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Atsushi Tokiyasu (for LEPS collaboration) Experimental Nuclear and Hadronic Physics Laboratry, Department of Physics, Kyoto University.

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Presentation on theme: "Atsushi Tokiyasu (for LEPS collaboration) Experimental Nuclear and Hadronic Physics Laboratry, Department of Physics, Kyoto University."— Presentation transcript:

1 Atsushi Tokiyasu (for LEPS collaboration) Experimental Nuclear and Hadronic Physics Laboratry, Department of Physics, Kyoto University

2 strangeness in nuclei 2013/2/13 GCOE Symposium @ Kyoto University1 / 11 ds us, SU(3) octet baryonSU(3) nonet meson  ? Hyper nuclei Shrinkage  impurity effect. nuclear force in SU(3) Kaonic nuclei new form of the nuclei whether exist or not? What happens in nuclei? uds hyperon kaon

3 dependent on the models of KN interaction the calculation methods. Formation of Cold (T=0) and Dense  > 2  0 ) nuclei. 2013/2/13 GCOE Symposium @ Kyoto University2 / 11 K can be bound in the nuclei by strong interaction. K N interaction (I=0) is strongly attractive ! X-ray shift of Kaonic Hydrogen K - p scattering data 2-body: KN :  (1405) ? 3-body: KNN : lightest nucleus. K - pp  the strongest bound state in 3-body systems Theoretical prediction (All theory support the existence) B.E. = 20-100 MeV  = 40- 110 MeV If  > B.E, it is difficult to observe experimentally. Ref: Particle Data Group Kaonic nuclei

4 Experiments 2013/2/13 GCOE Symposium @ Kyoto University3 / 11 FINUDA @ DA  NE (2005) DISTO@ SATURNE(2010) stropped K - on ( 6 Li, 7 Li, 12 C, 27 Al and 51 V) p p   p K + B.E. =  = invariant mass (  + p)Missing mass (   ) MeV M.Agnello, Nagae and Fujoka et al., PRL 94, 212303 (2005)T.Yamazaki et al., PRL 104, 132502 (2010) K - pp   p,   p,   n (non-mesonic decay)  easy to identify experimentally   p  (mesonic decay)

5 Summary of the introduction K - pp is the lightest kaonic nuclei. Existence of K - pp is not established. Experimental search using different reactions are awaited! Forthcoming experiments 3 He(K -, n)X  E15 @ J-PARC D(  +, K + )X  E27 @ J-PARC  D  K +  - X  LEPS @ SPring-8 2013/2/13 GCOE Symposium @ Kyoto University4 / 11  Prof.Nagae’s talk

6  D  K +  - X reaction 2013/2/13 GCOE Symposium @ Kyoto University5 / 11 K+K+ --  “K” exchanged in t-chanel  unique for  -induced reaction  ( J = 1)  polarization observables are available. K - pp is “soft” object.  small momentum transfer  detect K + and  - at forward angle Search for a bump structure in the missing mass spectrum M x 2 = (E  + M D – E K - E  ) 2 - (p  – p K - p  ) 2  independent of decay chanel. K, K* Y* p n p K-K- p (E , p  ) (E , p  ) (E , p  ) (M D,0) Y* door-way.

7 SPring-8 “Super Photon ring-8 GeV” 2013/2/13 GCOE Symposium @ Kyoto University6 / 11 Data take: 2002/2003, 2006/2007  7.6 x 10 12 photons on LD 2 target SPring-8: 8 GeV electron storage-ring LEPS : hadron physics using  beam Back-word Compton Scattering e e Detect with Tagging counter E  =1.5 - 2.4 GeV experimental hatch  355nm laser 8 GeV LEPS  E  =12 MeV

8 LEPS spectrometer 2013/2/13 GCOE Symposium @ Kyoto University7 / 11 TOF Dipole Magnet 0.7 [Tesla] Target Start Counter DC2DC3 DC1SVTX AC(n=1.03) SSD (SVTX) Drift Chamber (DC 1~3) position Start Counter (SC) Time of flight wall (TOF) time Aerogel Cherencov counter (AC) Start Counter (SC) trigger   GeV  -- K+K+

9 particle identification 2013/2/13 GCOE Symposium @ Kyoto University8 / 11 K+K+ --  p/p ~ 6 MeV/c @ 1 GeV/c TOF (Time of flight) m 2 = p 2 (1/β 2 - 1) line tracking + Runge-Kutta method. mass p = 938.3 MeV mass K + = 493.7 MeV mass  - = 139.6 MeV c.f. p ++ K-K- 0

10 Missing Mass Spectrum 2013/2/13 GCOE Symposium @ Kyoto University9 / 11 Error Bar : statistical uncertainty (~5%) Red Box : systematic uncertainty (~20%) Hatched : discrepancy between datasets (~12%) preliminary No bump structure was observed!  upper limit of cross section   n search region: Mass = 2.22 - 2.36 GeV/c 2 B.E. = 150 - 10 MeV acceptance was corrected with Monte-Carlo simulation expected signal

11 Upper Limits of differential cross section 2013/2/13 GCOE Symposium @ Kyoto University10 / 11 preliminary -  = 20 MeV 0.05 - 0.25  b -  = 60 MeV 0.15 - 0.6  b -  =100 MeV 0.15 - 0.7  b a few % of typical hadron production cross section.  N   K  b   N   K  b  B.E.  15 points (10-150 MeV)   3 points upper limits of cross section were determined log likelihood ratio method

12 Conclusion and future prospect The existence of Kaonic nuclei is not established. K - pp was searched for using  D  K +  - X reaction No bump structures were found, and the upper limits of differential cross section were determined to be a few % of typical hadron production cross section. Future prospect detect the decay products from K - pp.  increase S/N search for other charge states using  D  K + K - pn,  D  K +  + K-nn 2013/2/13 GCOE Symposium @ Kyoto University11 / 11

13 Collaborators 2013/2/13 GCOE Symposium @ Kyoto University12 / 15

14 Appendix 2013/2/13 GCOE Symposium @ Kyoto University13 / 15

15 Appendix Merit deuteron  small nuclear effect(FSI). additional  - emission reduce the momentum transfer. K can be exchanged. polarization observable is available. Demerit small cross section (~nbarn). many background source limited information on hadron resonance. necessary to detect the decay product. 2013/2/13 GCOE Symposium @ Kyoto University14 / 15

16 Calculation of Upper Limits 2013/2/13 GCOE Symposium @ Kyoto University15 / 15 preliminary Upper Limit was calculated with log Likelihood ratio method Background proces  p  K +  -   p  K +  -   p  K +  -  (1385)  p  K +  -  (1385)-  p  K +  -  constant offset Signal Breit Wigner distribution -2  lnL = 3.841  upper limit (95% C.L.) Signal Yield

17 Theoretical calculation 2013/2/13 GCOE Symposium @ Kyoto University16 / 15 Binding EnergyDecay Width Method Yamazaki and Akaishi48 MeV61 MeVPhenomenological Variatioal Method Dote, Hyodo and Weise20±3 MeV40-70 MeVChiral SU(3) Variational Method Ikeda and Sato60 – 95 MeV45 - 80 MeVChiral SU(3) Fadeev Calculation Shevchenko, Gal and Mares 50 – 70 MeV90 – 110 MeVPhenomenological Fadeev Calculation S. Wycech and A. M. Green 56.5~78 MeV39~60 MeV Uchino, Hyodo and Oka depend on  * N Variational Method All calculations predict that K - pp can exist!! However… B.E. = 20 – 100 MeV  = 40 – 110 MeV Depending on the K N interaction model and Calculation Method.

18 Background processes 2013/2/13 GCOE Symposium @ Kyoto University17 / 15 preliminary 15 quasi- free processes were considered for fitting.  N  Y K+ Y K+  - Y* K+  - Y K+  -  The main background (~20 %)  n  K +  (1520)      N  K +  - X MM(K + ) MM(K +,  - ) MM(K + ) MM(K +,  - )   /ndf ~ 1.3 Y hyperon (  ) Y* hyperon resonance (  …)


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