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《中国物理C》(英文)编辑部
2024年10月30日

Ground-state properties of light kaonic nuclei signaling symmetry energy at high densities

  • A sensitive correlation between the ground-state properties of light kaonic nuclei and the symmetry energy at high densities is constructed under the framework of relativistic mean-field theory. Taking oxygen isotopes as an example, we see that a high-density core is produced in kaonic oxygen nuclei, due to the strongly attractive antikaon-nucleon interaction. It is found that the 1S1/2 state energy in the high-density core of kaonic nuclei can directly probe the variation of the symmetry energy at supranormal nuclear density, and a sensitive correlation between the neutron skin thickness and the symmetry energy at supranormal density is established directly. Meanwhile, the sensitivity of the neutron skin thickness to the low-density slope of the symmetry energy is greatly increased in the corresponding kaonic nuclei. These sensitive relationships are established upon the fact that the isovector potential in the central region of kaonic nuclei becomes very sensitive to the variation of the symmetry energy. These findings might provide another perspective to constrain high-density symmetry energy, and await experimental verification in the future.
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  • [1] C. Xu and B. A. Li, Phys. Rev. C, 81:064612 (2010)
    [2] M. B. Tsang et al, Phys. Rev. C, 86:015803 (2012)
    [3] A. W. Steiner, and S. Gandolfl, Phys. Rev. Lett., 108:081102 (2012)
    [4] P. Wang and W. Zuo, Chinese Phys. C, 39:014101 (2015)
    [5] B. A. Li, W. J. Guo, and Z. Z. Shi, Phys. Rev. C, 91:044601 (2015)
    [6] O. Hen, B. A. Li, W. J. Guo, L. B. Weinstein, and E. Piasetzky, Phys. Rev. C, 91:025803 (2015)
    [7] B. J. Cai, B. A. Li, and L. W. Chen, Phys. Rev. C, 94:061302(R) (2016)
    [8] L. W. Chen, C. M. Ko, and B. A. Li, Phys. Rev. Lett., 94:032701 (2005)
    [9] F. zel, Nature, 441:1115 (2006)
    [10] B. A. Li, L. W. Chen, and C. M. Ko, Phys. Rep., 464:113 (2008)
    [11] M. B. Tsang, Y. X. Zhang, P. Danielewicz, M. Famiano, Z. X. Li, W. G. Lynch, and A. W. Steiner, Phys. Rev. Lett., 102:122701 (2009)
    [12] C. Xu, B. A. Li, and L. W. Chen, Phys. Rev. C, 82:054607 (2010)
    [13] A. Carbone, G. Colo, A. Bracco, L. G. Cao, P. F. Bortignon, F. Camera, and O. Wieland, Phys. Rev. C, 81:041301(R) (2010)
    [14] A. W. Steiner, J. M. Lattimer, and E.F. Brown, Astrophys. J., 722:33 (2010)
    [15] M. Zhang, Z. G. Xiao, and S. J. Zhu, Chinese Phys. C, 34:1100 (2010)
    [16] Z. Zhang and L.-W. Chen, Phys. Lett. B, 726:234 (2013)
    [17] X. H. Li, B. J. Cai, L. W. Chen, R. Chen, B. A. Li, and C. Xu, Phys. Lett. B, 721:101 (2013)
    [18] C. W. Ma, H. L. Song, J. Pu, T. L. Zhang, S. Zhang, S. S. Wang, X. L. Zhao, and L. Chen, Chinese Phys. C, 37:024102 (2013)
