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《中国物理C》(英文)编辑部
2024年10月30日

Magnetic moments of octet baryons in hot and dense nuclear matter

  • We have calculated the in-medium magnetic moments of octet baryons in the presence of hot and dense symmetric nuclear matter. Effective magnetic moments of baryons have been derived from medium modified quark masses within the chiral SU(3) quark mean field model. Further, for better insight into the medium modification of baryonic magnetic moments, we have considered the explicit contributions from the valence quarks, sea quarks and the sea orbital angular momentum of sea quarks. These effects have been successful in giving the description of baryonic magnetic moments in vacuum. The magnetic moments of baryons are found to vary significantly as a function of density of nuclear medium.
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  • [1] J. Beringer et al, Phys. Rev. D, 86:010001(2012)
    [2] J. Ashman et al (EMC Collaboration), Phys. Lett. B, 206:364(1988); J. Ashman et al (EMC Collaboration), Nucl. Phys. B, 328:1(1989)
    [3] V. Friese, Nucl. Phys. A,774:377(2005)
    [4] Johann M. Heuser, Nucl. Phys. A, 830:563(2009)
    [5] G. Aad et al, Phys. Rev. D, 89:092009(2014)
    [6] P. Senges, Acta Physica Polonica B, 37:1(2006)
    [7] S. Sahu, Revista Mxicana De Fisica, 48:48(2002)
    [8] F. Schlumpf, Phys. Rev. D, 48:4478(1993),
    [9] W. R. B. de Araujo et al, Brazilian Journal of Physics, 34:871(2004)
    [10] E. J. Hackett-Jones, D. B. Leinweber, and A. W. Thomas, Phys. Lett. B, 489:143(2000)
    [11] J. G. Contreras, R. Huerta, Revista Mxicana De Fisica, 50:490(2004)
    [12] H. E. Jun, Dong Yu-Bing, Commun. Theor. Phys., 43:139(2005)
    [13] Lalit K. Sharma, C. Mai, J. Sci., 34:13(2007)
    [14] T. P. Cheng and Ling Fong Li, Phys. Rev. Lett., 74:2872(1995)
    [15] J. Linde, T. Ohlsson, and H. Snellman, Phys. Rev. D, 57:092009(1998)
    [16] T. Draper, Keh-Fei Liu, Nucl. Phys. A, 527:531(1991)
    [17] D. B. Leinweber, R. M. Woloshyn, Nucl. Phys. B, Proc. Suppl., 20:463(1991)
    [18] M. Z. Navgran, Maryam, Int. Sci. index, 59:1174(2011)
    [19] C. Y. Ryu, M. K. Cheoun, and C. H. Hyun, Journal of Korean Physical Society, 54:1448(2009)
    [20] B. O. Kerbikov, Yu. A. Simonov, Phys. Rev. D, 62:093016(2000).
    [21] L. S. Geng, J. M. Camalich, L. A. Ruso, and M. J. Vincente Vacas, Phys. Rev. Lett., 101:222002(2008)
    [22] L. S. Geng, J. M. Camalich, and M. J. Vincente Vacas, Phys. Rev. D, 80:034027(2009)
    [23] J. Gasser, H. Leutwyler, Nucl. Phys. B, 250:465(1985)
    [24] J. Gasser, M. E. Sainio and A. Svarc, Nucl. Phys. B, 307:779(1988)
    [25] S. Scherer, Adv. Nucl. Phys., 27:277(2003)
    [26] E. E. Jenkins et al, Phys. Lett. B, 302:482(1993)
    [27] L. Durand, P. Ha, Phys. Rev. D, 58:013010(1998)
    [28] S. J. Puglia, M. J. Ramsey-Musolf, Phys. Rev. D, 62:034010(2000)
    [29] U. G. Meissner, S. Steininger, Nucl. Phys. B, 499:349(1997)
    [30] J. J. Aubert et al, Phys. Lett. B, 123:275(1983)
    [31] P. J. Mulders, Phys. Reports, 185:83(1990)
    [32] J. D. Walecka, Ann. Phys. (N. Y.), 83:491(1974)
    [33] N. Petropoulas, arxiv:hep-ph/0402136
    [34] P. Wang et al, Phys. Rev. C, 70:015202(2004)
    [35] H. Q. Song, R. K. Su, Phys. Lett. B, 358:179(1995)
    [36] G. A. Miller, Phys. Rev. C, 66:032201(2002)
    [37] M. Buballa, Phys. Rept., 407:205(2005)
    [38] Gustavo A. Contera, Phys. Lett. B, 661:113(2008)
    [39] P. Rau et al, J. Phys. G:Nucl. Part. Phys., 40:085001(2013)
    [40] T. Hatsuda, T. Kunihiro, Phys. Rept., 247:221(1994)
    [41] P. Wang, Z. Zong-Ye and Y. You-Wen, Commun. Theor. Phys., 36:71(2001)
    [42] H. Shen and H. Toki, Phys. Rev. C, 61:045205(2000)
    [43] P. Papazoglou, D. Zschiesche, S. Schramm, J. Schaffner-Bielich, H. Stcker, and W. Greiner, Phys. Rev. C, 59:411(1999)
    [44] M. A. Thaler, R. A. Schneides, W. weise, Phys. Rev. C, 69:035210(2003)
    [45] R. F. Wagenbrunn et al, Phys. Rev. B, 33:511(2001)
    [46] S. Capstick, B. D. Keister, arXiv:nucl-th/9611055
    [47] J. Linde, T. Ohlsson, and Hakan Snellman, Phys. Rev. D, 57:452(1998)
