×
近期发现有不法分子冒充我刊与作者联系,借此进行欺诈等不法行为,请广大作者加以鉴别,如遇诈骗行为,请第一时间与我刊编辑部联系确认(《中国物理C》(英文)编辑部电话:010-88235947,010-88236950),并作报警处理。
本刊再次郑重声明:
(1)本刊官方网址为cpc.ihep.ac.cn和https://iopscience.iop.org/journal/1674-1137
(2)本刊采编系统作者中心是投稿的唯一路径,该系统为ScholarOne远程稿件采编系统,仅在本刊投稿网网址(https://mc03.manuscriptcentral.com/cpc)设有登录入口。本刊不接受其他方式的投稿,如打印稿投稿、E-mail信箱投稿等,若以此种方式接收投稿均为假冒。
(3)所有投稿均需经过严格的同行评议、编辑加工后方可发表,本刊不存在所谓的“编辑部内部征稿”。如果有人以“编辑部内部人员”名义帮助作者发稿,并收取发表费用,均为假冒。
                  
《中国物理C》(英文)编辑部
2024年10月30日

Nuclear structure and decay modes of Ra isotopes within an axially deformed relativistic mean field model

  • We examine the structural properties and half-life decay of Ra isotopes within the axially deformed Relativistic Mean-Field (RMF) theory with NL3 force parameters. We work out the binding energy (BE), RMS radii, two-neutron separation energies (S2n), and some other observables. The results are in good agreement with the finite-range droplet model (FRDM) and experimental results. Considering the possibility of neutron magic number, the α-decay and cluster decay half-lives of Ra isotopes are calculated systematically using the Q-values obtained from the RMF formalism. These decay half-life calculations are carried out by taking three different empirical formulae. The calculated decay half-lives are found to be highly sensitive to the choice of Q-values. Possible shell or sub-shell closures are found at daughter nuclei with N=128 and N=126 when alpha and 8Be, 12C, 18O respectively are emitted from Ra isotopes. Though the cluster radioactivity is affected by the shell closure of parent and daughter, a long half-life indicates the stability of the parent, and a small parent half-life indicates that the shell stability of the daughter against decay.
      PCAS:
  • 加载中
  • [1] A. STndulescu, D. N. Poenaru, and W. Greiner, Sov. J. Part. Nucl., 11:528 (1980)
    [2] D. N. Poenaru, M. Ivascu, A. Sandulescu, and W. Greiner, J. Phys. G:Nucl. Part. Phys., 10:L183 (1984)
    [3] D. N. Poenaru, M. Ivascu, A. Sandulescu, and W. Greiner, Phys. Rev. C, 32:572 (1985)
    [4] D. N. Poenaru, W. Greiner, A. Sandulescu, and M. Ivascu, Phys. Rev. C, 32:2198 (1985)
    [5] W. Greiner, M. Ivascu, D. N. Poenaru, and A. Sandulescu, Z. Phys. A, 320 347 (1985)
    [6] Y. J. Shi and W. J. Swiatecki, Phys. Rev. Lett., 54:300 (1985)
    [7] G. A. Pik-Pichak and Sov. J. Nucl. Phys., 44:923 (1986)
    [8] G. Shanmugam and B. Kamalaharan, Phys. Rev. C, 38:1377 (1988)
    [9] B. Buck, A. C. Merchant, J. Phys. G:Nucl. Part. Phys., 15:615 (1989)
    [10] K. P. Santhosh, A. Joseph, Ind. J. of Pure App. Phys., 42:806 (2004)
    [11] K. P. Santhosh, A. Joseph, Pramana J. Phys., 55:375 (2000)
    [12] S. Landowne, C. H. Dasso, Phys. Rev. C, 33:387 (1986)
    [13] M. Iriondo, D. Jerrestan, and R. J. Liotta, Nucl. Phys. A, 454:252 (1986)
    [14] R. Blendoaske, T. Fliessbach, and H. Walliser, Nucl. Phys. A, 464:(75) (1987)
    [15] S. S. Malik, R. K. Gupta, Phys. Rev. C, 39:1992 (1989)
    [16] S. Kumar, R. K. Gupta, Phys. Rev. C, 55:218 (1997)
    [17] D. N. Poenaru, W. Greiner, in:C. Beck (Ed.), Clusters in Nuclei, in:Lecture Notes in Physics, vol., 818:Springer, Berlin, p. 1 (2010)
    [18] H. J. Krappe, K. Pomorski, in:Theory of Nuclear Fission:A Textbook, in:Lecture Notes in Physics, vol., 838:Springer, Berlin, p. 233 (2010)
    [19] D. N. Poenaru, R. A. Gherghescu, W. Greiner, Phys. Rev. Lett., 107:062503 (2011)
    [20] D. Ni, Z. Ren, T. Dong, C. Xu, Phys. Rev. C, 78:044310 (2008)
    [21] Z. Ren, C. Xu, Z. Wang, Phys. Rev. C, 70:034304 (2004).
