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Meson Properties at Finite Density from Meson-Nucleus Systems

This paper discusses the meson properties in meson-nucleus systems at finite density, particularly focusing on the eta meson. The study uses the NJL model with the Kobayashi-Maskawa term and explores the formation of eta-4He through the d + d reaction. The strong coupling between the eta meson and the N*(1535) resonance is also investigated.

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Meson Properties at Finite Density from Meson-Nucleus Systems

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  1. Meson Properties at Finite Density from Meson Nucleus Systems Satoru Hirenzaki (Nara Womens University, Japan) 10 June 2015 * eta by d+d * Comments on phi data

  2. Basic Motivation Symmetry Breaking Pattern and Meson Properties h’ h p … cf.) NJL model with KMT Schematic View of the PS meson mass spectrum Jido et al., PRC85(12)032201(R) Nagahiro et al., PRC (2013) 1000 800 UA(1) breaking (KMT term[1,2]) 600 UA(1)anomaly effect Meson mass [MeV] 400 200 massless [1] Kobayashi-Maskawa PTP44(70)1422 [2] G. ’t Hooft, PRD14(76)3432 ChS manifest dynamically broken dyn. & explicitly broken Costa et al.,PLB560(03)171, Nagahiro-Takizawa-Hirenzaki, PRC74(06)045203 

  3. Formation of η-4He by d + d reaction at COSY with H. Nagahiro (Nara Women’s Univ.) N. Ikeno (Tottori Univ.) D. Jido (Tokyo Metropolitan Univ)

  4. hNN* system -No I=3/2 baryon contamination -Large coupling constant -no suppression at threshold (s-wave coupling) Doorway to N*(1535) eta-Nucleus system h-mesic nuclei properties of eta meson h meson h-N system • Strong Coupling to N*(1535), Motivation and our aim • h-N system … strongly couples to the N*(1535) resonance • h-mesic nuculei … doorway to in-medium N*(1535) • N*(1535) … a candidate of the chiral partner of nucleon • chiral symmetry for baryons ?

  5. h-mesic nuclei Many works for h mesic nuclei from 1980’s • Theor. Liu, Haider, PRC34(1986)1845 Kohno, Tanabe, PLB231(1989)219; NPA519(1990)755 Garcia-Recio, Nieves, Inoue, Oset PLB550(02)47 C. Wilkin, T. Ueda, S. Wycech, …… • Exp. Chrien et al., PRL60(1988)2595 TAPS@MAMI (g + 3He  p0 + p + X) COSY-GEM (p + Al  3He + Mg-h) WASA-at-COSY (d + d  3He + p + p) JPARC (Itahashi, Fujioka…), …… Our works for eta-mesic nuclei • R.S. Hayano, S. Hirenzaki, A. Gillitzer, Eur. Phys. J. (99) • D.Jido, H.Nagahiro and S.Hirenzaki, Phys.Rev.C66, 045202, 2002. • H.Nagahiro, D.Jido, S.Hirenzaki, Phys.Rev.C68, 035205, 2003. • H.Nagahiro, D.Jido and S.Hirenzaki, Nucl.Phys.A761,92, 2005. • D.Jido, E.E.Kolomeitsev, H.Nagahiro, S.Hirenzaki, Nucl.Phys.A811:158, 2008. • H.Nagahiro, D.Jido, S.Hirenzaki, Phys.Rev.C80,025205, 2009.

  6. A Theoretical Calculation for (discussions with P.Moskal, W. Krzemien, M. Skurzok) Some remarks • Momentum transfer ------- Large pd = 1.025 GeV/c, pa = ph= 0 at threshold in C.M. • Data of d d 4He h above threshold • Simple spectral structure is expected for light systems • It’s a few body system (2N+2N  4N + eta), but the momentum transfer is large. • NO SPECTATOR! All 4N participate to the formation reaction seriously for ‘the signal process’. • Results of experiments: • exclusive analysis for the final states, charge channels,,,

  7. A Theoretical Calculation for Some remarks • Transition (h-production) part h High q transfer at each propagator Parameterize this part.

  8. A Theoretical Calculation for Schematic picture d h Green function method a d with h-a optical potential s total s s(dd4Heh) data escape conversion Etot Etot threshold threshold

  9. Green’s function method Ref. O.Morimatsu and K. Yazaki, NPA435(1985)727-737  

  10. h d F(q) a d Scattering Amplitude F(q) ( f (r) : r-space representation)… Assumed to be Gaussian

  11. A Theoretical Calculation for 3 parameters in this model • h-a optical potential • (used to calculate the eta Green’s function • V0, W0 • Potential Strength • at nuclear center • h production part dd 4Heh • F should include the information on • Deuterons and alpha particle structure and their overlap (fusion) • Nucleon - nucleon interaction for eta meson production • for high momentum transfer region.

  12. A Theoretical Calculation for Exp. Data of dd4Heh Fig. taken from NFQCD10@YITP, 2010 slide by S. Schadmand R.Frascaria et al., Rhys.Rev.C50 (1994) 573, N. Wills et al., Phys. Lett. B 406 (1997) 14, A.Wronska et al., Eur. Phys. J. A 26, 421-428 (2005). This part can be compared with the escape part of Green’s function calculation. s s(dd4Heh) data • Some restrictions • to the model parameters. Etot threshold

  13. Numerical Results (Ideal case) 8 stot [nb] 25 20 7 15 10 5 0 6 5 (V0,W0) = (−100, −10) MeV p0 = 500 MeV/c Arbitrary unit 4 3 2 1 0 −20 −15 −10 −5 0 5 10 15 Eh − mh [MeV]

  14. ~ ~ ~ ~ Numerical Results (Larger imaginary part ) 6 stot [nb] 25 5 20 15 10 5 4 0 Arbitrary unit (V0,W0) = (−100, −20) MeV p0 = 500 MeV/c 3 2 0 −20 −15 −10 −5 0 5 10 15 Eh − mh [MeV]

  15. ~ ~ ~ ~ Numerical Results (Larger imaginary part ) 12 stot [nb] 25 20 11 15 10 5 0 (V0,W0) = (−100, −40) MeV p0 = 500 MeV/c 10 Arbitrary unit 9 8 0 −20 −15 −10 −5 0 5 10 15 Eh − mh [MeV]

  16. (V0 = -100 MeV) (W0= -5, -10, -20, -40 MeV) (p0 =500 MeV/c)

  17. (V0 = -100 MeV) (W0= -5, -10, -20 MeV) (p0 =1000 MeV/c)

  18. (V0 = -100, -50, -30 MeV) (W0= -20 MeV) (p0 =500 MeV/c)

  19. (V0 = -100, -50 MeV) (W0= -20 MeV) (p0 =1000 MeV/c)

  20. (V0 = -100 MeV) (W0= -10 MeV) (p0 =1000, 500, 400 MeV/c)

  21. (V0 = -100 MeV) (W0= -20 MeV) (p0 =1000, 500 MeV/c)

  22. In these cases, eta production data above threshold can not be reproduced. (V0 = -50 MeV) (W0= -5 MeV) (p0 =1000, 500 MeV/c)

  23. Summary for d+d reaction ★ Formation of h mesic nucleus • d + d  (4He-h )  X (several channels) reaction • High momentum transfer (~1GeV/c) • h production data above threshold exist • Simple spectra are expected ★ A model calculation with Green’s function • It may provide an estimation and interpretation of the inclusive experimental data. • But for the comparison, backgrounds • from non-(eta + alpha) processes must be removed • (quasi-elastic pion production etc).

  24. Summary for d+d reaction ★ Further studies = Better form for transition part = Exclusive treatment of the final particles * Evaluation of ImV for each channel * Implementation of the realistic meson self-energy * Independent treatment of the eta-alpha decay process could be fine (decay model different from formation part)

  25. Vector mesons in nucleus = Transparency ratio and Invariant mass = with S. Tokunaga (Nara Women’s Univ.) J. Yamagata-Sekihara (Oshima National College of Maritime Technology) H. Nagahiro (Nara Women’s Univ.)