    [19] Y. F. Guo, P. H. Chen, F. Niu, H. F. Zhang, G. M. Jin, and Z. Q. Feng, Chinese Phys. C, 41:104104 (2017)
    [20] A. L. Watts et al, Rev. Mod. Phys., 88:021001 (2016)
    [21] J. M. Lattimer and M. Prakash, Phys. Rep., 621:127 (2016)
    [22] Z. Xiao, B. A. Li and L. W. Chen, G.C. Yong, M. Zhang, Phys. Rev. Lett., 102:062502 (2009)
    [23] Z. Q. Feng and G. J. Ming, Phys. Lett. B, 683:140 (2010)
    [24] P. Russotto, W. Trauntmann, Q. F. Li et al, Phys. Lett. B, 697:471 (2011)
    [25] W. Z. Jiang, Phys. Rev. C, 81:044306 (2010)
    [26] N. Wang, M. Liu, and X. Z. Wu, Phys. Rev. C, 81:044322 (2010)
    [27] M. Liu, N. Wang, Z. X. Li, and F. S. Zhang, Phys. Rev. C, 82:064306 (2010)
    [28] J. L. Tian, H. T. Cui, T. Gao, and N. Wang, Chinese Phys. C, 40:094101 (2016)
    [29] N. Wang, M. Liu, L. Ou, and Y. X. Zhang, Phys. Lett. B, 751:553 (2015)
    [30] J. Xu, L.W. Chen, B. A. Li, H. R. Ma, Phys. Lett. B, 650:348 (2007)
    [31] G. H. Zhang and W. Z. Jiang, Phys. Lett. B, 720:148 (2013)
    [32] C. J. Horowitz and J. Piekarewicz, Phys. Rev. Lett., 86:5647 (2001)
    [33] W. Z. Jiang, Y. L. Zhao, Phys. Lett. B, 617:33 (2005)
    [34] L. W. Chen, C. M. Ko, B. A. Li, and J. Xu, Phys. Rev. C, 82:024321 (2010)
    [35] Z. Zhang and L. W. Chen, Phys. Rev. C, 92:031301(R) (2015)
    [36] H. Jiang, N. Wang, L. W. Chen, Y. M. Zhao, and A. Arima, Phys. Rev. C, 91:054302 (2015)
    [37] A. Klimkiewicz et al, Phys. Rev. C, 76:051603(R) (2007)
    [38] X. Roca-Maza, M. Centelles, X. Vinas, and M. Warda, Phys. Rev. Lett., 106:252501 (2011)
    [39] S. Abrahamyan et al, Phys. Rev. Lett., 108:112502 (2012)
    [40] C. J. Horowitz, K. S. Kumar, and R. Michaels, Eur. Phys. J. A, 50:48 (2014)
    [41] C. M. Tarbert et al, Phys. Rev. Lett., 112:242502 (2014)
    [42] J. Schafiner, C. B. Dover, A. Gal, C. Greiner, and H. Stker, Phys. Rev. Lett., 71:1328 (1993)
    [43] J. Schafiner, C. B. Dover, A. Gal, C. Greiner, D. J. Millener, and H. Stker, Ann. Phys., 235:35 (1994)
    [44] W. Z. Jiang, Phys. Lett. B, 642:28 (2006)
    [45] T. Kishimoto, Phys. Rev. Lett., 83:4701 (1999)
    [46] T. Yamazaki and Y. Akaishi, Phys. Lett. B, 353:70 (2002)
    [47] Y. Akaishi and T. Yamazaki, Phys. Rev. C, 65:044005 (2002)
    [48] I. Tanihata, H. Hamagaki, O. Hashimoto et al, Phys. Rev. Lett., 55:2676 (1985)
    [49] M. V. Zhukov, B. V. Danilin, D. V. Fedorov et al, Phys. Rep., 231:151 (1993)
    [50] H. W. Hammer, A. Nogga, and A. Schwenk, Rev. Mod. Phys., 85:197 (2013)
    [51] W. von Oertzen, M. Freer, and Y. Kanada-En'yo, Phys. Rep., 432:43 (2006)
    [52] E. Epelbaum, H. Krebs, D. Lee, and Ulf-G. Meissner, Phys Rev. Lett., 106:192501 (2011)
    [53] T. Otsuka, T. Suzuki, M. Honma et al, Phys. Rev. Lett., 104:012501 (2010)
    [54] T. Otsuka, T. Suzuki, J. D. Holt, A. Schwenk, and Y. Akaishi, Phys. Rev. Lett., 105:032501 (2010)
    [55] T. Otsuka, R. Fujimoto, Y. Utsuno, B. A. Brown, M. Honma, T. Mizusaki Phys. Rev. