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《中国物理C》(英文)编辑部
2024年10月30日

Influence of isovector pairing and particle-number projection effects on spectroscopic factors for one-pair like-particle transfer reactions in proton-rich even-even nuclei

  • Isovector neutron-proton (np) pairing and particle-number fluctuation effects on the spectroscopic factors (SF) corresponding to one-pair like-particle transfer reactions in proton-rich even-even nuclei are studied. With this aim, expressions of the SF corresponding to two-neutron stripping and two-proton pick-up reactions, which take into account the isovector np pairing effect, are established within the generalized BCS approach, using a schematic definition proposed by Chasman. Expressions of the same SF which strictly conserve the particle number are also established within the Sharp-BCS (SBCS) discrete projection method. In both cases, it is shown that these expressions generalize those obtained when only the pairing between like particles is considered. First, the formalism is tested within the Richardson schematic model. Second, it is applied to study even-even proton-rich nuclei using the single-particle energies of a Woods-Saxon mean-field. In both cases, it is shown that the np pairing effect and the particle-number projection effect on the SF values are important, particularly in N=Z nuclei, and must then be taken into account.
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  • [1] B. Blank and M. J. G. Borge, Progr. Part. Nucl. Phys., 60:403-483 (2008)
    [2] M. Pfutzner, M. Karny, L. V. Grigorenko et al, Rev. Mod. Phys., 84:567-619 (2012)
    [3] H. Sagawa and K. Hagino, Eur. Phys. J. A, 51:102 (2015)
    [4] T. Nakamura, H. Sakurai, and H. Watanabe, Progr. Part. Nucl. Phys., 97:53-122 (2017)
    [5] A. L. Goodman, Adv. Nucl. Phys., 11:263-366 (1979)
    [6] J. Engel, S. Pittel, M. Stoitsov et al, Phys. Rev. C, 55:1781-1788 (1997)
    [7] O. Civitarese and M. Reboiro, Phys. Rev. C, 56:1179-1182 (1997)
    [8] A. A. Raduta, L. Pacearescu, P. Sarriguren et al, Nucl. Phys. A, 675:503-530 (2000)
    [9] F. Simkovic, Ch. C. Moustakidis, L. Pacearescu et al, Phys. Rev. C, 68:054319 (2003)
    [10] N. Sandulescu, D. Negrea, J. Dukelsky et al, Phys. Rev. C, 85:061303 (R) (2012)
    [11] H. Sagawa, Y. Tanimura, and K. Hagino, Phys. Rev. C, 87:034310 (2013)
    [12] N. Hinohara and J. Engel, Phys. Rev. C, 90:031301 (R) (2014)
    [13] M. Sambataro and N. Sandulescu, Phys. Rev. C, 93:054320 (2016)
    [14] Wenjin Tan, Dongdong Ni, and Zhongzhou Ren, Chin. Phys. C, 41:54103 (2017)
    [15] P. Van Isacker, J. Engel, and K. Nomura, arXiv:1708.05925.
    [16] S. Frauendorf and A. O. Machiavelli, Prog. Part. Nucl. Phys., 78:24-90 (2014)
    [17] C. Qi and R. Wyss, Phys. Scr., 91:013009 (2016)
    [18] J. Bardeen, L. N. Cooper and J. R. Schriefier, Phys. Rev., 106:162-164 (1957)
    [19] A. Goswami, Nucl. Phys., 60:228-240 (1964)
    [20] A. Goswami and L. S. Kisslinger, Phys. Rev., 140:B26-B31 (1965)
    [21] H. T. Chen and A. Goswami, Nucl. Phys., 88:208-214 (1966)
    [22] H. Chen and A. Goswami, Phys. Lett. B, 24:257-259 (1967)
    [23] G. G. Dussel, E. Maqueda and R. P. J. Perazzo, Nucl. Phys. A, 153:469-480 (1970)
    [24] H. H. Wolter, A. Faessler and P. U. Sauer, Nucl. Phys. A, 167:108-128 (1971)
    [25] A. L. Goodman, Nucl. Phys. A, 186:475-492 (1972)
    [26] O. Civitarese, M. Reboiro and P. Vogel, Phys. Rev. C, 56:1840-1843 (1997)
    [27] D. Mokhtari, N. H. Allal and M. Fellah, Acta Phys. Hung. A:Heavy Ion Phys., 19:187-190 (2004)
    [28] D. Mokhtari, M. Fellah and N. H. Allal, Int. J. Mod. Phys. E, 25:1650035 (2016)
    [29] P. Ring and P. Schuck, The Nuclear Many Body Problem, (Berlin, Springer, 1980)
    [30] J. Dukelsky, S. Pittel and C. Esebbag, Phys. Rev. C, 93:034313 (2016)
    [31] N. H. Allal and M. Fellah, Phys. Rev. C, 43:2648-2657 (1991)
    [32] N. H. Allal, M. Fellah, N. Benhamouda et al, Phys. Rev. C, 77:054310 (2008)
    [33] Faiza Hammache, N. H. Allal, M. Fellah et al, Int. J. Mod. Phys. E, 25:1650032 (2016)
    [34] N. Benhamouda, N. H. Allal, M. Fellah et al, Int. J. Mod. Phys. E, 17:1357-1365 (2008)
    [35] S. Kerrouchi, D. Mokhtari, N. H. Allal et al, Int. J. Mod. Phys. E, 18:141-160 (2009)
    [36] M. Douici, N. H. Allal, M. Fellah, et al, Int. J. Mod. Phys. E, 21:1250046 (2012)
    [37] N. H. Allal, M. Fellah, M. Douici et al, Int. J. Mod. Phys. E, 25:1650108 (2016)
    [38] M. Douici, N.H. Allal, M. Fellah, et al, Int. J. Mod. Phys. E, 22:1350029 (2013)
    [39] M. Borrajo and J. L. Egido, Phys. Lett. B, 764:328-334 (2017)
    [40] D. C. Zheng, D. W. L. Sprung and H. Flocard, Phys. Rev. C, 46:1355-1363 (1992)
    [41] J. A. Sheikh, P. Ring, E. Lopes et al, Phys. Rev. C 66:044318 (2002)
    [42] G. Hupin and Denis Lacroix, Phys. Rev. C, 86:024309 (2012)
    [43] S. Kerrouchi, N. H. Allal, M. Fellah et al, Int. J. Mod. Phys. E, 19:1383-1409 (2010)
    [44] S. Kerrouchi, N. H. Allal, M. Fellah et al, Int. J. Mod. Phys. E, 24:1550014 (2015)
    [45] H. J. Lipkin, Ann. Phys. (NY), 12:452-462 (1960)
    [46] Y. Nogami, Phys. Rev., 134, B313-B321 (1964)
    [47] W. Satula and R. Wyss, Phys. Lett. B, 393:1-6 (1997)
    [48] W. Satula and R. Wyss, Nucl. Phys. A, 676:120-142 (2000)
    [49] K. Sieja and A. Baran, Acta Phys. Pol. B, 35:107-114 (2006)
    [50] V. N. Fomenko, J. Phys A, 3:8-20 (1970)
    [51] M. Fellah, T. F. Hammann, and D. E. Medjadi, Phys. Rev. C, 8:1585-1592 (1973)
    [52] M. Fellah and T. F. Hammann, Phys. Rev. C, 20:1560-1571 (1979)
    [53] N. H. Allal, M. Fellah, M. R. Oudih et al, Eur. Phys. J. A, 27, s01:301-306 (2006)
    [54] N. Sandulescu, B. Erren and J. Dukelsky, Phys. Rev. C, 80:044335 (2009)
    [55] M. Fellah, N. H. Allal, Faiza Hammache et al, Int. J. Mod. Phys. E, 24:1550097 (2015)
    [56] K. Allaart and E. Boeker, Nucl. Phys. A, 168:630-662 (1971)
