Relativistic chiral mean field model for nuclear physics (II) Hiroshi Toki Research Center for Nuclear Physics Osaka University.

Slides:



Advertisements
Similar presentations
HL-3 May 2006Kernfysica: quarks, nucleonen en kernen1 Outline lecture (HL-3) Structure of nuclei NN potential exchange force Terra incognita in nuclear.
Advertisements

Delta-hole effects on the shell evolution of neutron-rich exotic nuclei Takaharu Otsuka University of Tokyo / RIKEN / MSU Chiral07 Osaka November 12 -
Denis Parganlija (Frankfurt U.) Meson 2010 Workshop, Kraków - Poland Structure of Scalar Mesons f 0 (600), a 0 (980), f 0 (1370) and a 0 (1450) Denis Parganlija.
Chiral freedom and the scale of weak interactions.
Chiral symmetry breaking and structure of quark droplets
Finite Nuclei and Nuclear Matter in Relativistic Hartree-Fock Approach Long Wenhui 1,2, Nguyen Van Giai 2, Meng Jie 1 1 School of Physics, Peking University,
1 A Model Study on Meson Spectrum and Chiral Symmetry Transition Da
1 Chiral Symmetry Breaking and Restoration in QCD Da Huang Institute of Theoretical Physics, Chinese Academy of
Naoki Yamamoto (Univ. of Tokyo) Tetsuo Hatsuda (Univ. of Tokyo) Motoi Tachibana (Saga Univ.) Gordon Baym (Univ. of Illinois) Phys. Rev. Lett. 97 (2006)
1 Nuclear Binding and QCD ( with G. Chanfray) Magda Ericson, IPNL, Lyon SCADRON70 Lisbon February 2008.
Chiral freedom and the scale of weak interactions.
QCD – from the vacuum to high temperature an analytical approach an analytical approach.
Chiral freedom and the scale of weak interactions.
Modern Physics LECTURE II.
1 Debye screened QGP QCD : confined Chiral Condensate Quark Potential Deconfinement and Chiral Symmetry restoration expected within QCD mm symmetryChiral.
Joint Lecture Groningen-Osaka
Masayasu Harada (Nagoya Univ.) based on M.H., M.Rho and C.Sasaki, Phys. Rev. D 70, (2004) M.H., Work in progress at “Heavy Quark Physics in QCD”
Isospin effect in asymmetric nuclear matter (with QHD II model) Kie sang JEONG.
Charm hadrons in nuclear medium S. Yasui (KEK) K. Sudoh (Nishogakusha Univ.) “Hadron in nucleus” 31 Nov. – 2 Dec arXiv:1308:0098 [hep-ph]
Sigma model and applications 1. The linear sigma model (& NJL model) 2. Chiral perturbation 3. Applications.
「第5回 J-PARC における高エネルギーハドロン物理」 J-PARC に活きる南部先生のアイデア 1.Introdution 2.Stability of hadronic matter 3. Chiral symmetry in vacuum & in medium 4. No summary.
The first systematic study of the ground-state properties of finite nuclei in the relativistic mean field model Lisheng Geng Research Center for Nuclear.
Mass modification of heavy-light mesons in spin-isospin correlated matter Masayasu Harada (Nagoya Univ.) at Mini workshop on “Structure and production.
LBL 5/21/2007J.W. Holt1 Medium-modified NN interactions Jeremy W. Holt* Nuclear Theory Group State University of New York * with G.E. Brown, J.D. Holt,
Pengfei Zhuang Physics Department, Tsinghua University, Beijing
Exotic Nuclei in Relativistic and Non-Relativistic Models Exotic Nuclei large isospin asymmetry - nuclei close to the drip lines - superheavy nuclei non-relativistic.
0 Yoko Ogawa (RCNP/Osaka) Hiroshi Toki (RCNP/Osaka) Setsuo Tamenaga (RCNP/Osaka) Hong Shen (Nankai/China) Atsushi Hosaka (RCNP/Osaka) Satoru Sugimoto (RIKEN)
Chiral condensate in nuclear matter beyond linear density using chiral Ward identity S.Goda (Kyoto Univ.) D.Jido ( YITP ) 12th International Workshop on.
Eigo Shintani (KEK) (JLQCD Collaboration) KEKPH0712, Dec. 12, 2007.
Scalar response of the nucleon, Chiral symmetry and nuclear matter properties G. Chanfray, IPN Lyon, IN2P3/CNRS, Université Lyon 1 M. Ericson, IPN Lyon,
Relativistic mean field and RPA with negative energy states for finite nuclei Akihiro Haga, Hiroshi Toki, Setsuo Tamenaga, Yoko Ogawa, Research Center.
Extended Brueckner-Hartree-Fock theory in many body system - Importance of pion in nuclei - Hiroshi Toki (RCNP, KEK) In collaboration.
