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The tubmitteg,\anutaopt#has bmn authored by a contr,ymr of,he fj s GW~rnment under contract No, W31109ENG38 A~ardkgly, the U S Gowrnmanc retains a nonexclusive, rovalwfree lcansu to publish Or rwoduco thu publiihed fmm Of this contribution, or allow o!hdr$ to do so, for U S Government Gurpasa ~iece~ved 1 SEP2H 999 (z)s~l Study of Hyperon-Nucleon nteractions with d(e, e K) Reactions T-S H Leea, V Stoksa*, B Saghaib, C Fayardc Physics Division, Argonne National Laboratory, Argonne, llinois 60439, USA bservice de Physique Nue16aire, CEA-Saclay, F-91191 Gif-sur-Yvette Cedex, i?ance Cnstitut de Physique Nuc16aire de Lyon, N21?3-CNRS, Universit6 Claude Bernard, F-69622 Villeurbanne Cedex, fiance Abstract The dependence of the d(ej e K+) reaction cross sections on the hyperon-nucleon interactions is investigated t is shown that the data obtained with Longitudinal- l%msverse separation or polarized photons can distinguish a class of Nijmegen models of hyperonnucleon interactions which are X2-equivalent in fitting the existing 35 data points of hyperon-nucleon reactions The study of hypernuclei has been mainly based on the phenomenological shell model[l] This is highly unsatisfactory for exploring the question concerning how hyperons behave in nuclear medium, an interesting and fundamental question often raised in the study of QCD effects in nuclear medium as well as in the study of relativistic heavy-ion collisions To make progress, it is necessary to develop a many-body approach starting with realistic hyperon-nucleon and hyperon-hyperon interactions Obviously, the success in this direction depends entirely on the accuracy of the starting hyperon-nucleon and hyperon-hyperon interactions The SU(3) flavor symmetry has been the guiding principle in developing [2,3] theoretical models for these interactions The data for testing these models are however very limited While using the SU(3) symmetry, it is still possible to generate many hyperon-nucleon potentials which give equally good descriptions of the existing 35 data points of hyperon-nucleon reactions To develop a many-body approach to hypernuclear physics, we clearly need to use more reaction data to distinguish these models n this work we consider d(e, e K+) reaction which has been the focus of a recent experiment at TJNAF, as reported by J Reinhold at this conference n our calculations, the amplitude for the d(e, e K+) reaction is written as Z (E) = w qq + 2W)(E) (1) where T(imp) is due to the production of K+Y on one of the nucleons in the deuteron, This work was supported in part by the US Department of Energy, Nuclear Physics Division, under Contract No W-31-109-ENG-38 -

DSCLAMER This repoti was prepared as an account of work sponsored byanagency of the Uriited States Government Neither the United States Government nor any agency thereof, nor any of their employees, make any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof The views and opinions of authors expressed herein do not necessarily state or reflect those of the United States Government or any agency thereof

,, - - DSCLAMER Portions of this document may be iilegible in electronic image products mages are produced from the best available original document

2 Tt~gilcontains theeffects duetothe final YNscattering Foragiven final hyperon-nucleon state YV, these two amplitudes are calculated from the following matrix elements and T(fsi)(E)= ~ (YiV tyv,y~v/(17)gyn/ (13) [~ ~Yuvwv(~)] i~~), (3) YN, i=l,2 where ~YN,7~ is the kaon production amplitude, Ld is the deuteron wave function, GYN is the propagator of the intermediate YN state, and tyn,ynlis the hyperon-nucleon scattering t-matrix The deuteron wave function can be generated accurately iiom the well-developed nucleon-nucleon potentials The Kaon production amplitude can be determined from the data of TN + KY and V(e, e K)Y reactions n this work we employ the model developed by a Saclay-Lyon collaboration[5] n addition to imposing the SU(3) symmetry, the unknown parameters of this model are determined from a global fit to all existing data This model is currently being refined by introducing the off-shell effects to account for the new data from TJNAF and Bonn With these two theoretical inputs fixed in the calculation of Eqs (l)-(3), we can explore how the data of the d(~, K)YN reaction can be used to distinguish the constructed hyperon-nucleon models We have carried out calculations for five YN models recently constructed by Rijken and Stoks[4] using the approach developed by the Nimegen group[2] These five models, yield the same X2 N 16 in fitting the existing 35 data points of YN reactions However, they predict very dfferent phase shifts and are very different in the short-rsnge parts of the potentials 012 010 008 006 004 002 000 }!! t 1 1 1 t 208 21 212 214 8 Figure 1 The differential cross section (in unit of @/GeV2-Sr2) of d(e,e K+) at Q2 = 0367 (GeV/c)2, d~ = 15 as a function of An invariant mass (GeV) The solid (dotted) curve is from full (impulse approximation) calculation ~,1;- ~,*~v>,-~ <--,T~L-f,7- ;>T+,T,-Z nm!yy+%~ 77 ---! >,!,<~?> :- - ~, -~ :---, w,7- --, - ----