    [48] C. Y. Ryu, C. H. Hyun, T. S. Park, and S. W. Hong, Phys. Lett. B, 674:122(2009)
    [49] H. J. Lipkin, arxiv:hep-ph/9911261
    [50] S. Weinberg, Physica A, 96:327(1979)
    [51] A. Manohar, H. Georgi, Nucl. Phys. B, 234:189(1984)
    [52] P. Wang, Z. Y. Song et al, Nucl. Phys. A, 688:791(2001)
    [53] P. Wanget al, Nucl. Phys. A, 744:273(2004)
    [54] H. Dahiya, M. Gupta, Phys. Rev. D, 64:014013(2001)
    [55] T. P. Cheng, L. F. Li, Phys. Rev. Lett., 80:2789(1998)
    [56] T. P. Cheng, Ling Fong Li, Phys. Rev. D, 57:344(1998)
    [57] M. Gupta, N. Kaur, Phys. Rev. D, 28:534(1983)
    [58] A. Gridhar, H. Dahiya, M. Randhawa, Phys. Rev. D, 92(3):033012(2015)
    [59] Ikuo S. Sogami, N. Oh'yamaguchi, Phys. Rev. Lett., 54:2295(1985); Kuang-Ta Chao, Phys. Rev. D, 41:920(1990)
    [60] C. V. Christov, E. R. Arriola, and K. Goeke, Nucl. Phys. A, 556:641(1993); M. Arneodo et al, Phys. Rev. D, 50:R1(1994)
    [61] M. Abu-Shady, A. K. Abu-Nab, American Journal of Physics and App., 46:1(2014)
    [62] J. W. Holt, M. Rho, and W. Weise, arxiv:1411.6681v2[nucl-th]
    [63] S. Theberge and A. W. Thomas, Phys. Rev. D, 25:284(1982); J. Cohen and H.J. Weber, Phys. Lett. B, 165:229(1985)
    [64] L. Durand and P. Ha, Phys. Rev. D, 58:013010(1998)
    [65] C. Y. Ryu and K. S. Kim, Phys. Rev. C, 82:025804(2010)
    [66] N. Barik, B. K. Dash, Phys. Rev. D, 31:7(1985)
    [67] T. P. Cheng and L. F. Li, Phys. Rev. Lett., 74:2872(1995); T. P. Cheng and L. F. Li, Phys. Rev. D, 59:097503(1999); X. Song and V. Gupta, Phys. Rev. D, 49:2211(1994)
    [68] N. Barik et al, Phys. Rev. C, 88:015206(2013)
    [69] P. Wang et al, Phys. Rev. C, 72:045801(2005)
    [70] A. Mishra et al, Eur. Phys, J. A, 41:205(2009); 98:631(1997)
    [71] M. Gupta, J. Phys. G, 16:L213(1990)
    [72] A. J. Buchmann, E. M. Henley, Phys. Rev. D, 83:096011(2010)
    [73] L. M. Sehgal, Phys. Rev. D, 10:1663(1974)
    [74] X. Ji, Phys. Rev. Lett., 78:610(1997).
    [75] J. M. S. Rana, H. Dahiya, M. Gupta, AIP Conference Proceedings, 63:1056(2008)
    [76] A. W. Thomas, Int. J. Mod. Phys. E, 18:1116(2009)
    [77] S. J. Brodsky, S. Gardner, Phys. Lett. B, 643:22(2006)
    [78] H. Dahiya, M. Randhawa, Phys. Rev. D, 93:114030(2016)
    [79] X. Song, arxiv:hep-ph/0012295v3
    [80] L. F. Li and T. P. Cheng, Chinese Journal of Physics, 35:6(1997)
    [81] L. F. Li and T. P. Cheng, Phys. Rev. Lett., 74:15(1995)
    [82] New Muon Collaboration, P. Amaudruz et al:Phys. Rev. Lett., 66:2712(1991)
    [83] L. Ya. Glozman, D. O. Riska, Phys. Lett. B, 459:49(1999)
    [84] L. F. Li and T. P. Cheng, arxiv:hep-ph/9709293
    [85] W-M Yao, C. Amsler, D. Asner et al, Particle Data Group. J. Phys. G, 33:1(2006)
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Harpreet Singh, Arvind Kumar and Harleen Dahiya. Magnetic moments of octet baryons in hot and dense nuclear matter[J]. Chinese Physics C, 2017, 41(9): 094104. doi: 10.1088/1674-1137/41/9/094104
Harpreet Singh, Arvind Kumar and Harleen Dahiya. Magnetic moments of octet baryons in hot and dense nuclear matter[J]. Chinese Physics C, 2017, 41(9): 094104.  doi: 10.1088/1674-1137/41/9/094104 shu
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Received: 2017-04-24
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Magnetic moments of octet baryons in hot and dense nuclear matter

Abstract: We have calculated the in-medium magnetic moments of octet baryons in the presence of hot and dense symmetric nuclear matter. Effective magnetic moments of baryons have been derived from medium modified quark masses within the chiral SU(3) quark mean field model. Further, for better insight into the medium modification of baryonic magnetic moments, we have considered the explicit contributions from the valence quarks, sea quarks and the sea orbital angular momentum of sea quarks. These effects have been successful in giving the description of baryonic magnetic moments in vacuum. The magnetic moments of baryons are found to vary significantly as a function of density of nuclear medium.

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