CPOD2011 , Wuhan, China 1 Isospin Matter Pengfei Zhuang Tsinghua University, Beijing ● Phase Diagram at finite μ I ● BCS-BEC Crossover in pion superfluid.
Chiral symmetry breaking and low energy effective nuclear Lagrangian Eduardo A. Coello Perez.
NEW TRENDS IN HIGH-ENERGY PHYSICS (experiment, phenomenology, theory) Alushta, Crimea, Ukraine, September 23-29, 2013 Effects of the next-to-leading order.
July 29-30, 2010, Dresden 1 Forbidden Beta Transitions in Neutrinoless Double Beta Decay Kazuo Muto Department of Physics, Tokyo Institute of Technology.
Furong Xu (许甫荣) Many-body calculations with realistic and phenomenological nuclear forces Outline I. Nuclear forces II. N 3 LO (LQCD): MBPT, BHF, GSM (resonance.
Time Dependent Quark Masses and Big Bang Nucleosynthesis Myung-Ki Cheoun, G. Mathews, T. Kajino, M. Kusagabe Soongsil University, Korea Asian Pacific Few.
Denis Parganlija (Frankfurt U.) Excited QCD 2010, Tatranska Lomnica/Slovakia Nature of Light Scalar Mesons f 0 (600), a 0 (980), f 0 (1370) and a 0 (1450)
And Mesons in Strange Hadronic Medium at Finite Temperature and Density Rahul Chhabra (Ph.D student) Department Of Physics NIT Jalandhar India In cooperation.
Helmholtz International Summer School, Dubna, 24 July 2008 Pion decay constant in Dense Skyrmion Matter Hee-Jung Lee ( Chungbuk Nat’l Univ.) Collaborators.
Furong Xu (许甫荣) Nuclear forces and applications to nuclear structure calculations Outline I. Nuclear forces II. N 3 LO (LQCD): MBPT, BHF, GSM (resonance.
1 11/20/13 21/11/2015 Jinniu Hu School of Physics, Nankai University Workshop on “Chiral forces and ab initio calculations” Nov. 20- Nov. 22,
Water ( H 2 O ) oxygen atom ( O ) proton ( p ) electrons ( e ) neutron ( n ) 3 quarks What the matters are made out of ? 3 quarks
1 Keitaro Nagata and Atsushi Hosaka Research Center for Nuclear Physics, Osaka Univ. Quark-Diquark approach for the nucleon and Roper resonance Workshop.
Beijing, QNP091 Matthias F.M. Lutz (GSI) and Madeleine Soyeur (Saclay) Irfu/SPhN CEA/ Saclay Irfu/SPhN CEA/ Saclay Dynamics of strong and radiative decays.
Denis Parganlija (Vienna UT) Mesons in non-perturbative and perturbative regions of QCD Mesons in non-perturbative and perturbative regions of QCD Denis.
Possible hadron physics To be done With use of unstable nuclei Teiji Kunihiro (Kyoto U.) Yonsei University, Korea.
1 NJL model at finite temperature and chemical potential in dimensional regularization T. Fujihara, T. Inagaki, D. Kimura : Hiroshima Univ.. Alexander.
Denis Parganlija (Frankfurt U.) Finite-Temperature QCD Workshop, IST Lisbon Non-Strange and Strange Scalar Quarkonia Denis Parganlija In collaboration.
Accurate vacuum correction in finite nuclei A. Haga 1, H. Toki 1, S. Tamenaga 1, and Y. Horikawa 2 1.RCNP, Osaka Univ. 2.Juntendo Univ.
Su Houng Lee 1. Few words on a recent sum rule result 2. A simple constituent quark model for D meson 3. Consequences 4. Summary D meson in nuclear medium:
Tensor interaction in Extended Brueckner-Hartree-Fock theory Hiroshi Toki (RCNP, Osaka) In collaboration with Yoko Ogawa.
The role of isospin symmetry in medium-mass N ~ Z nuclei
Tensor optimized shell model and role of pion in finite nuclei
Nuclear Symmetry Energy in QCD degree of freedom Phys. Rev
mesons as probes to explore the chiral symmetry in nuclear matter
Role of Pions in Nuclei and Experimental Characteristics
Relativistic Chiral Mean Field Model for Finite Nuclei
Aspects of the QCD phase diagram
Relativistic mean field theory and chiral symmetry for finite nuclei
Color Superconductivity in dense quark matter
Relativistic extended chiral mean field model for finite nuclei
The Structure of Nuclear force in a chiral quark-diquark model
Effective Theory for Mesons
Deeply Bound Mesonic States -Case of Kaon-
Pions in nuclei and tensor force
A possible approach to the CEP location
Institute of Modern Physics Chinese Academy of Sciences
Theory on Hadrons in nuclear medium
Presentation transcript:

Relativistic chiral mean field model for nuclear physics (II) Hiroshi Toki Research Center for Nuclear Physics Osaka University

Pion is important !! Yukawa introduced pion as a mediator of nuclear interaction (1934) Meyer-Jensen introduced shell model for finite nuclei (1949) Nambu-Jona-Lasinio introduced chiral symmetry and its breaking for mass and pion generation (1961)

Motivation for the second stage Pion is important in nuclear physics. Pion appears due to chiral symmetry. Particles as nucleon, rho mesons,.. may change their properties in medium. Chiral symmetry may be recovered partially in nucleus. Unification of QCD physics and nuclear physics.

Spontaneous breaking of chiral symmetry Quarks & gluons Hadrons & nuclei Confinement, Mass generation Potential energy surface of the vacuum Chiral order parameter Yoichiro Nambu Hosaka

He was motivated by the BCS theory. Nobel prize (2008) is the order parameter Particle number Chiral symmetry

Nambu-Jona-Lasinio Lagrangian Mean field approximation; Hartree approximation Fermion gets mass. The chiral symmetry is spontaneously broken. Chiral transformation

Chiral condensate is The fermion mass is The mass is similar to the pairing gap in the BCS formalism. The mass generation mechanism for a fermion. m G GcGc

The particle-hole excitation (pion channel): RPA T = K + T K J(q)

The pion mass is zero. Nambu-Goldstone mode has a zero mass. The nucleon gets mass by chiral condensation. There appears a massless boson; pseudo-scalar meson. All the masses of particles are zero at the beginning, but they are generated dynamically. Massless boson appears (Nambu-Goldstone boson) with pseudo-scalar quantum number.

Bosonization (Eguchi:1974) Fermion field is quark Auxiliary fields

Nuclear physics with NJL model Auxiliary fields SU2 chiral transformation Confinement (Polyakov NJL Mode) SU2 c is done SU3 c is not yet done.

