Quark-model baryon-baryon interactions and their applications to few-body systems Y. Fujiwara (Kyoto) Y. Suzuki (Niigata) C. Nakamoto (Suzuka) M. Kohno(Kyushu Dental) K. Miyagawa(Okayama) 1. Introduction 2. B8 B8 interactions fss2 and FSS: spin-flavor SU6 symmetry 3. B8 interactions by quark-model G-matrix 4. Some applications 4.1. N interaction and 3H Faddeev calculation 4.2 effective potential and 9Be Faddeev calculation 4.3. s. p. potential and , (3N) potentials 4.4. N total cross sections and potential 5. Summary 2006.10.13 HYP2006 Mainz Oka – Yazaki (1980) B8B8 interactions by fss2 Phys. Rev. C64 (2001) 054001 Phys. Rev. C65 (2002) 014001 A natural and accurate description of NN, YN, YY interactions in terms of (3q)-(3q) RGM • Short-range repulsion and LS by quarks • Medium-attraction and long-rang tensor by S, PS and V meson exchange potentials (fss2) (Cf. FSS without V) Phys. Rev. C54 (1996) 2180 Model Hamiltonian H =∑ 6i=1 (mi+pi2/2mi) +∑ 6i<j (UijConf+UijFB+∑βUijSβ +∑βUijPSβ + ∑βUijVβ) f(3q)f(3q)|E-H|A {f(3q)f(3q)c(r)}=0 QMPACK homepage PPNP in press http://qmpack.homelinux.com/~qmpack/index.php 2006.10.13 HYP2006 Mainz Arndt : SAID Nijmegen : NN-OnLine Lippmann-Schwinger (LS) RGM P.T.P. 103 (2000) 755 Solve [ - H0 - VRGM() ] c=0 with VRGM()=VD+G+ K in the mom. representation ( = E - Eint ) Born kernel qf|VRGM() |qi T-matrix, G-matrix 1) non-local 2) energy-dependent 3) Pauli-forbidden states in N - N (I=1/2), - N - (I=0), - (I=1/2) 1S0 : i.e. SU3 (11)s : Ku=u 3-cluster Faddeev formalism using VRGM() G 0 ( E )T ( E h , )( ) u | P u | 0 self-consistency equation for P | h V RGM P.T.P. 107 (2002) 745; 993 ( ) | P B8 interaction by quark-model G-matrix : “(0s)4” G (p, p’; K, , kF) k’=p’- p , q’=(p+p’)/2 G (k’, q’; q1, q’) k=k’ - cluster folding q1=q for direct and knock-on V (k, q) B8 relative q’ incident q1 =0.257 fm-2 in total c. m. kF=1.35 fm-1 VW (R, q) : Wigner transform k=pf - pi , q=(pf+pi)/2 V (pf , pi) U(R)=VW(R, (h2/2)(E-U(R)) Lippmann - Schwinger equation exact EB , (E) 2006.10.13 HYP2006 Mainz Transcendental equation Schrödinger equation EBW , W(E) “constant K , , kF” n RGM by G-matrix of fss2 n sactt. phase shift S1/2 P3/2 P1/2 2006.10.13 HYP2006 Mainz exp q1=0 q’=3/5 kF kF=1.35 fm-1 B8B8 systems classified in the SU3 states with (l, ) S B8B8(I) 1E, 3O (P =symmetric) 3E, 1O (P =antisymmetric) 0 NN(0) NN(1) ― (22) (03) ― ‐1 N N(1/2) N(3/2) ‐2 N(0) N(1) (0) (1) (2) ‐3 (1/2) (3/2) ‐4 (0) (1) (11)s 1 10 1 10 9 1 1 [(11)s+3(22)] [3(11)s‐(22)] (22) 2 1 2 1 (11)s+ 2 30(22)+ 2 2 (00) 5 3 1 1 (11) ‐ (22)+ (00) s 10 2 5 3 (11)s+ 52 (22) 5 2 3 ー 5 (11)s+ 5 (22) 1 3 3 (11) - (22)- (00) 2 10 8 s 5 ― (22) 1 10 1 10 2 1 2 ― (22) complete Pauli forbidden ― (11)a 1 [‐(11)a+ (30)+(03)] 3 1 [(30)‐(03)] 2 ― 1 [2(11)a+ (30)+(03)] 6 ― 1 [(11)s+3(22)] [3(11)s‐(22)] (22) [‐(11)a+(03)] [(11)a+(03)] (30) [‐(11)a+(30)] [(11)a+(30)] (03) (30) ― (30) almost forbidden (=2/9) Spin-flavor SU6 symmetry 1. Quark-model Hamiltonian is approximately SU3 scalar ・ no confinement contribution (assumption) ・ Fermi-Breit int. … quark-mass dependence only ・ EMEP … automatic SU3 relations for coupling constants phenomenology Cf. OBEP: exp data g, f, … (integrated) 2. -on plays an important role through SU3 relations and FSB 3. effect of the flavor symm. breaking (FSB) by ms>mud , B, M masses Characteristics of SU3 channels 1S, 3P (P-symmetric) (22) attractive pp 3S, 1P (P-antisymmetric) (03) strongly attractive np (11)s strongly repulsive N(I=1/2) (30) strongly repulsive N(I=3/2) (00) strongly attractive H-particle channel (11)a weakly attractive N(I=0) “only this part is ambiguous” 1S 0 phase shifts for B8B8 interactions with the pure (22) state (fss2) S=‐2 S=0 1S 0 S=‐3 S=‐1 S=‐4 (22) 3S 1 phase shifts NN 3S (3/2) fss2 1 (03) NN (03) central only (no tensor) (11)a N (0) (11)a : weakly (0) attractive (30) N (3/2) (30) : Pauli repulsion +p differential cross sections and +p, p asymmetries a() Ahn et al. (KEK-PS E251, E289) NP A648(1999)263, A761(2005)41 350 MeV/c plab 750 MeV/c Kurosawa et al. (KEK-PS E452B) KEK preprint 2005-104 (2006) +p +p elastic aexp=0.44±0.2 at p=800±200 MeV/c Kadowaki et al. (KEK-PS E452) Euro. Phys. J. A15 (2002) 295 p elastic reported by K. Nakai N interaction by fss2 Backward/Forward ratio P-wave N is weakly attractive fss2 FSS N - N coupling : 3S1 + 3D1 by one- tensor 1P + 3P by FB LS (-) 1 1 2006.10.13 HYP2006 Mainz from 3He Faddeev 3 H NN-NN CC Faddeev (hypertriton) Phys. Rev. C70, 024001 (2004) N on-shell properties are directly reflected 1S / 3S relative 0 1 “deuteron” Λ(∑0 ) u strength s d exp’t u u d = 2.22 MeV ~5 fm d B=130 ±50 keV p close to NSC89 P (%) ~2 fm u n d d fss2 289 keV 0.80 FSS 878 keV 1.36 NN = 19.37 – 21.03 = -1.66 |d |= 17.50 – 19.72 = -2.22 (MeV) 2006.10.13 HYP2006 Mainz 150 channel calculation N 1S0 and model 3S 1 effective range parameters FSS as (fm) rs (fm) -5.41 2.26 at (fm) rt (fm) -1.03 4.20 fss2 -2.59 2.83 -1.60 NSC89 -2.59 2.90 “fss2” -2.15 3.05 878 1.36 3.01 289 0.80 -1.38 3.17 143 0.5 -1.80 2.87 145 0.53 “fss2”: m c2 = 936 MeV 1,000 MeV B (keV) fss2 “fss2” 6 ch (S) 15 ch (SD) 102 ch (J4) 150 ch (J6) 137 198 288 289 44 85 145 145 2006.10.13 HYP2006 Mainz B(keV) P(%) favorable for 4H (1+) Effect of the higher partial waves is large 90 – 60 keV vs. 20 – 30 keV in NSC89 BΛexp=130 ±50 keV effective local potentials by G-matrix B8B8 interaction effective potentials quark-model N-N ND EB (exact) -3.62 MeV -3.18 MeV EBexp=3.120.02 MeV Cf. U(0)=‐46 (FSS), ‐48 (fss2) MeV in symmetric matter (3.04 MeV) 2+ 2 Faddeev for 9Be Phys. Rev. C70, 024002, 0407002 (2004) (0) 92 keV 0+ 8Be + + RGM kernel (MN3R) effective pot. (SB u=0.98) exp’t -3.120.02 MeV 3067(3) keV 3/2+ 3026 keV +5He 3024(3) keV 5/2+ 2828 keV -6.620.04 MeV + 1/2 9 Be calc. l s splitting by N LS Born kernel 198 keV (fss2 quark+), 137 keV (FSS) : 3 5 times too large Tamura et al. (BNL E930) Eexp(3/2+ - 5/2+) = 43 5 keV Akikawa, Phys. Rev. Let. 88, 082501 (2002) 2006.10.13 HYP2006 Mainz ls splitting of 9Be by 2 Faddeev using quark-model G-matrix LS Born kernel 0.5 0 kF (fm-1) 1.07 ‐10.5 -1.9 188 7 G-matrix fss2 (cont) S (MeV fm5) FSS (cont) Faddeev E (keV) fss2 (cont) FSS (cont) E exp (keV) 0.70 0 N Born 1.20 1.35 ‐10.6 ‐10.7 -2.9 -3.6 194 198 34 59 43 5 -10.9 -7.8 198 137 FSS (cont) reproduces E exp at kF=1.25 fm-1 ! P-wave N-N coupling by LS(-) is important. S-meson LS in fss2 is not favorable. 2006.10.13 HYP2006 Mainz potentials (VWC (R, 0)) by quark-model G-matrix interaction FSS fss2 I=3/2 I=3/2 total total I=1/2 I=1/2 The Pauli repulsion of N(I=3/2) 3S1 is very strong. 2006.10.13 HYP2006 Mainz (3N) potentials by quark-model G-matrix interaction ( 0+, T=1/2 channel) 3/2 V S ( 3 N ) ( S = 0, T = 1 / 2) = (4 / 3)V s FSS EB(exact)=-3.79 MeV + (3 / 2)V t 1/ 2 + (1 / 6)V s fss2 EB(exact)=-5.70 MeV consistent with 4He (0+) resonance 2006.10.13 HYP2006 Mainz 1/ 2 (3N): (0s)3 =0.22 fm-2 q1=0 (-, K+) inclusive spectra on 28Si exp: Noumi et al. PRL 89, 072301 (2002) ; 90, 049902 (E) (2003) Saha et al. Phys. Rev. C70, 044613 (2004) poster session by M. Kohno Repulsive U (q) in symmetric nuclear matter is experimentally confirmed. potentials (VWC (R, 0)) by quark-model G-matrix interaction fss2 FSS I=1 total total I=0 I=0 Some attraction in the surface region. I=1 +3.7 Tamagawa et al. (BNL-E906) -N (in medium) = 30.7±6.7 -3.6 mb Nucl. Phys. A691 (2001) 234c et al. (eikonal approx.)= 20.9±4.5 +2.5 mb Yamamoto Prog. Theor. Phys. 106 (2001)363 -2.4 -p /-n =1.1 +1.4+0.7 -0.7 -0.4 at plab=550 MeV/c FSS fss2 Ahn et al. Phys. Lett. B 633 (2006) 214 More experiments are needed. Summary Quark-model description for the baryon-baryon interaction is very successful to reproduce many experimental data. In particular, the extension of the (3q)-(3q) RGM study for the NN and YN interactions to the strangeness S=-2, -3, -4 sectors has clarified characteristic features of the B8B8 interactions. The results seem to be reasonable if we consider 1) spin-flavor SU6 symmetry 2) weak π-on effect in the strangeness sector 3) effect of the flavor symmetry breaking We have analyzed B8, B8(3N) interactions based on the G-matrix calculations of fss2 and FSS. 2006.10.13 HYP2006 Mainz Characteristics of fss2 and FSS S=0 ・ triton binding energy … fss2: +150 keV (3 body force?) S=‐1 p and +p interactions are progressively known. ・ + p total and differential cross sections and polarization … fss2, FSS ・ N 1S0 and 3S1 attraction (relative strength) ( 3H Faddeev calculation: 289 keV for fss2) ・ small ls splitting in 9Be excited states (FSS) ・ N (I=1/2 1S0), N (I=3/2 3S1) repulsion repulsive s. p. and potentials … fss2, FSS S=‐2 interaction is not much attractive ! ・ interaction |V|<|VN|<|VNN| B 1 MeV (Nagara event 6He) … fss2 ・ N in-medium total cross section (fss2, FSS) … strong isospin dependence of s.p. potential ・ N (I=0 3S1): (11)a 0 or weakly attractive (fss2, FSS) vs. ESC04(d): strongly attractive