    [57] M. R. Oudih, M. Fellah and N. H. Allal, Int. J. Mod. Phys. E, 12:109-123 (2003)
    [58] M. V. Stoitsov, J. Dobaczewski, R. Kirchner, et al, Phys. Rev. C, 76:014308 (2007)
    [59] H. Olofsson, R. Bengtsson and P. Moller, Nucl. Phys. A, 784:104-146 (2007)
    [60] M. R. Oudih, M. Fellah, N. H. Allal et al, Phys. Rev. C, 76:047307 (2007)
    [61] A. A. Raduta, M. I. Krivoruchenko and A. Faessler, Phys. Rev. C, 85:054314 (2012)
    [62] A. A. Raduta and E. Moya de Guerra, Ann. Phys. (NY), 284:134-166 (2000)
    [63] K. Sieja, T. L. Ha, P. Quentin et al., Int. J. Mod. Phys. E, 16:289-298 (2007)
    [64] L. Bonneau, P. Quentin, and K. Sieja, Phys. Rev. C, 76:014304 (2007)
    [65] H. Laftchiev, J. Libert, P. Quentin et al, Nucl. Phys. A, 845:33-57 (2010)
    [66] K. W. Schmid, F. Grummer and A. Faessler, Ann. Rev. (NY), 180:1-73 (1987)
    [67] A. Petrovici, K. W. Schmid and Amand Faessler, Nucl. Phys. A, 647:197-216 (1999)
    [68] A. Petrovici, K. W. Schmid and Amand Faessler, Nucl. Phys. A, 728:396-414 (2003)
    [69] R. R. Chassman, Phys. Rev. Lett., 95:262501 (2005)
    [70] R. R. Chassman and P. Van Isacker, Phys. Lett. B, 685:55-58 (2010)
    [71] A. Mukherjee, Y. Alhassid, and G. F. Bertsch, Phys. Rev. C, 83:014319 (2011)
    [72] L.Y. Jia, Phys. Rev. C, 88:044303 (2013)
    [73] L. Y. Jia, Nucl. Phys. A, 941:293-306 (2015)
    [74] J. Q. Chen, Nucl. Phys. A, 626:686-714 (2000)
    [75] Y. M. Zhao, N. Yoshinaga, S. Yamaji et al, Phys. Rev. C, 62:014304 (2000)
    [76] G. J. Fu, Y. Lei, Y. M. Zhao et al, Phys. Rev. C, 87:044310 (2013)
    [77] S. Shlomo and I. Talmi, Nucl. Phys. A, 198:81-108 (1972)
    [78] L. Y. Jia, J. Phys. G:Nucl. Part. Phys., 42:115105 (2015)
    [79] M.-J. Cheng, L. Liu, and Y.-X. Zhang, Chin. Phys. C, 39:104102 (2015)
    [80] N. K. Timofeyuk, Phys. Rev. C, 81:064306 (2010)
    [81] O. Jensen, G. Hagen, T. Papenbrock et al, Phys. Rev. C, 82:014310 (2010)
    [82] F. Flavigny, Dtermination de facteurs spectroscopiques absolus par ractions de knockout et de transfert, Ph. D. Thesis (Universit Paris-Sud 6, 2011) (in French)
    [83] P. C. Srivastava and V. Kumar, Phys. Rev. C, 94:064306 (2016)
    [84] M. B. Tsang, Jenny Lee, and W. G. Lynch, Phys. Rev. Lett., 95:222501 (2005)
    [85] F. Beck, D. Frekers, P. von Neumann-Cosel et al, Phys. Lett. B, 645:128-132 (2007)
    [86] Jenny Lee, M. B. Tsang and W. G. Lynch, Phys. Rev. C, 75:064320 (2007)
    [87] M. B. Tsang, Jenny Lee, S. C. Su et al, Phys. Rev. Lett., 102:062501 (2009)
    [88] Sh. Hamada, N. Burtebayev, and N. Amangeldi, Int. J. Mod. Phys. E, 23:1450061 (2014)
    [89] N. Burtebayev, J. T. Burtebayeva, A. Duisebayev et al, Acta Phys. Pol. B, 46:1037-1054 (2015)
    [90] Vishal Srivastava, C. Bhattacharya, T. K. Rana et al, Phys. Rev. C, 93:044601 (2016)
    [91] F. Wang, B. H. Sun, Z. Liu et al, Phys. Lett. B, 770:83-87 (2017)
    [92] M. Horoi, J. Phys.:Conf. Ser., 413:012020 (2013)
    [93] P. O. Hess, A. Algora, J. Cseh et al, Phys. Rev. C, 70:051303 (R) (2004)
    [94] N. K. Timofeyuk, Phys. Rev. C, 88:044315 (2013)
    [95] H. T. Fortune and R. Sherr, Phys. Rev. C, 85:027305 (2012)
    [96] N. V. Gnezdilov, E. E. Saperstein, and S. V. Tolokonnikov, Phys. Atom. Nucl., 78:27-37 (2015)