    [22] D. Ni, Z. Ren, Phys. Rev. C, 82:024311 (2010)
    [23] S. Hofmann et al, Eur. Phys. J. A, 10:5 (2001)
    [24] Yu. Ts. Oganessian et al, Phys. Rev. C, 74:044602 (2006); Phys, Rev, C, 70:064609 (2004)
    [25] G. Gamow, Z. Phys., 51:204 (1928)
    [26] E. U. condon, R. W. Gurney, Nature, 122:439 (1928)
    [27] H. Geiger, J. M. Nuttall, Philos. Mag., 22:613 (1911)
    [28] A. Sandulescu, D. N. Poenaru, W. Greiner, and J. H. Hamilton, Phys. Rev. Lett., 54:490 (1985)
    [29] H. J. Rose and G. A. Jones, Nature, 307:245 (1984)
    [30] S. Gales et al, Phys. Rev. Lett., 53:759 (1984)
    [31] P. B. Price et al, Phys. Rev. Lett., 54:297 (1985)
    [32] L. P. Gaffney et al, Nature, 497:199 (2013)
    [33] S. K. Ghorui, B. B. Sahu, C. R. Praharaj, and S. K. Patra, Phys. Rev. C, 85:064327 (2012)
    [34] B. B. Sahu, S. K. Singh, S. K. Patra, C. R. Praharaj, M. Bhuyan, Z. Naik, and S. K. Ghorui, Acta Physica. Polo. B, 43:451 (2012)
    [35] B. D. Serot and J. D. Walecka, Adv. Nucl. Phys., 16:1 (1986)
    [36] Y. K. Gambhir, P. Ring, and A. Thimet, Ann. Phys. (NY), 198:132 (1990)
    [37] H. Toki, Y. Sugahara, D. Hirata, B. V. Carlson, and I.Tanihata, Nucl. Phys. A, 524:633 (1991)
    [38] C. Qi, F.R. Xu, R. J. Liotta, R. Wyss, M. Y. Zhang, C. Asawatangtrakuldee, and D. Hu, Phys. Rev. C, 80:044326 (2009)
    [39] Z. Sheng, D. Ni, and Z. Ren, J. Phys. G, Nucl. Part. Phys., 38:055103 (2011)
    [40] T. T. Ibrahim, S. M. Perez, S. M. Wyngaardt, B. Buck, and A. C. Merchant, Phys. Rev. C, 85:044313 (2012) 062503 (2011).
    [41] M. Balasubramaniam, R. K. Gupta, Phys. Rev. C, 60:064316 (1999)
    [42] J. L. Egido, L. M. Robledo, Nucl. Phys. A, 738:31 (2004)
    [43] L. M. Robledo, M. Warda, Int. J. Mod. Phys. E, 17:204 (2008)
    [44] L. M. Robledo, M. Warda, Int. J. Mod. Phys. E, 17:2275 (2008)
    [45] B. Buck, A. C. Merchant, and S. M. Perez, Nucl. Phys. A, 657:267 (1999)
    [46] K. P. Santhosh, R. K. Biju, and A. Joseph, J. Phys. G, Nucl. Part. Phys., 35:085102 (2008)
    [47] K. P. Santhosh, S. Sahadevan, B. Priyanka, and M. S. Unnikrishnan, Nucl. Phys. A, 882:49 (2012)
    [48] K. P. Santhosh, R. K. Biju, S. Sahadevan, and A. Joseph, Phys. Scr., 77:065210 (2008)
    [49] K. P. Santhosh, Phys. Scr., 81:015203 (2010)
    [50] D. N. Poenaru, R. A. Gherghescu, and W. Greiner, Phys. Rev. C, 83:014601 (2011)
    [51] S. S. Malik, R. K. Gupta, Phys. Rev. C, 39:1992 (1989)
    [52] D. N. Basu, Phys. Rev. C, 66:027601 (2002)
    [53] R. K. Gupta, S. Singh, R. K. Puri, W. Scheid, Phys. Rev. C, 47:561 (1993)
    [54] S. Kumar, R. K. Gupta, Phys. Rev. C, 49:1922 (1994)
    [55] K. P. Santhosh, S. Sahadevan, B. Priyanka, and M. S. Unnikrishnan, Nucl. Phys. A, 882:49 (2012)
    [56] T. R. Routray, J. Nayak, and D. N. Basu, Nucl. Phys. A, 826:223 (2009)
    [57] G. Sawhney, M. K. Sharma, R. K. Gupta, Phys. Rev. C, 83:064610 (2011)
    [58] A. Soylu, Y. Sert, O. Bayrak, and I. Boztosun, Eur. Phys. J. A, 48:128 (2012)
    [59] K. P. Santhosh, A. Joseph, and Pramana J. Phys., 59:679-684 (2002)
    [60] A. Soylu and S. Evlice, Nucl. Phys. A, 936:59 (2015)
    [61] K. P. Santhosh, T. Ambily, S. Sabina, R. K. Biju, and A. Joseph, Proc. Nat. Symp. Nucl. Phys. (India), 1:33 (2009)
    [62] K. P. Santhosh, S. Sabina, B. Priyanka, M. S. Unnikrishnan, G. J. Jayesh, and R. K. Biju, Proc. DAE Symp. Nucl. Phys. (India), 56:298 (2011)
    [63] G. A. Lalazissis et al, Phys. Rev. C, 55:540 (1997)
    [64] B. G. Todd-Rutel et al, Phys. Rev. Lett., 95:122501 (2005)
    [65] V. E. Viola, Jr. and G. T. Seaborg, J. Inorg. Nucl. Chem., 28:741 (1966)
    [66] G. Royer, Nucl. Phys. A, 848:279 (2010)
    [67] J. M. Dong, et al, Nucl. Phys. A, 832:198 (2010)
    [68] C. Qi, F. R. Xu, R. J. Liotta, and R. Wyss, Phys. Rev. Lett., 103:072501 (2009)
    [69] C. Qi, F. R. Xu, R. J. Liotta, R. Wyss, M. Y. Zhang, C. Asawatangtrakuldee, and D. Hu, Phys. Rev. C, 80:044326 (2009)
    [70] L. I. Schiff, Phys. Rev., 84:1 (1951)
    [71] M. H. Johnson and E. Teller, Phys. Rev., 98:783 (1955)
    [72] H. P. Durr and E. Teller, Phys. Rev., 101:494 (1956)
    [73] J. D. Walecka, Ann. Phys. (N.Y.), 83:491 (1974)
    [74] C. J. Horowitz, and B. D. Serot, Nucl. Phys. A, 368:503 (1981)
    [75] T. Gonzales-Llarena, J. L. Egido, G. A. Lalazissis, and P. Ring, Phys. Lett. B, 379:13 (1996)
    [76] W. Pannert, P. Ring, and J. Boguta, Phys. Rev. Lett., 59:2420 (1986)
    [77] Y. K. Gambhir, P. Ring, and A. Thimet, Ann. Phys. (N.Y.), 198:132 (1990)
    [78] J. Boguta, A. R. Bodmer, Nucl. Phys. A, 292:413 (1977)
    [79] S. K. Patra and C. R. Praharaj, Phys. Rev. C, 44:552 (1991)
    [80] M. Del Estal, M. Centelles, X. Vinas, and S. K. Patra, Phys. Rev. C 63:024314 (2001)
    [81] G. Gangopadhyay, Phys. Rev. C, 59:2541 (1999)
    [82] G. A. Lalazissis and S. Raman, Phys. Rev. C, 58:1467 (1998)
    [83] J. Meng et al, Prog. Part. Nucl. Phys., 57:470 (2006)
    [84] J. Konig, and P. Ring, Phys. Rev. Lett., 71:3079 (1993)
    [85] Z. Z. Ren, Phys. Rev. C, 65:051304(R) (2002)
    [86] S. Das and G. Gangopadhyay, J. Phys. G:Nucl. Part. Phys. 30:957 (2004)
    [87] H. F. Zhang et al, Phys. Rev. C, 71:054312 (2005)
    [88] J. Q. Li et al, Phys. Rev. C, 65:064305 (2002)
    [89] Renli Xu, Chen Wu, and Zhongzhou Ren, J. Phys. G:Nucl. Part. Phys., 39:085107 (2012)
    [90] Renli Xu, Chen Wu, Guoliang Ma, Deqing Fang, and Zhongzhou Ren Phys. Rev. C, 87:014335 (2012)
    [91] B. B. Sahu, S. K. Agarwalla, and S. K. Patra, Phys. Rev. C, 84:054604 (2011)
    [92] D. G. Madland and J. R. Nix, Nucl. Part. Phys. A, 476:1 (1981)
    [93] P. Moller and J. R. Nix, At. Data Nucl. Data Tables 39:213 (1988)
    [94] G. A. Lalazissis, et al., Phys. Rev. C, 60:014310 (1999)
    [95] A. Sobiczewski, Z. Patyk, S. Cwiok, Phys. Lett. B, 224:1 (1989)
    [96] A. M. Lane and R. G. Thomas, Rev. Mod. Phys., 30:257 (1958)
    [97] R. G. Lovas, R. J. Liotta, A. Insolia, K. Varga, and D. S. Delion, Phys. Rep., 294:265 (1998)
    [98] D. S. Delion, R. J. Liotta, and R. Wyss, Phys. Rev. Lett., 96:072501 (2006)
    [99] C. Qi, F. R. Xu, R. J. Liotta, and R. Wyss, Phys. Rev. Lett., 103:072501 (2009)
    [100] G. Royer, J. Phys. G. Nucl. Part. Phys., 26:1149 (2000)
    [101] P. Mller, J. R. Nix, W. D. Wyers, and W. J. Swiaterecki, At.Data and Nucl. Data Tables, 59:(1995) 185; P. Mller, J. R. Nix, and K. -L. Kratz, At. Data and Nucl. Data Tables, 66:1318 (1997)
    [102] S.Iversen, H.Nann, A.ObstKamal, K.Seth, N.Tanaka, C.L.Morris, H.A.Thiessen, K.Boyer, W.Cottingame, C.Fred Moore, R.L.Boudrie, D.Dehnhard, Phys, Lett, B, 82:51 (1979)
    [103] W. Hirt, Nuclear Physics B, 9:447, (1969)
    [104] B. Sahu et. al., Phy. Rev. C, 77:024604 (2008)
    [105] S.A. Changizi, C. Qi, Nucl. Phys. A, 951:97 (2016)
    [106] F. Iachello, and N. V. Zamfir, Phys Rev. Lett., 92:212501 (2004)
    [107] Bidhubhusan Sahu, S. K. Agarwalla, and S. K. Patra, Phys. Rev. C, 84:054604 (2011)
    [108] R. D. Page et al., Phys. Rev. C, 75:061302(R) (2007)
    [109] G. Audi, A. H. Wapstra, C. Thivault, Nucl. Phys. A, 729:337 (2003)
  • 加载中

