ebook img

SAID Analysis of Meson Photoproduction : Determination of Neutron and Proton EM Couplings PDF

0.31 MB·
Save to my drive
Quick download
Download
Most books are stored in the elastic cloud where traffic is expensive. For this reason, we have a limit on daily download.

Preview SAID Analysis of Meson Photoproduction : Determination of Neutron and Proton EM Couplings

TheJournal’snamewillbesetbythepublisher DOI:willbesetbythepublisher (cid:13)c Ownedbytheauthors,publishedbyEDPSciences,2014 SAID Analysis of Meson Photoproduction: Determination of Neutron and Pro- ton EM Couplings IgorStrakovsky1,a,WilliamBriscoe1,AlexanderKudryavtsev2,1,VladimirTarasov2,andRonWorkman1 1InstituteforNuclearStudies,DepartmentofPhysics,TheGeorgeWashingtonUniversity,Washington,DC20052,USA. 4 2InstituteofTheoreticalandExperimentalPhysics,Moscow,117259Russia. 1 0 2 Abstract.WepresentanoverviewoftheGWSAIDgroupefforttoanalyzeonnewpionphotoproductionon both proton- and neutron-targets. The main database contribution came from the recent CLAS and MAMI n unpolarized and polarized measurements. The differential cross section for the processes γn → π−p was a J extractedfromnewmeasurementsaccountingforFermimotioneffectsintheimpulseapproximation (IA)as wellasNN-andπNeffectsbeyondtheIA.Theelectromagneticcouplingresultsarecomparedtootherrecent 3 studies. 1 ] h p SAIDforBaryonSpectroscopy. Thepropertiesofthe sections requires the use of a model-dependent nuclear - resonances for the non-strange sector have been deter- correction, which mainly comes from final-state interac- p minedalmostentirelyfromtheresultsofπNelastic scat- tions (FSI) [6]. As a result, our knowledge of the neu- e h tering analyses [1]. Meson photoproduction reactions tral resonance couplings is less precise than that of the [ havemainlyservedtofixelectromagnetic(EM)couplings. charged values for well-known low-laying baryons. The With the refinement of multichannel fits and the avail- uncertainties for such kind of neutral states with JP = 1, 1 2 v ability of highprecision photoproduction data for both forinstance,N(1440)1/2+,N(1535)1/2−,andN(1650)1/2− 7 single- and double-meson production, identifications of vary from 25% to 140% [1]. Some of the N∗ baryons 2 some new states have emerged mainly due to evidence [N(1675)5/2−, for instance] have stronger EM couplings 0 fromreactionsnotinvolvingsingle-pion-nucleoninitialor totheneutronthantotheproton,butparametersarevery 3 final states [1]. The GW SAID N∗ program consists of uncertain (N∗ → γp : +0.019 ± 0.008 GeV−1/2 while . 1 πN →πN,γN →πN,andγ∗p→πN componentsaswas N∗ → γn : −0.043±0.012GeV−1/2 [1]). Then, PDG12 0 establishedbyDickArndton1997.Assumingdominance estimates for the A and A proton decay amplitudes 4 1/2 3/2 oftwohadronicchannels[πNelastic andπN → ηN], we of the N(1720)3/2+ state are consistent with zero, while 1 : parametrize γ∗p → πN in terms of πN → πN ampli- the recent SAID determination [2] gives small but non- v tudes([2] and referencestherein). Most ofthe pionpho- vanishing values. Other unresolved issues relate to the i X toproduction analyses use SAID πN partial-wave analy- second P , N(1710)1/2+, that we do not seen in the re- 11 r