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Coulomb breakup of the two-neutron halo nucleus 11 Li Takashi Nakamura Tokyo Institute of Technology International Conference on Finite Fermionic Systems.

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Presentation on theme: "Coulomb breakup of the two-neutron halo nucleus 11 Li Takashi Nakamura Tokyo Institute of Technology International Conference on Finite Fermionic Systems."— Presentation transcript:

1 Coulomb breakup of the two-neutron halo nucleus 11 Li Takashi Nakamura Tokyo Institute of Technology International Conference on Finite Fermionic Systems Nilsson Model 50 Years June 14-18 2005, Lund, Sweden

2 T.Nakamura, A.M. Vinodkumar, T.Sugimoto, N.Fukuda, M.Miura, Y.Kondo, N.Aoi, N.Imai, T.Kubo, T.Kobayashi, T.Gomi, A.Saito, H.Sakurai, S.Shimoura,D.Bazin, H.Hasegawa, H.Baba, T. Motobayashi, T.Yakushiji, Y. Yanagisawa, K.Yoneda, K. Watanabe, Y.X.Watanabe, M.Ishihara

3 Coulomb Breakup 11 Li High-Z Target (Pb) 9 Li n  = N E1 (E x ) dB(E1) dE x d  CD dE x 9hc 16  3 Cross section = (Photon Number)x  Transition Probability) Invariant Mass ~70MeV/nucleon (  ~0.4 c ) Equivalent Photon Method Introduction 11 Li* n

4 11 Be – One neutron Halo Case ExEx 10~20MeV 1~2MeV N.Fukuda, TN et al., PRC70, 054606 (2004) TN et al.,PLB 331,296(1994) dB(E1) dE x S n =504keV core n dB(E1) dE x  exp(iqr)| rY 1 m |  gs  | 2 Z A Direct Breakup

5 |  gs (1/2 + )  =  | 10 Be(0 + )  s 1/2  | 10 Be(2 + )  d 5/2      : Spectroscopic factor dB(E1) dE x  exp(iqr)| rY 1 m |  gs  | 2 Z A   -S n  ~   |exp(-r/ )/r| 2 Fourier Transform   = 0.72  c.f.   = 0.77 10 Be(d,p) 11 Be  2 = 0.61(5) R.Palit PRC68,034318(2003)(GSI) Low-lying E1 Strength Halo State Spectroscopic Significance---1n Halo nucleus 11 Be(g.s.) Exclusively Sensitive to the Halo State B(E1) @E~1MeV  exp(iqr)| rY 1 m | s 1/2  | 2 Z A Halo State Direct Breakup Mechanism N.Fukuda, TN et al., PRC70, 054606 (2004)

6 One neutron halo nucleus vs. Two neutron halo nucleus 9Li9Li n n 10 Be n Motion between core and 1 valence neutron Motion between 1.Core and neutron 2.Core and neutron 3.Two valence neutrons (neutron-neutron correlations) S 2n =300 keV S n =504 keV

7 RIKEN @ 43MeV/nucleon PLB348 (1995) 29. MSU@ 28MeV/nucleon PRL 70 (1993) 730. Coulomb Dissocitaion of 11 Li GSI @280MeV/nucleon NPA 619 (1997) 151. dB(E1)/dEx Should be Compared !

8 Coulomb Dissocitaion of 11 Li (Summary of Previous Results) RIKEN @ 43MeV/nucleon PLB348 (1995) 29. GSI @280MeV/nucleon NPA 619 (1997) 151. MSU@ 28MeV/nucleon PRL 70 (1993) 730. PRC 48(1993) 118.

9 11 Li 9 Li n n Experimental Setup @RIPS at RIKEN Pb Target NEUT HOD BOMAG DC DALI 70MeV/nucleon

10 Examine Different Wall Events t1t1 t2t2 11 22  12 Condition: Almost no bias E th =6MeVee to avoid any gamma related events Elimination of Cross-Talk events

11 Coulomb Dissociation Spectrum of 11 Li Preliminary 11 Li 9 Li+n+n

12 Angular Distribution E1 Strength Distribution

13 =E x (E rel +0.2MeV) Uncorrelated pair Correlated Pair Independent Particle Model ( 10 Li+n) H.Esbensen et al.,NPA542(1992)310. “Soft dipole excitations in 11 Li” Correlation? (E rel ~0.2MeV) (E rel ~0.7MeV)

14 Correlation? B(E1) sum rule (H.Esbensen et al.,NPA542(1992)310.) Experimental value c.f. Shimoura et al.,PLB348(1995)29. Correlated pair 1.57 e 2 fm 2 ~60deg Independent Particle 1.07e 2 fm 2 90deg Preliminary

15 Experimental Result E(9Li-n) 1MeV Simulation (Phase-space decay) E(9Li-n) 1MeV Correlation? Preliminary

16 Summary Coulomb Dissociation----- Low-lying B(E1) Strength ---- Sensitive to Halo s-wave neutron x Core( 0 + ) Powerful Spectroscopic Tool 11 Be(1n halo)+Pb Data 11 Li(2n halo)+Pb Data Low-lying B(E1) Strength Could be used to see the nn correlation & 9 Li-n correlation in 11 Li (E1 Non-energy weighted sum rule) Strong B(E1) at very low excitation energy E( 9 Li-n) - E( 9 Li-n) 2 dimensional Plot Strong Correlations Theoretical interpretation is necessary   = 0.72  N.Fukuda, T.N. et al., PRC70, 054606 (2004)


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