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Pions in nuclei and tensor force

Pions in nuclei and tensor force. Hiroshi Toki (RCNP, Osaka) in collaboration with Yoko Ogawa (RCNP, Osaka) Jinniu Hu (RCNP, Osaka) Takayuki Myo (Osaka Inst. Tech.) Kiyomi Ikeda (RIKEN). Pion is important !! In Nuclear Physics.

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Pions in nuclei and tensor force

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  1. Pions in nuclei and tensor force Hiroshi Toki (RCNP, Osaka) in collaboration with Yoko Ogawa (RCNP, Osaka) Jinniu Hu (RCNP, Osaka) Takayuki Myo (Osaka Inst. Tech.) Kiyomi Ikeda (RIKEN) toki@yukawa.kyoto

  2. Pion is important !!In Nuclear Physics • Yukawa introduced pion as mediator of nuclear interaction for nuclei. (1934) • Nuclear Physics started by shell model with strong spin-orbit interaction. (1949: Meyer-Jensen: Phenomenological) • The pion had not played the central role in nuclear physics until recent years. toki@yukawa.kyoto

  3. Variational calculation of light nuclei with NN interaction VMC+GFMC VNNN Fujita-Miyazawa C. Pieper and R. B. Wiringa, Annu. Rev. Nucl. Part. Sci.51(2001) Relativistic We want to calculate heavy nuclei!! toki@yukawa.kyoto Pion is a key element

  4. Giant GT Not simple RCNP experiment (good resolution) Y. Fujita et al., E.Phys.J A13 (2002) 411 H. Fujita et al., PRC toki@yukawa.kyoto

  5. The pion (tensor) is important. S=1 and L=0 or 2 NN interaction Deuteron (1+) toki@yukawa.kyoto

  6. Deuteron and tensor interaction Pion Tensor spin-spin • Central interaction has strong repulsion. • Tensor interaction is strong in 3S1 channel. • S-wave function has a dip. • D-wave component is only 6%. • Tensor attraction provides 80% of entire attraction. • D-wave is spatially shrank by a half. toki@yukawa.kyoto

  7. Chiral symmetry (Nambu:1960) • Chiral symmetry is the key symmetry to connect real world with QCD physics • Chiral model is very powerful in generating various hadronic states • Nucleon gets mass dynamically • Pion is the Nambu-Goldstone particle of the chiral symmetry breaking toki@yukawa.kyoto

  8. Nobel prize (2008) He was motivated by the BCS theory(1958). is the order parameter is the order parameter Chiral symmetry Particle number toki@yukawa.kyoto

  9. Nambu-Jona-Lasinio Lagrangian Chiral transformation Mean field approximation; Hartree approximation Fermion gets mass. The chiral symmetry is spontaneously broken. Pion appears as a Nambu-Goldstone boson. toki@yukawa.kyoto

  10. Chiral sigma model Y. Ogawa et al. PTP (2004) Pion is the Nambu boson of chiral symmetry Linear Sigma Model Lagrangian Polar coordinate Weinberg transformation toki@yukawa.kyoto

  11. where M = gsfp M* = M + gsj mp2 = m2 + l fp ms2 = m2 +3 l fp ~ ~ mw = gwfp mw* =mw + gwj Non-linear sigma model N r = fp + j Lagrangian Free parameters are and (Two parameters) toki@yukawa.kyoto

  12. Relativistic Chiral Mean Field Model Wave function for mesons and nucleons p p Mean field approximation for mesons. h h Nucleons are moving in the mean field and occasionally brought up to high momentum states due to pion exchange interaction Bruekner argument toki@yukawa.kyoto

  13. Relativistic Brueckner-Hartree-Fock theory Brockmann-Machleidt (1990) RBHF relativity Non-RBHF Us~ -400MeV Uv~ 350MeV toki@yukawa.kyoto RBHF theory provides a theoretical foundation of RMF model.

  14. Density dependent RMF model Brockmann Toki PRL(1992) toki@yukawa.kyoto

  15. Why 2p-2h states are necessary for the tensor interaction? The spin flipped states are already occupied by other nucleons. Pauli forbidden G.S. Spin-saturated toki@yukawa.kyoto

  16. Energy minimization with respect to meson and nucleon fields (Mean field equation) toki@yukawa.kyoto

  17. Energy Energy minimization toki@yukawa.kyoto

  18. RCMF equation toki@yukawa.kyoto

  19. Energy minimization with respect to meson and nucleon fields (Mean field equation) (Corrrelation function) toki@yukawa.kyoto

  20. Unitary Correlation Operator Method (UCOM) short-range correlator Bare Hamiltonian Shift operator depending on the relative distance r H. Feldmeier, T. Neff, R. Roth, J. Schnack, NPA632(1998)61 toki@yukawa.kyoto

  21. Short-range correlator : C Hamiltonian in UCOM 2-body approximation in the cluster expansion of operator toki@yukawa.kyoto

  22. Ogawa Toki NP 2009 Numerical results (1) 4He 12C 16O Adjust binding energy and size. toki@yukawa.kyoto

  23. Numerical results 2 O The difference between 12C and 16O is 3MeV/N. P1/2 C The difference comes from low pion spin states (J<3). This is the Pauli blocking effect. P3/2 S1/2 Pion tensor provides large attraction to 12C Pion energy toki@yukawa.kyoto

  24. Ogawa Toki NP(2009) Chiral symmetry Nucleon mass is reduced by 20% due to sigma. N Not 45% We want to work out heavier nuclei for magic number. Spin-orbit splitting should be worked out systematically. toki@yukawa.kyoto

  25. Hu Ogawa Toki Phys. Rev. 2009 Nuclear matter E/A Total Pion toki@yukawa.kyoto

  26. Deeply bound pionic atom Predicted to exist Toki Yamazaki, PL(1988) Found by (d,3He) @ GSI Itahashi, Hayano, Yamazaki.. Z. Phys.(1996), PRL(2004) Findings: isovector s-wave toki@yukawa.kyoto

  27. Halo structure in 11Li Myo Kato Toki Ikeda PRC(2008) Deuteron wave function Deuteron-like state is made by 2p-2h states in shell model. toki@yukawa.kyoto

  28. Tensor interaction Tensor interaction needs 2p-2h excitation of pn pair. P1/2 orbit is used for this Excitation. This orbit is blocked When we want to put two neutrons. S1/2 orbit is free of this. toki@yukawa.kyoto

  29. Conclusion • Pion (tensor) is treated within relativistic chiral mean field model. • We extended RBHF theory for finite nuclei. • Nucleon mass is reduced by 20% • Chiral condensate is similar to the model independent value. (Sigma term~50MeV) • Deeply bound pionic atom seems to verify partial recovery of chiral symmetry. toki@yukawa.kyoto

  30. Picture of nucleus proton Snapshot neutron pionic pair toki@yukawa.kyoto

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