sis(PWA)outcome[3]oritsmodificationasinputforthe cent SAID πN PWA [3] contraryto the findings of other a constraint as well. However, beyond πN elastic scatter- PWAsreferencedbyPDG12[1]. ing, single-pion photoproduction remains the most stud- Pionphotoproductionofftheproton. The overall ied source of resonance information. Much of the ef- SAID χ2 has remained stable (χ2/data = 2.1) against the fort aimed at providing complete or nearly complete in- growing database, which has increased by a factor of 2 formation for meson-nucleon photoproduction reactions since 1995 (13.4k up to 27.3k data points) [7]. Most of has been directed to measuring double-polarization ob- thisincreasecomingfromphoton-taggingfacilities. More servables. However,oftenoverlookedisthatthedatacov- completedatasetsfordouble-andsingle-polarizationob- erage for severalsingle-polarizationobservables, also vi- servables for pion photoproduction can offer important talindeterminingthepropertiesofthenucleonresonance constraintsonanalysesofthephotoproductionreaction. spectrum,stillremainsincomplete. Herewefocusonthesingle-pionproductiondataand Using linearly polarized photons and an unpolarized notethatacompletesolutionrequirescouplingsfromboth target, CLAS provides a large set of beam asymmetry Σ charged and neutral resonances [4, 5], the latter requir- measurements for γp → π0p and γp → π+n from Eγ ing π−p and π0n photoproduction off a neutron target, = 1.100 and up to 1.860 GeV in laboratory photon en- typically a neutron bound in a deuteron target. Extrac- ergy, corresponding to a CM energy W range of 1.7 − tion of the two-body (γn → π−p and γn → π0n) cross 2.1 GeV (θ = 30 − 150◦ of pion production angle in CM) [8]. Its contribution to the world database is more ae-mail:[email protected] than doubled [7]. In Figs. 1, we show the effect of new TheJournal’sname Table1.ProtonhelicityamplitudesspA1/2and pA3/2(in Pionphotoproductionofftheneutron. In addition to [(GeV)−1/2×10−3]units). being less precise, experimental data for neutron-target photoreactionsaremuchlessabundantthanthoseutilizing Resonance pA1/2 pA3/2 Ref. aprotontarget,constitutingonlyabout15%ofthepresent ∆(1700)3/2− 132±5 108±5 SAIDDU13[8] SAID database [7]. At low to intermediate energies, this 105±5 92±4 SAIDCM12[2] lackofneutron-targetdataispartiallycompensatedbyex- 160±20 165±25 BnGa12[10] periments using pionic beams, e.g., π−p → γn, as has 58±10 97±8 Kent12[11] been measured, for example, by the Crystal Ball Collab- 226 210 MAID[9] oration at BNL [15] for the inverse photon energy E = γ 104±15 85±22 PDG12[1] 285−690MeVandθ=40−150◦,whereθistheinverse ∆(1905)5/2+ 20±2 −49±5 SAIDDU13[8] productionangle of pion in the CM frame. This process 19±2 −38±4 SAIDCM12[2] is free from complications associated with the deuteron 25±5 −49±4 BnGa12[10] target. However, the disadvantage of using the reaction 66±18 −223±29 Kent12[11] π−p → γn forthe pionphotoproductionstudy isthe 5 to 18 −28 MAID[9] 500 times larger cross sections for π−p → π0n → γγn, 26±11 −45±20 PDG12[1] dependingonE andθ. γ Weextracttheγn→π−pcrosssectiononfreenucleon from the deuteron data in the quasi-free (QF) kinematic CLAS Σ measurements in terms of partial cross sections regionof the γd → π−pp