000020163 001__ 20163 000020163 005__ 20240610121033.0 000020163 0247_ $$2DOI$$a10.1088/1742-6596/295/1/012119 000020163 0247_ $$2WOS$$aWOS:000297031400044 000020163 0247_ $$2Handle$$a2128/25165 000020163 035__ $$9SPIRESTeX$$zStephan:2011zz 000020163 037__ $$aPreJuSER-20163 000020163 082__ $$a530 000020163 1001_ $$0P:(DE-HGF)0$$aStephan, E.$$b0 000020163 245__ $$aVector and Tensor Analyzing Powers in Deuteron-Proton Breakup 000020163 260__ $$aBristol$$bIOP Publ.$$c2011 000020163 300__ $$a012119 000020163 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article 000020163 3367_ $$2DataCite$$aOutput Types/Journal article 000020163 3367_ $$00$$2EndNote$$aJournal Article 000020163 3367_ $$2BibTeX$$aARTICLE 000020163 3367_ $$2ORCID$$aJOURNAL_ARTICLE 000020163 3367_ $$2DRIVER$$aarticle 000020163 440_0 $$015961$$aJournal of Physics : Conference Series$$v295$$x1742-6588$$y1 000020163 500__ $$aRecord converted from VDB: 12.11.2012 000020163 520__ $$9IOP$$aVector and tensor analyzing powers of the breakup reaction at 130 and 100 MeV deuteron beam energies have been measured at KVI Groningen with the use of the detection systems covering large fractions of the phase space. The high precision data are compared to the theoretical predictions based on various approaches to describe the three nucleon (3N) system dynamics. Theoretical predictions describe very well the vector analyzing power data, with no need to include any three-nucleon force effects fo r these observables. The tensor analyzing powers can be also very well reproduced by calculations in most of the studied region, but locally certain discrepancies are observed. At 130 MeV for Axy such discrepancies usually appear, or are enhanced, when mo del 3N forces (3NFs), TM99 or Urbana IX, are included. Problems of all theoretical approaches with describing Axx and Ayy are limited to very small regions of the phase space, usually characterized with the lowest relative energies of the two protons. Pre dicted effects of 3NFs are much lower at 100 MeV, therefore at this energy equally good consistency between the data and the calculations is obtained with or without 3NFs. 000020163 536__ $$0G:(DE-Juel1)FUEK413$$2G:(DE-HGF)$$aPhysik der Hadronen und Kerne$$cP53$$x0 000020163 7001_ $$0P:(DE-HGF)0$$aKistryn, S.$$b1 000020163 7001_ $$0P:(DE-HGF)0$$aKalantar-Nayestanaki, N.$$b2 000020163 7001_ $$0P:(DE-HGF)0$$aBiegun, A.$$b3 000020163 7001_ $$0P:(DE-HGF)0$$aBodek, K.$$b4 000020163 7001_ $$0P:(DE-HGF)0$$aCiepal, I.$$b5 000020163 7001_ $$0P:(DE-HGF)0$$aDeltuva, A.$$b6 000020163 7001_ $$0P:(DE-HGF)0$$aEslami-Kalantari, M.$$b7 000020163 7001_ $$0P:(DE-HGF)0$$aFonseca, A. C.$$b8 000020163 7001_ $$0P:(DE-HGF)0$$aGasparic, I.$$b9 000020163 7001_ $$0P:(DE-HGF)0$$aGolak, J.$$b10 000020163 7001_ $$0P:(DE-HGF)0$$aJamroz, B.$$b11 000020163 7001_ $$0P:(DE-HGF)0$$aJoulaeizadeh, L.$$b12 000020163 7001_ $$0P:(DE-HGF)0$$aKamada, H.$$b13 000020163 7001_ $$0P:(DE-HGF)0$$aKis, M.$$b14 000020163 7001_ $$0P:(DE-HGF)0$$aKlos, B.$$b15 000020163 7001_ $$0P:(DE-HGF)0$$aKozela, A.$$b16 000020163 7001_ $$0P:(DE-HGF)0$$aMahjour-Shafiei, M.$$b17 000020163 7001_ $$0P:(DE-HGF)0$$aMardanpour, H.$$b18 000020163 7001_ $$0P:(DE-HGF)0$$aMesschendorp, J.$$b19 000020163 7001_ $$0P:(DE-HGF)0$$aMicherdzinska, A.$$b20 000020163 7001_ $$0P:(DE-HGF)0$$aMoeini, H.$$b21 000020163 7001_ $$0P:(DE-Juel1)131273$$aNogga, A.$$b22$$uFZJ 000020163 7001_ $$0P:(DE-HGF)0$$aRamazani-Moghaddam-Arani, A.$$b23 000020163 7001_ $$0P:(DE-HGF)0$$aSkibinski, R.$$b24 000020163 7001_ $$0P:(DE-HGF)0$$aSworst, R.$$b25 000020163 7001_ $$0P:(DE-HGF)0$$aWitala, H.$$b26 000020163 7001_ $$0P:(DE-HGF)0$$aZejma, J.$$b27 000020163 773__ $$0PERI:(DE-600)2166409-2$$a10.1088/1742-6596/295/1/012119$$gVol. 295, p. 012119$$p012119$$q295<012119$$tJournal of physics / Conference Series$$v295$$x1742-6588$$y2011 000020163 8567_ $$uhttp://dx.doi.org/10.1088/1742-6596/295/1/012119 000020163 8564_ $$uhttps://juser.fz-juelich.de/record/20163/files/Stephan_2011_J._Phys.%20_Conf._Ser._295_012119.pdf$$yOpenAccess 000020163 8564_ $$uhttps://juser.fz-juelich.de/record/20163/files/Stephan_2011_J._Phys.%20_Conf._Ser._295_012119.pdf?subformat=pdfa$$xpdfa$$yOpenAccess 000020163 909CO $$ooai:juser.fz-juelich.de:20163$$pdnbdelivery$$pdriver$$pVDB$$popen_access$$popenaire 000020163 9131_ $$0G:(DE-Juel1)FUEK413$$bStruktur der Materie$$kP53$$lPhysik der Hadronen und Kerne$$vPhysik der Hadronen und Kerne$$x0 000020163 9132_ $$0G:(DE-HGF)POF3-511$$1G:(DE-HGF)POF3-510$$2G:(DE-HGF)POF3-500$$aDE-HGF$$bKey Technologies$$lSupercomputing & Big Data $$vComputational Science and Mathematical Methods$$x0 000020163 9141_ $$y2011 000020163 915__ $$0StatID:(DE-HGF)0020$$aNo peer review 000020163 915__ $$0StatID:(DE-HGF)0010$$aJCR/ISI refereed 000020163 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess 000020163 915__ $$0LIC:(DE-HGF)CCBY4$$2HGFVOC$$aCreative Commons Attribution CC BY 4.0 000020163 9201_ $$0I:(DE-Juel1)IKP-3-20111104$$gIKP$$kIKP-3$$lTheoretische Kernphysik$$x0 000020163 970__ $$aVDB:(DE-Juel1)135274 000020163 9801_ $$aFullTexts 000020163 980__ $$aVDB 000020163 980__ $$aConvertedRecord 000020163 980__ $$ajournal 000020163 980__ $$aI:(DE-Juel1)IKP-3-20111104 000020163 980__ $$aUNRESTRICTED 000020163 981__ $$aI:(DE-Juel1)IAS-4-20090406