-- -,- --,m ---+&& w,m,,,-, 7m F- +>,,= --V-,==-----m --4- -= -, -me--, ------- ----s-= -- --- d 3 n this short contribution we will only present results for A productions calculated fkom two of the constructed X2-equivalent potentials The calculations including X production are in progress All results are for the experiment at TJNAF at 8K = 15, Q2 = 0376 (GeV/c)2 The predicted observable are plotted as functions of the invarizmt mass M= of the outgoing An system n Fig 1, we illustrate the importance of the An final state interaction As expected, it generates the cusp structure due to the opening of the ZN channel However the difference between the full calculation (solid curve) and the impulse approximation calculation (dotted curve) is not large enough for distinguishing the considered X2-equivalent YN models Here, we observe that the predicted magnitudes are is about 2070 lower the the preliminary data report by J Reinhold at this conference This discrepancy could be reduced if the Z production is included in the calculation The progress in determining YN interactions can be made if we can separate the longitudinal parts of the cross sections in the measurements This is illustrated in Fig 2 Here we see that the differences between two considered YN models are very striking, in particular at energies near the Z production threshold 0006 0005 F j 0004 0003 ()0(-)2 0001 0000 1,,,,,,,,,,,,,,,,,,,,: 208 21 212 214 Figure 2 The longitudinal differential cross, section (in unit of pb/gev2 Sr2) at Q2 =0367 (GeV/c)2, t9~= 15 as a function of An invariant mass (GeV) The solid (dotted) curve is from using YN Mode (V) of Ref 4 For possible future experiments with polarized photons at the newly constructed SPring- 8 facility in Japan, we have also made predictions for the photon asymmetry at Q2 = O and d~ = OO The results are shown in Fig 3 Again, we see the striking differences between the considered two YN models

4 n summary, we have developed an approach to investigate the YN interactions using the d(e, e ~) and ~ + d ~ K + Y + N reactions t is shown that the data for Longitudinal-Transverse separation and photon symmetries will be very useful in distinguishing X2-equivalent YN models This is a necesssry step in developing a many-body approach to hypernuclear physics starting with realistic hyperon-nucleon and hyperonhyperon interactions 010 1 1 1 1 i 1 8 1 1 t 1 1 i 1 1 005 000-005 -010 ~ ; ; ; --, -------------------- -------------------- --- Fttl,,,, l,, Al,!,,,,,,= 208 21 212 214 4 Figme 3 Same as Fig 2 except for photon asymmetry at Q2 = O, (?~= 15 REFEitENCES 1 DJ Millener, A Gal, CB Dover, and DH Dalitz, Phys Rev C31 (1985) 499 2 PMM Maessen, TA Rijken and JJ de Swart, Phys Rev C40 (1989) 2226 3 B Holzenkamp, K Holinde, and J Speth, Nucl Phys A500 (1989) 485; A Reuber, K Holinde, and J Speth, Nucl Phys A570 (1994) 543 4 Th A Rijken, contribution to this conference; Th A Rijken, V Stoks, and Y Yamamoto, in preparation 5 JC David, C Fayard, GH Lamot, and B Saghai, Phys Rev C53 (1996) 2613 7-4,- -, - 7-- ---wrxt--vn - r,7t-a-- -a -, --, -- --T--, :- rt 7-n----, -,-- -- -