reactionwith fast knocked-out from SAID (CM12 [2] and recent DU13 [8] included proton and slow proton-spectator assumed not to be in- new CLAS data) and MAID [9]. While the CM12 and volved in the pion production process. In this, so-called DU13 solutions differ over the energy range of the re- impulseapproximation(IA)[16],thereactionmechanism centCLASexperiment,theresonancecouplingsarefairly correspondstothediagraminFig.3(a).Thereare2critical stable. The largest change is found for the ∆(1700)3/2− factorstobetakenintoaccountwhenusingthisapproach: and ∆(1905)5/2+ states, for which the various analyses (i)theneutronisboundand(ii)thereareNN-andπN-FSI disagreesignificantlyintermsofphoto-decayamplitudes effects. (Table1). Item(i)meansthattheeffectivemassoftheneutronis not equal to the mass of the free neutron. In our former analyses[17,18],theγn →π−pamplitudeforagivenE γ andCMpionproductionangleθisassumedtobethesame asonafreeneutronatrest. Thatiswhythecrosssection obtainedshouldbeconsideredasanaverageoverenergies aroundE . Thesizeoftheaveragingregionisdetermined γ byasmearingoftheenergyowingtotheFermi-motionin thedeuteron.Thetypicalscalehereis20MeVinenergy. Item (ii) corresponds to the inclusion of the FSI cor- rections. Their leading terms correspond to Feynman diagrams shown on Fig. 3(b,c). Determinations of the γd → π−ppdifferentialcrosssection, with theFSI taken into account (all the diagrams on Fig. 3, were included) weredonerecentlyfortheCLAS[17]andMAMI-B[18] γd → π−pp data. The SAID phenomenological am- Figure1. Partial cross sections for multipoles withthe largest plitudes for γN → πN [19], NN-elastic [20], and πN- changewasfoundafterincludingthenewCLASdatainthefit, elastic[3]wereusedasinputstocalculatethediagramsin ∆(1700)3/2− and∆(1905)5/2+. Solid(dash-dotted) linescorre- Fig.3. TheBonnpotential[21]wasusedforthedeuteron spondtotheSAIDDU13[8](CM12[2])solution. Dashedlines give MAID07 [9], Vertical arrows indicate resonance energies description. W andhorizontalbarsshowfullΓ widthsassociatedwiththe Recently,weappliedourFSIcorrections[22]toCLAS R πN SAIDπNsolutionWI08[3]. γd → π−pp data (E = 1050 − 2700 MeV and θ = 30 γ − 160◦) [23] to get elementary cross sections for γn → π−p [17]. New CLAS differentialcrosssectionsare qua- Withtheinclusionofnewhigh-precisiondata,ourfits druplingtheworlddatabase forγn → π−p above1GeV. are becomingmore stable and predictive. Plots of recent The FSI correction factor for the CLAS kinematics was doublepolarizedG data, coveredE = 630 − 1300MeV found to be small, ∆σ/σ < 10%. However, these new γ andθ=20−160◦,inFig.2fromCB-ELSA[12]showthat crosssectionsdepartedsignificantlyfromourpredictions theSAIDCM12fitgivesagoodpredictionofthisquantity. at the higherenergies, and greatlymodified the fit result, WehaverecentlyanalyzedC (E =460−1340MeVand which allows to determine new neutron couplings (Ta- x′ γ θ = 75− 140◦) [13] andpreliminary F andT data (E = ble2). γ 440 − 1430 MeV and θ = 30 − 160◦) [14] from Mainz, In our recent study [18], we addressed to the differ- findingasimilarlyquantitativelevelofagreement. ential cross section measurements for γn → π−p in the MENU2013 Figure2. Thedouble-polarizationobservableGasafunctionofpionproductionangleinCM.Dashed(solid)linescorrespondtothe