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Weihu YE, Yibin QIAN. Study of Multiple Physical Constraints on the Duflo-Zuker Nuclear Mass Model[J]. Nuclear Physics Review, 2024, 41(1): 269-275. DOI: 10.11804/NuclPhysRev.41.2023CNPC20
Citation: Weihu YE, Yibin QIAN. Study of Multiple Physical Constraints on the Duflo-Zuker Nuclear Mass Model[J]. Nuclear Physics Review, 2024, 41(1): 269-275. DOI: 10.11804/NuclPhysRev.41.2023CNPC20

Study of Multiple Physical Constraints on the Duflo-Zuker Nuclear Mass Model

Funds: National Natural Science Foundation of China(12075121); Fundamental Research Funds for Central Universities (30922010312)
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  • Corresponding author:

    Yibin QIAN, E-mail: qyibin@njust.edu.cn

  • Received Date: June 28, 2023
  • Revised Date: November 09, 2023
  • Available Online: March 14, 2024
  • Nuclear mass plays an important role in both nuclear physics and astrophysics. While the theoretical accuracy of masses has reached quite astonishing accuracy, their extrapolations have been conflicting, especially in neutron-rich regions. This paper reviews the main results of the extrapolations of nuclear mass models in recent years. By using a rigorous multi-objective optimization on mass models, we take the mass differences α decay energy and the Garvey-Kelson relations as multiple physical constraints to reduce the degree of overfitting phenomenon, resulting that the predictive power of models was improved in some degree. In addition, we use the improved mass data for the rapid neutron capture processes in nuclear astrophysics, further validating the reliability of the extrapolations.
  • [1]
    LUNNEY D, PEARSON J, THIBAULT C. Rev Mod Phys, 2003, 75(3): 1021. DOI: 10.1103/RevModPhys.75.1021
    [2]
    LARSEN A C, SPYROU A, LIDDICK S N, et al. Prog Part Nucl Phys, 2019, 107: 69. DOI: 10.1016/j.ppnp.2019.04.002
    [3]
    YAMAGUCHI T, KOURA H, LITVINOV Y A, et al. Prog Part Nucl Phys, 2021, 120: 103882. DOI: 10.1016/j.ppnp.2021.103882
    [4]
    ERLER J, BIRGE N, KORTELAINEN M, et al. Nature, 2012, 486(7404): 509. DOI: 10.1038/nature11188
    [5]
    何建军, 郭冰, 柳卫平, 等. 科学通报, 2018, 63(24): 2439. DOI: 10.1360/N972017-01368

    HE Jianjun, GUO Bing, LIU Weiping, et al. Chinese Science Bulletin, 2018, 63(24): 2439. (in Chinese) DOI: 10.1360/N972017-01368
    [6]
    CHAI Q, QIANG Y, PEI J. Phys Rev C, 2022, 105: 034315. DOI: 10.1103/PhysRevC.105.034315
    [7]
    DUFLO J, ZUKER A. Phys Rev C, 1995, 52: R23. DOI: 10.1103/PhysRevC.52.R23
    [8]
    MÖLLER P, MYERS W D, SAGAWA H, et al. Phys Rev Lett, 2012, 108(5): 052501. DOI: 10.1103/PhysRevLett.108.052501
    [9]
    SCHUETRUMPF B, REINHARD P G, STEVENSON P, et al. Comput Phys Commun, 2018, 229: 211. DOI: 10.1016/j.cpc.2018.03.012
    [10]
    NEUFCOURT L, CAO Y, NAZAREWICZ W, et al. Phys Rev C, 2018, 98: 034318. DOI: 10.1103/PhysRevC.98.034318
    [11]
    GARVEY G T, KELSON I. Phys Rev Lett, 1966, 16: 197. DOI: 10.1103/PhysRevLett.16.197
    [12]
    GARVEY G, GERACE W, JAFFE R, et al. Rev Mod Phys, 1969, 41(4): S1. DOI: 10.1103/RevModPhys.41.S1
    [13]
    FU G, JIANG H, ZHAO Y, et al. Phys Rev C, 2010, 82: 034304. DOI: 10.1103/PhysRevC.82.034304
    [14]
    JIANG H, FU G, SUN B, et al. Phys Rev C, 2012, 85: 054303. DOI: 10.1103/PhysRevC.85.054303
    [15]
    DONG J, GU J, ZHANG Y, et al. Phys Rev C, 2019, 99: 014319. DOI: 10.1103/PhysRevC.99.014319
    [16]
    DONG J, ZHANG Y, ZUO W, et al. Phys Rev C, 2018, 97: 021301. DOI: 10.1103/PhysRevC.97.021301
    [17]
    BAO M, HE Z, LU Y, et al. Phys Rev C, 2013, 88: 064325. DOI: 10.1103/PhysRevC.88.064325
    [18]
    BAO M, HE Z, CHENG Y, et al. Science China Physics, Mechanics & Astronomy, 2017, 60: 1.
    [19]
    BAO M, LU Y, ZHAO Y, et al. Phys Rev C, 2016, 94: 044323. DOI: 10.1103/PhysRevC.94.044323
    [20]
    ZONG Y, LIN M, BAO M, et al. Phys Rev C, 2019, 100: 054315. DOI: 10.1103/PhysRevC.100.054315
    [21]
    鲍曼, 姜慧, 赵玉民. 原子核物理评论, 2023, 40(2): 141. DOI: 10.11804/NuclPhysRev.40.2022098

    BAO Man, JIANG Hui, ZHAO Yumin. Nuclear Physics Review, 2023, 40(2): 141. (in Chinese) DOI: 10.11804/NuclPhysRev.40.2022098
    [22]
    NIU Z, LIANG H. Phys Lett B, 2018, 778: 48. DOI: 10.1016/j.physletb.2018.01.002
    [23]
    UTAMA R, PIEKAREWICZ J. Phys Rev C, 2017, 96: 044308. DOI: 10.1103/PhysRevC.96.044308
    [24]
    UTAMA R, PIEKAREWICZ J. Phys Rev C, 2018, 97: 014306. DOI: 10.1103/PhysRevC.97.014306
    [25]
    NIU Z, FANG J, NIU Y, et al. Phys Rev C, 2019, 100: 054311. DOI: 10.1103/PhysRevC.100.054311
    [26]
    SHARMA A, GANDHI A, KUMAR A. Phys Rev C, 2022, 105: L031306. DOI: 10.1103/PhysRevC.105.L031306
    [27]
    MUMPOWER M R, SPROUSE T M, LOVELL A E, et al. Phys Rev C, 2022, 106: L021301. DOI: 10.1103/PhysRevC.106.L021301
    [28]
    LOVELL A E, MOHAN A T, SPROUSE T M, et al. Phys Rev C, 2022, 106: 014305. DOI: 10.1103/PhysRevC.106.014305
    [29]
    LI C Q, TONG C N, DU H J, et al. Phys Rev C, 2022, 105: 064306. DOI: 10.1103/PhysRevC.105.064306
    [30]
    WU X, LU Y, ZHAO P. Phys Lett B, 2022, 834: 137394. DOI: 10.1016/j.physletb.2022.137394
    [31]
    SOBICZEWSKI A, LITVINOV Y A. Phys Rev C, 2014, 90: 017302. DOI: 10.1103/PhysRevC.90.017302
    [32]
    SOBICZEWSKI A, LITVINOV Y A. Phys Rev C, 2014, 89: 024311. DOI: 10.1103/PhysRevC.89.024311
    [33]
    PASTORE A, NEILL D, POWELL H, et al. Phys Rev C, 2020, 101: 035804. DOI: 10.1103/PhysRevC.101.035804
    [34]
    LIU M, WANG N, DENG Y, et al. Phys Rev C, 2011, 84: 014333. DOI: 10.1103/PhysRevC.84.014333
    [35]
    GORIELY S, CHAMEL N, PEARSON J. Phys Rev C, 2010, 82: 035804. DOI: 10.1103/PhysRevC.82.035804
    [36]
    GORIELY S, CHAMEL N, PEARSON J. Phys Rev C, 2013, 88: 024308. DOI: 10.1103/PhysRevC.88.024308
    [37]
    MENDOZA-TEMIS J, HIRSCH J G, ZUKER A P. Nucl Phys A, 2010, 843(1-4): 14. DOI: 10.1016/j.nuclphysa.2010.05.055
    [38]
    KIRSON M W. Nucl Phys A, 2012, 893: 27. DOI: 10.1016/j.nuclphysa.2012.09.001
    [39]
    MARLER R T, ARORA J S. Struct Multidiscip Optim, 2004, 26(6): 369. DOI: 10.1007/s00158-003-0368-6
    [40]
    NGATCHOU P, ZAREI A, EL-SHARKAWI A. Pareto Multi Objective Optimization[C]//Proceedings of the 13th International Conference on, Intelligent Systems Application to Power Systems. IEEE, 2005: 84.
    [41]
    TAPIA M G C, COELLO C A C. Applications of Multi-objective Evolutionary Algorithms in Economics and Finance: A Survey[C]//2007 IEEE Congress on Evolutionary Computation. IEEE, 2007: 532.
    [42]
    FORTIN F A, PARIZEAU M. Revisiting the Nsga-ii crowdingdistance Computation[C]//Proceedings of the 15th Annual Conference on Genetic and Evolutionary Computation. 2013: 623.
    [43]
    DEB K, PRATAP A, AGARWAL S, et al. IEEE Trans Evol Comput, 2002, 6(2): 182. DOI: 10.1109/4235.996017
    [44]
    WANG M, HUANG W, KONDEV F, et al. Chin Phys C, 2021, 45: 030003. DOI: 10.1088/1674-1137/abddaf
    [45]
    BAREA J, FRANK A, HIRSCH J, et al. Phys Rev C, 2008, 77(4): 041304. DOI: 10.1103/PhysRevC.77.041304
    [46]
    ORFORD R, VASSH N, CLARK J, et al. Phys Rev C, 2022, 105: L052802. DOI: 10.1103/PhysRevC.105.L052802
    [47]
    PORTER W, ASHRAFKHANI B, BERGMANN J, et al. Phys Rev C, 2022, 105: L041301. DOI: 10.1103/PhysRevC.105.L041301
    [48]
    LI H, NAIMI S, SPROUSE T, et al. Phys Rev Lett, 2022, 128: 152701. DOI: 10.1103/PhysRevLett.128.152701
    [49]
    QIAN Y Z, WOOSLEY S. Astrophys J, 1996, 471: 331. DOI: 10.1086/177973
    [50]
    [51]
    [EB/OL]. [2023-06-10] https://reaclib.jinaweb.org/.
    [52]
    ARNOULD M, GORIELY S, TAKAHASHI K. Phys Rep, 2007, 450(4-6): 97. DOI: 10.1016/j.physrep.2007.06.002
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