  26. Summary Table -- Results by independent groups Mass shift: 3.4% Mass shift: no mention

  27. meson • Isolated peak structure • Long life time • (selection of slow particle)

  28. We consider here. • DATA by KEK E325, LEPS/SPring8, JPARC E16 • R. Muto et al., Phys. Rev. Lett. 98 (2007) 042501 • T. Ishikawa et al., Phys. Lett. B 608 (2005) 215-222 • T. Sawada, Doctor Thesis, Osaka University (2013) • Thoretical works from Hatsuda and Lee, importance and sensitivity to • S quark condensate.

  29. Motivation / Interests * Determine the <N|sbar s|N> from in-medium * Importance of <N|sbar s|N> = How much is the strangeness component in nucleon (important for hadron structure studies.) = <N|sbar s|N> basic quantity for nuclear matter, which relate to various phenomena (KN sigma term => kaon condensattion in neutron star, etc ) = <N|sbar s|N> may complete SU(3) info. on condesates with SU(2) part info. by other data

  30. * First of all, we need ‘Stable (consistent) interpretation of data’ * Then, we should check ‘How reliable is theoretical connection between in-medium phi property and condensate ? ’ * Mass shift is not mandatory. If, it is zero, it’s important to confirm how accurately 0.

  31. Mass shift: 3.4% Mass shift: no mention

  32. Goal for the first step • Describe ‘Transparency ratio (LEPS/SPring8)’ • and ‘Invariant Mass (KEK E325)’ in an unified manner. • * Find the consistent interpretation of the observables. • And deepen the understanding between observables • and meson propertes.

  33. Formula of the transparency ratio -T. Ishikawa et al., Phys. Lett. B 608 (2005) 215-222-T. Sawada, Doctor Thesis, Osaka University (2013) Transparency ratio A : mass number : incident photon number : Flux loss of the incident photon : Flux loss of phi : path of the phi : phi momentum

  34. 3, Transparency Ratio–計算結果– Calculated Results

  35. Formula for Invariant Mass • Unified treatment with Transparency  → Calcualte Invariant mass dist. by the same model parameters as the Transparency Decay phi number : Produced phi at (b, z0) : Number of phi at (b, z) : Num of Incident particles : Branching Ratio of phi in vacuum,

  36. An Example Production at origin φの生成位置 入射粒子 (φの飛距離) density Distance from production point

  37. Phi meson decay number per unit length Phi meson decay number to e+e- channel

  38. Target case Distance from production point

  39. Target case Target case density Distance from production point

  40. Target case Target case density Distance from production point Nuclear center Nuclear surface/ Outside

  41. Phi meson decay number per unit length Phi meson decay number to e+e- channel Invariant mass distribution seen in e+e- decay channel phi production point phi mass in vacuum Full width in vacuum : φ中間子の生成位置 Parameter for mass shift C : φ中間子の質量変化の大きさを決めるパラメータ

  42. Numerical Results – Invariant Mass of e+e- pair • Input data γ-distortion: proton-distortion:

  43. proton-induced, target: , βγ=1.0 (KEK E325) Experimental energy resolution (~10.7MeV) is not taken into account.

  44. proton-induced, target: , βγ=1.0 (KEK E325) Experimental energy resolution (~10.7MeV) is not taken into account.

  45. proton-induced, target: , βγ=1.0 (KEK E325) Experimental energy resolution (~10.7MeV) is not taken into account.

  46. proton-induced, target: , βγ=1.0 (KEK E325) Experimental energy resolution (~10.7MeV) is not taken into account.

  47. proton-induced, target: , βγ=1.0 (KEK E325) Experimental energy resolution (~10.7MeV) is not taken into account.

  48. γ-induced • , target: ,βγ=1.0

  49. Larger initial distortion  Larger contribution of in-medium decay at forward directions. ( Meson is produced at early stage in Nucleus. ) Angular dependence of the mass shift contribution can be interesting (But large distortion of initial particles may break the target seriously before meson production.)

  50. proton-induced, target: , βγ=0.5 (J-PARC E16) (Slow phi in large Nucleus) Simulation By S. Yokkaichi (Resolution 5 MeV)

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