SAID(DU13[8]andpreliminarysolutionincludednewCB-ELSAGmeasuremenents. Dotted(dash-dotted)linesgiveBnGa12[10] (MAID07[9]). ∆-isobarregion.ThedatacamefromMAMI-B(E =300 from the previous SAID SN11 [25] determination and γ − 455 MeV and θ = 60 − 140◦) [24]. At energies dom- PDG12 [1] values, e.g., for N(1650)1/2−, N(1675)5/2−, inated bythe ∆-resonance, the isospinI = 3/2multipoles and N(1680)5/2+. While BnGa13 group [26] used the areconstrainedbyextensivestudiesperformedusingpro- same (almost) data to fit them as we are while BnGa13 ton targets. The forwardpeaking structure is due largely hasseveralnew adhocresonances. Meanwhile,BnGa13 totheBorncontribution,whichiswellknown.Asaresult, determinationisdifferentforN(1535)1/2−,N(1650)1/2−, onewouldexpectmodelstogivepredictionswithinatight andN(1680)5/2+. range. Summary. Future progress in the database develop- γ π− γ π− γ p1,2 ment is expecting from tagged-photon fasilities as JLab, MAMI-C, SPring-8, CB-ELSA, and ELPH. Partial-wave p1,2 analyseswillclearlybenefitfromtheconstraintsprovided p1 π− bythesenewdata,whichhighlighttheimportanceofnew d p2,1 d p2 d p2,1 polarization observables in providing a stringent test of (a) (b) (c) PWA, even in kinematic regions where a large number Figure3. Feynmandiagramsfortheleadingtermsoftheγd → of cross section and polarization observables are already π−ppamplitude.(a)IA,(b)pp-FSI,and(c)πN-FSI.Filledblack presentintheworlddatabase.AnaccuratePWAmustulti- circlesshowFSIvertices. Wavy,dashed,solid,anddoublelines matelydescribeacompletesetofobservables.Thecurrent correspond to the photons, pions, nucleons, and deuterons, re- data and future experiments exploiting these polarimetry spectively. developmentsat large acceptance detectors will be a key parttoachievingthiscompletemeasurement. Wehaveincludedthenewneutroncrosssectionsfrom In this regard, future experiments to measure unpo- theCLASandMAMI-Bexperimentsinanumberofmul- larized and the spin polarization of neutrons are already tipole analyses covering incident photon energies up to planned at MAMI-C. Measurements of such observables 2.7 GeV, using the full SAID database [7], in order to with large acceptance are crucial to the world program gauge the influence of these measurements, as well as aiming to determine the excitation spectrum of the nu- their compatibility with previous experiments. The so- cleon. lution, GB12 [17], uses the same fitting form as our re- We proposed to perform a precision measurement of cent SN11 solution [25]. A second fit, GZ12, instead dσ/dΩ in the reactions γd → π−pp and γd → π0np usedtherecentlyproposedformbasedonaunifiedChew- in the tagged-photon energy region from threshold to Mandelstamparametrizationofthe GWDACfits to both 800 MeV [27] and then to 1500 MeV [28]. The dσ/dΩ πNelasticscatteringandphotoproduction[2]. for the processes γp → π−p and γp → π0n will be ex- Table 2 shows that the new SAID GB12 nA and tractedfromtheseCB@MAMI-Cmeasurementsaccount- 1/2 nA helicities sometimes have a significant deviation ingforFermimotioneffectsinIA[16]aswellasNN-and 3/2 TheJournal’sname Table2.NeutronhelicityamplitudesnA andnA (in[(GeV)−1/2×10−3]units). 