NUCLEAR PHYSICS |
|
|
|
|
Symmetry Potential and Effective Mass with Consistent Three-Body Force |
LI Zeng-Hua1,2**, ZUO Wei3 |
1Institute of Modern Physics, Fudan University, Shanghai 200433 2Applied Ion Beam Physics Laboratory (Ministry of Education), Fudan University, Shanghai 200433 3Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000 |
|
Cite this article: |
LI Zeng-Hua, ZUO Wei 2012 Chin. Phys. Lett. 29 062104 |
|
|
Abstract The momentum and isospin dependence of symmetry potential and effective mass in isospin asymmetric nuclear matter is investigated in the framework of the Brueckner–Hartree–Fock approach by adopting the realistic Bonn B two-body interaction in combination with a consistent microscopic three-body force. It is demonstrated that symmetry potentials at the normal density for different asymmetry parameters are in good agreement with the empirical value constrained by the experimental data, and the neutron and proton effective masses show strong isospin splitting with mn*>mp* on the whole range of asymmetry parameters. In the end, the density dependence of the Landau mass is displayed.
|
Keywords:
21.65.Cd
21.30.Fe
21.45.Ff
|
|
Received: 18 November 2011
Published: 31 May 2012
|
|
PACS: |
21.65.Cd
|
(Asymmetric matter, neutron matter)
|
|
21.30.Fe
|
(Forces in hadronic systems and effective interactions)
|
|
21.45.Ff
|
(Three-nucleon forces)
|
|
|
|
|
[1] Bertsch G F and Gupta S D 1988 Phys. Rep. 160 189[2] Li B A 2000 Phys. Rev. Lett. 85 4221 and references therein[3] Chen L W, Ko C M and Li B A 2005 Phys. Rev. Lett. 94 032701[4] Li Q F, Li Z X and Soff S 2006 J. Phys. G 32 407[5] Gao Y, Zhang L, Zhang H F et al 2011 Phys. Rev. C 83 047602[6] Feng Z Q 2011 Phys. Rev. C 84 024610[7] Lattimer J M and Prakash M 2000 Phys. Rep. 333 121[8] Cugnon J, Lejeune A and P Grang? 1987 Phys. Rev. C 35 861[9] Li Z H, Lombardo U, Schulze H J et al 2006 Phys. Rev. C 74 047304[10] Machleidt R, Holinde K and Elster Ch 1987 Phys. Rep. 149 1[11] Li Z H, Lombardo U, Schulze H J and Zuo W 2008 Phys. Rev. C 77 034316[12] Jeukenne J P, Lejeune A and Mahaux C 1976 Phys. Rep. 25 83[13] Grang? P, Lejeune A, Martzolff M and Mathiot J F 1989 Phys. Rev. C 40 1040[14] Coon S A, Scadron M D, McNamee P C et al 1979 Nucl. Phys. A 317 242[15] Baldo M and Ferreira L S 1999 Phys. Rev. C 59 682[16] Bombaci I and Lombardo U 1991 Phys. Rev. C 44 1892[17] Zuo W, Cao L G, Li B A et al 2005 Phys. Rev. C 72 014005[18] Lane A M 1962 Nucl. Phys. 35 676[19] Koning A J and Delaroche J P 2003 Nucl. Phys. A 713 231[20] Sammarruca F, Barredo W and Krastev P 2005 Phys. Rev. C 71 064306[21] Zuo W, Lombardo U, Schulze H J and Li Z H 2006 Phys. Rev. C 74 014317[22] Bombaci I and Lombardo U 1991 Phys. Rev. C 44 1892[23] Rizzo J, Colonna M, Di Toro M and Greco V 2004 Nucl. Phys. A 732 202[24] Jaminon M and Mahaux C 1989 Phys. Rev. C 40 354[25] van Dalen E N E, Fuchs C and Faessler A 2005 Phys. Rev. C 72 065803 |
|
Viewed |
|
|
|
Full text
|
|
|
|
|
Abstract
|
|
|
|
|