th/9911080$$sPhys.Rev.,C62,025207
000026310 999C5 $$rnucl-th/0209009$$sPhys.Rev.,C66,065201
000026310 999C5 $$sPhys.Rev.,C61,024002
000026310 999C5 $$sPhys.Rev.Lett.,88,192301
000026310 999C5 $$rnucl-th/9706046$$sNucl.Phys.,A633,519
000026310 999C5 $$sNucl.Instrum.Meth.,A379,57
000026310 999C5 $$rnucl-th/9706003$$sPhys.Rev.,C56,3005
000026310 999C5 $$sPhys.Rev.,C23,1698
000026310 999C5 $$sPhys.Rev.,D6,3085
000026310 999C5 $$sNucl.Phys.,A386,571
000026310 999C5 $$sSov.J.Nucl.Phys.,37,540
000026310 999C5 $$sPhys.Rev.,187,1856
000026310 999C5 $$sNucl.Phys.,A712,75