Constraining Isovector Nuclear Interactions with Giant Dipole Resonance and Neutron Skin in $^{208}$Pb from a Bayesian Approach
Jun Xu1,2*
1 The Interdisciplinary Research Center, Shanghai Advanced Research Institute, Chinese Academy of Sciences, Shanghai 201210, China2 Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Shanghai 201800, China
Abstract ：The remaining uncertainties in relation to isovector nuclear interactions call for reliable experimental measurements of isovector probes in finite nuclei. Based on the Bayesian analysis, although neutron-skin thickness data or isovector giant dipole resonance data in $^{208}$Pb can constrain only one isovector interaction parameter, correlations among other parameters can also be built. Using combined data for both the neutron-skin thickness and the isovector giant dipole resonance helps to significantly constrain all isovector interaction parameters; as such, it serves as a useful methodology for future research.
收稿日期: 2020-12-17
出版日期: 2021-04-06
:
21.65.Ef
(Symmetry energy)
21.60.Jz
(Nuclear Density Functional Theory and extensions (includes Hartree-Fock and random-phase approximations))
21.10.Gv
(Nucleon distributions and halo features)
[1] Baran V, Colonna M, Greco V and Di Toro M 2005 Phys. Rep. 410 335 [2] Steiner A W, Prakash M, Lattimer J M and Ellis P J 2005 Phys. Rep. 411 325 [3] Lattimer J M and Prakash M 2007 Phys. Rep. 442 109 [4] Li B A, Chen L W and Ko C M 2008 Phys. Rep. 464 113 [5] Li B A and Han X 2013 Phys. Lett. B 727 276 [6] Oertel M, Hempel M, Klähn T and Typel S 2017 Rev. Mod. Phys. 89 015007 [7] Li B A, Cai B J, Chen L W and Xu J 2018 Prog. Part. Nucl. Phys. 99 29 [8] Xu C, Li B A and Chen L W 2010 Phys. Rev. C 82 054607 [9] Trippa L, Colò G and Vigezzi E 2008 Phys. Rev. C 77 061304(R) [10] Reinhard P G and Nazarewicz W 2010 Phys. Rev. C 81 051303(R) [11] Piekarewicz J, Agrawal B K, Colò G, Nazarewicz W, Paar N, Reinhard P G, Roca-Maza X and Vretenar D 2012 Phys. Rev. C 85 041302(R) [12] Vretenar D, Niu Y F, Paar N and Meng J 2012 Phys. Rev. C 85 044317 [13] Roca-Maza X, Brenna M, Colò G, Centelles M, Vi N X, Agrawal B K, Paar N, Vretenar D and Piekarewicz J 2013 Phys. Rev. C 88 024316 [14] Colò G, Garg U and Sagawa H 2014 Eur. Phys. J. A 50 26 [15] Roca-Maza X, Vi N X, Centelles M, Agrawal B K, Colò G, Paar N, Piekarewicz J and Vretenar D 2015 Phys. Rev. C 92 064304 [16] Zhang Z and Chen L W 2015 Phys. Rev. C 92 031301(R) [17] Zheng H, Burrello S, Colonna M and Baran V 2016 Phys. Rev. C 94 014313 [18] Xu J and Qin W T 2020 Phys. Rev. C 102 024306 [19] Zhang Z and Chen L W 2016 Phys. Rev. C 93 034335 [20] Kong H Y, Xu J, Chen L W, Li B A and Ma Y G 2017 Phys. Rev. C 95 034324 [21] Brown B A 2000 Phys. Rev. Lett. 85 5296 [22] Typel S and Brown B A 2001 Phys. Rev. C 64 027302 [23] Horowitz C J and Piekarewicz J 2001 Phys. Rev. Lett. 86 5647 [24] Furnstahl R J 2002 Nucl. Phys. A 706 85 [25] Todd-Rutel B G and Piekarewicz J 2005 Phys. Rev. Lett. 95 122501 [26] Centelles M, Roca-Maza X, Viñas X and Warda M 2009 Phys. Rev. Lett. 