Get Citation
Rashmirekha Swain, S. K. Patra and B. B. Sahu. Nuclear structure and decay modes of Ra isotopes within an axially deformed relativistic mean field model[J]. Chinese Physics C, 2018, 42(8): 084102. doi: 10.1088/1674-1137/42/8/084102
Rashmirekha Swain, S. K. Patra and B. B. Sahu. Nuclear structure and decay modes of Ra isotopes within an axially deformed relativistic mean field model[J]. Chinese Physics C, 2018, 42(8): 084102.  doi: 10.1088/1674-1137/42/8/084102 shu
Milestone
Received: 2018-04-22
Fund

    Supported by Project No. SR/FTP/PS-106/2013, SERB, DST, Govt. of India

Article Metric

Article Views(1679)
PDF Downloads(27)
Cited by(0)
Policy on re-use
To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.
通讯作者: 陈斌, bchen63@163.com
  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Email This Article

Title:
Email:

Nuclear structure and decay modes of Ra isotopes within an axially deformed relativistic mean field model

  • 1.  School of Applied Sciences, KⅡT Deemed to be University, Bhubaneswar-751024, Odisha, India
  • 2.  Institute of Physics, Bhubaneswar-751005, India
Fund Project:  Supported by Project No. SR/FTP/PS-106/2013, SERB, DST, Govt. of India

Abstract: We examine the structural properties and half-life decay of Ra isotopes within the axially deformed Relativistic Mean-Field (RMF) theory with NL3 force parameters. We work out the binding energy (BE), RMS radii, two-neutron separation energies (S2n), and some other observables. The results are in good agreement with the finite-range droplet model (FRDM) and experimental results. Considering the possibility of neutron magic number, the α-decay and cluster decay half-lives of Ra isotopes are calculated systematically using the Q-values obtained from the RMF formalism. These decay half-life calculations are carried out by taking three different empirical formulae. The calculated decay half-lives are found to be highly sensitive to the choice of Q-values. Possible shell or sub-shell closures are found at daughter nuclei with N=128 and N=126 when alpha and 8Be, 12C, 18O respectively are emitted from Ra isotopes. Though the cluster radioactivity is affected by the shell closure of parent and daughter, a long half-life indicates the stability of the parent, and a small parent half-life indicates that the shell stability of the daughter against decay.

    HTML

Reference (109)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return