    [97] E. Baranger and T. T. S. Kuo, Nucl. Phys. A, 97:289-297 (1967)
    [98] S. Aberg, P. B. Semmes and W. Nazarewicz, Phys. Rev. C, 56:1762-1773 (1997)
    [99] C. Basu, Pramana J. Phys., 63:1047-1052 (2004)
    [100] J. M. Yao, B. Sun, P. J. Woods et al, Phys. Rev. C, 77:024315 (2008)
    [101] H. F. Zhang, Y. J. Wang, J. M. Dong et al, J. Phys. G:Nucl. Part. Phys., 37:085107 (2010)
    [102] K. Kumar, J. B. Gupta, and J. H. Hamilton, Nucl. Phys. A, 448:36-44 (1986)
    [103] Y. Benbouzid, N. H. Allal, and M. Fellah, Rom. Journ. Phys., 61:424-434 (2016)
    [104] R. R. Chasman, Phys. Lett. B, 524:81-86 (2002)
    [105] R. W. Richardson, and N. Sherman, Nucl. Phys., 52:253-268 (1964)
    [106] R. D. Woods and D. S. Saxon, Phys. Rev., 95:577-578 (1954)
    [107] N. H. Allal and M. Fellah, Phys. Rev. C, 50:1404-1411 (1994)
    [108] S. Goriely, F. Tondeur, and J. M. Pearson, Atom. Data Nucl. Data Tables, 77:311-381 (2001)
    [109] P. Moller, J. R. Nix, W. D. Myers et al, Atom. Data Nucl. Data Tables, 59:185-381 (1995)
    [110] M. Wang, G. Audi, A. H. Wapstra et al, Chin. Phys. C, 36:1603 (2012)
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Y. Benbouzid, N. H. Allal, M. Fellah and M. R. Oudih. Influence of isovector pairing and particle-number projection effects on spectroscopic factors for one-pair like-particle transfer reactions in proton-rich even-even nuclei[J]. Chinese Physics C, 2018, 42(4): 044103. doi: 10.1088/1674-1137/42/4/044103
Y. Benbouzid, N. H. Allal, M. Fellah and M. R. Oudih. Influence of isovector pairing and particle-number projection effects on spectroscopic factors for one-pair like-particle transfer reactions in proton-rich even-even nuclei[J]. Chinese Physics C, 2018, 42(4): 044103.  doi: 10.1088/1674-1137/42/4/044103 shu
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Influence of isovector pairing and particle-number projection effects on spectroscopic factors for one-pair like-particle transfer reactions in proton-rich even-even nuclei

Abstract: Isovector neutron-proton (np) pairing and particle-number fluctuation effects on the spectroscopic factors (SF) corresponding to one-pair like-particle transfer reactions in proton-rich even-even nuclei are studied. With this aim, expressions of the SF corresponding to two-neutron stripping and two-proton pick-up reactions, which take into account the isovector np pairing effect, are established within the generalized BCS approach, using a schematic definition proposed by Chasman. Expressions of the same SF which strictly conserve the particle number are also established within the Sharp-BCS (SBCS) discrete projection method. In both cases, it is shown that these expressions generalize those obtained when only the pairing between like particles is considered. First, the formalism is tested within the Richardson schematic model. Second, it is applied to study even-even proton-rich nuclei using the single-particle energies of a Woods-Saxon mean-field. In both cases, it is shown that the np pairing effect and the particle-number projection effect on the SF values are important, particularly in N=Z nuclei, and must then be taken into account.

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