102 122502 [27] Zhang Z and Chen L W 2013 Phys. Lett. B 726 234 [28] Agrawal B K, Malik T, De J N and Samaddar S K 2020 arXiv:2006.05758 [nucl-th] [29] Behera D, Tripathy S K, Routray T R and Behera B 2020 Phys. Scr. 95 105301 [30] Thiel M, Sfienti C, Piekarewicz J, Horowitz C J and Vanderhaeghen M 2019 J. Phys. G 46 093003 [31] Burgio G F and Vidaña I 2020 Universe 6 119 [32] Vi X, Centelles M, Roca-Maza X and Warda M 2014 Eur. Phys. J. A 50 27 [33] Roca-Maza X and Paar N 2018 Prog. Part. Nucl. Phys. 101 96 [34] Chen L W, Li B A, Ko C M and Xu J 2010 Phys. Rev. C 82 024321 [35] Chabanat E, Bonche P, Haensel P, Meyer J and Schaeffer R 1997 Nucl. Phys. A 627 710 [36] Vautherin D and Brink D M 1972 Phys. Rev. C 5 626 [37] Reinhard P G 1991 Computational Nuclear Physics 1: Nuclear Structure ed Langanke K, Maruhn J A and Koonin S E (New York: Springer-Verlag) chap 2 p 209 [38] Colò G, Cao L, Van Gia N and Capelli L 2013 Comput. Phys. Commun. 184 142 [39] Dietrich S S and Berman B L 1988 At. Data Nucl. Data Tables 38 199 [40] Tamii A, Poltoratska I, vonNeumann-Cosel P et al. 2011 Phys. Rev. Lett. 107 062502 [41] Zenihiro J, Sakaguchi H, Murakami T, Yosoi M, Yasuda Y, Terashima S, Iwao Y, Takeda H, Itoh M, Yoshida H P and Uchida M 2010 Phys. Rev. C 82 044611 [42] Friedman E 2012 Nucl. Phys. A 896 46 [43] Klos B et al. 2007 Phys. Rev. C 76 014311 [44] Brown B A, Shen G, Hillhouse G C, Meng J and Trzcinska A 2007 Phys. Rev. C 76 034305 [45] Tarbert C M et al. 2014 Phys. Rev. Lett. 112 242502 [46] Abrahamyan S et al. 2012 Phys. Rev. Lett. 108 112502 [47] Xu J, Xie W J and Li B A 2020 Phys. Rev. C 102 044316 [48] Xu J, Zhou J, Zhang Z, Xie W J and Li B A 2020 Phys. Lett. B 810 135820
[1]
.
[2]
.
[3]
.
[4]
.
[5]
.
[6]
.
[7]
.
[8]
MA Chun-Wang, PU Jie, WANG Shan-Shan, WEI Hui-Ling. The Symmetry Energy from the Neutron-Rich Nucleus Produced in the Intermediate-Energy 40,48 Ca and 58,64 Ni Projectile Fragmentation
[9]
ZHANG Fang,HU Bi-Tao,YONG Gao-Chan,ZUO Wei. Effects of Symmetry Energy in the Reaction 40 Ca+124 Sn at 140 MeV/Nucleon
[10]
ZHANG Fang**,LIU Yang,YONG Gao-Chan,ZUO Wei. Probing Nuclear Symmetry Energy with the Sub-threshold Pion Production
[11]
LI Zeng-Hua;**;ZHANG Da-Peng;SCHULZE Hans-Josef;ZUO Wei. Second-Order Contribution of the Incompressibility in Asymmetric Nuclear Matter
[12]
ZHOU Pei;TIAN Wen-Dong**;MA Yu-Gang**;CAI Xiang-Zhou;FANG De-Qing;WANG Hong-Wei
. The influence of Multi-Step Sequential Decay on Isoscaling and Fragment Isospin Distribution in GEMINI Simulation
[13]
BAI Chun-Lin;**;ZHANG HUAN-Qiao;ZHANG Xi-Zhen;XU Fu-Rong;H. Sagawa;G. Colò. Effect of the Tensor Force on Charge-Exchange Spin-Dependent Multipole Excitations
[14]
Sanjeev Kumar;Suneel Kumar. Systematic Study on System Size Dependence of Global Stopping: Role of Momentum-Dependent Interactions and Symmetry Energy
[15]
JIANG Wei-Zhou;CHEN Yun-Peng;LU Xing. De-excitation Energy of Superdeformed Secondary Minima of Odd-Odd Au Isotopes and Its Sensitivity to the Density Dependence of Symmetry Energy
2021, Vol. 38 