Chiral sigma model Linear Sigma Model Lagrangian Polar coordinate Weinberg transformation Pion is the Nambu boson of chiral symmetry

Non-linear sigma model Lagrangian  = f  +  where M = g  f  M* = M + g   m  2 =  2 + f  m  2 =  2 +3 f  m  = g  f  m   =  m  + g   ~~ Free parameters are and (Two parameters) N

Relativistic mean field model (standard) Mean field approximation: Then take only the mean field part, which is just a number. The pion mean field is zero. Hence, the pion contribution is zero in the standard mean field approximation.

Relativistic mean field model (pion condensation) Ogawa, Toki, et al. Brown, Migdal.. Since the pion has pseudo-scalar (0 - ) nature, the parity and charge symmetry are broken. In finite nuclei, we have to project out spin and isospin, which involves a complicated projection. Dirac equation

Mean field approximation for mesons. Nucleons are moving in the mean field and occasionally brought up to high momentum states due to pion exchange interaction h h p p Brueckner argument Relativistic Chiral Mean Field Model (powerful method) Wave function for mesons and nucleons

Why 2p-2h states are necessary for pion (tensor) interaction? G.S. Spin-saturated The spin flipped states are already occupied by other nucleons. Pauli forbidden

Energy minimization with respect to meson and nucleon fields (Mean field equation) Hartree-Fock G-matrix component

Numerical results (1) 4 He 12 C 16 O Ogawa Toki NP 2009 Adjust binding energy and size Tensor Spin-spin Pion Total 12 C

Numerical results 2 The difference between 12 C and 16 O is 3 MeV/N. The difference comes from low pion spin states (J<3). This is the Pauli blocking effect. P 3/2 P 1/2 C O S 1/2 Pion energy Pion tensor provides large attraction to 12 C O C Cumulative Individual contribution

Chiral symmetry Nucleon mass is reduced by 20% due to sigma. We want to work out heavier nuclei for magic number. Spin-orbit splitting should be worked out systematically. Ogawa Toki NP(2009) Not 45% as discussed in RMF model. N One half is from sigma meson and the other half is from the pion.

Nuclear matter Hu Ogawa Toki Phys. Rev E/A Total Pion Total

Deeply bound pionic atom Toki Yamazaki, PL(1988) Predicted to exist Found by GSI Itahashi, Hayano, Yamazaki.. Z. Phys.(1996), PRL(2004) Findings: isovector s-wave

Suzuki, Hayano, Yamazaki.. PRL(2004) Optical model analysis for the deeply bound state.

Summary-2 NJL model provides the linear sigma model. Pion (tensor) is treated within the relativistic chiral mean field model. JJ-magic is produced by pion. Nucleon mass is reduced by 20% Deeply bound pionic atom seems to verify partial recovery of chiral symmetry.

Summary Pion is important in Nuclear Physics. Pion is a Goldstone-Nambu boson of chiral symmetry breaking. By integrating out the quark field with confinement, we can get sigma model Lagrangian. Relativistic chiral mean field model is able to work out the sigma model Lagrangian. We have now a tool to unify the quark picture with the hadron picture and describe nucleus from quarks.

Joint Lecture Groningen-Osaka Spontaneous Breaking of Chiral Symmetry in Hadron Physics 30 Sep 09:00- CEST/16:00- JST Atsushi HOSAKA 07 Oct 09:00- CEST/16:00- JST Nuclear Structure 21 Oct 09:00- CEST/16:00- JST Nasser KALANTAR-NAYESTANAKI 28 Oct 09:00- CET/17:00- JST Low-energy tests of the Standard Model 25 Nov 09:00- CET/17:00- JST Rob TIMMERMANS 02 Dec 09:00- CET/17:00- JST Relativistic chiral mean field model description of finite nuclei 09 Dec 09:00- CET/17:00- JST Hiroshi TOKI 16 Dec 09:00- CET/17:00- JST + WRAP-UP/DISCUSSION