1/2 3/2 Resonance nA Resonance nA nA Ref. 1/2 1/2 3/2 N(1535)1/2− −58±6 N(1520)3/2− −46±6 −115±5 SAIDGB12[17] −60±3 −47±2 −125±2 SAIDSN11[25] −93±11 −49±8 −113±12 BnGa13[26] −49±3 −38±3 −101±4 Kent12[11] −46±27 −59±9 −139±11 PDG12[1] N(1650)1/2− −40±10 N(1675)5/2− −58±2 −80±5 SAIDGB12[17] −26±8 −42±2 −60±2 SAIDSN11[25] 25±20 −60±7 −88±10 BnGa13[26] 11±2 −40±4 −68±4 Kent12[11] −15±21 −43±12 −58±13 PDG12[1] N(1440)1/2+ 48±4 N(1680)5/2+ 26±4 −29±2 SAIDGB12[17] 45±15 50±4 −47±2 SAIDSN11[25] 43±12 34±6 −44±9 BnGa13[26] 40±5 29±2 −59±2 Kent12[11] 40±10 29±10 −33±9 PDG12[1] πN-FSIeffectsbeyondtheIA.Databelow800MeVwere man et al., Phys. Rev. Lett. 110, 169101 (2013); takeninMarchof2013andanalysisisinprogress.Conse- A.Thiel(CBELSA/TAPSCollaboration)etal.,Phys. quentialcalculationsoftheFSI corrections,asdeveloped Rev.Lett.110,169102(2013). byourGW-ITEPCollaboration,willbeapplied. Wewill [13] M.H. Sikora (A2 Collaboration) et al., extend our FSI code [22] to extractγn → π0n data from arXiv:1309.7898. γd → π0np measurements as well. Polarized measure- [14] V. Kashevarov, Proceedings of MENU 2013 work- mentswillhelptobringmorephysicsin. FSIcorrections shop. needtoapply. [15] A. Shafi et al. (Crystal Ball Collaboration), Phys. Acknowledgments. This work was supported in part Rev.C70,035204(2004). bytheU.S.DOEGrantNo. DE-FG02-99ER41110. [16] G. Chew and M. Goldberger, Phys. Rev. 87, 778 (1952). [17] W.Chenetal.,Phys.Rev.C86,015206(2012). References [18] W.J.Briscoeetal.,Phys.Rev.C86,065207(2012). [1] J.Beringeretal.(ParticleDataGroup),Phys.Rev.D [19] M. Duggeret al. (CLAS Collaboration),Phys. Rev. 86,010001(2012). C76,025211(2007). [2] R.Workmanetal.,Phys.Rev.C86,015202(2012). [20] R.A.Arndtetal.,Phys.Rev.C76,025211(2007). [3] R.A.Arndtetal.,Phys.Rev.C74,045205(2006). [21] R.Machleidt,K.Holinde,andC.Elster,Phys.Rept. [4] K.M.Watson,Phys.Rev.95,228(1954). 140,1(1987). [5] R.L.Walker,Phys.Rev.182,1729(1969). [22] V.E.Tarasovetal.,Phys.Rev.C84,035203(2011). [6] A.B.Migdal,JETP1,2(1955);K.M.Watson,Phys. [23] W. Chen et al. (CLAS Collaboration), Phys. Rev. Rev.88,1163(1952). Lett.103,012301(2009). [7] Institute of Nuclear Studies of GW Database [24] J.Ahrens,etal.(GDHandA2Collaborations),Eur. (W.J.Briscoe,I.I.Strakovsky,andR.L.Workman); Phys.J.A44,189(2010). http://gwdac.phys.gwu.edu/analysis/pr_analysis.html [25] R.Workmanetal.,Phys.Rev.C85,025201(2012). [8] M.Duggeretal.(CLASCollaboration),Phys.Rev.C [26] A.Anisovichetal.,Eur.Phys.J.A49,67(2013). 88,065203(2013). [27] Meson production off the deuteron, Spokespersons: [9] D.Drechseletal.,Eur.Phys.J.A34,69(2007). W.J. Briscoe and I.I. Strakovsky, MAMI Proposal [10] A.Anisovichetal.,Eur.Phys.J.A48,15(2012). MAMI-A2-02/12,Mainz,Germany,2012. [11] M. Shrestha and D.M. Manley, Phys. Rev. C 86, [28] Meson production off the deuteron. II, Spokesper- 055203(2012). sons: W.J. Briscoe, V.V. Kulikov,K. Livingston,and [12] A. Thiel (CBELSA/TAPS Collaboration) et al., I.I. Strakovsky, MAMI Proposal MAMI-A2-02/13, Phys. Rev. Lett. 109, 102001 (2012); R.L. Work- Mainz,Germany,2013.

See more

The list of books you might like

Most books are stored in the elastic cloud where traffic is expensive. For this reason, we have a limit on daily download.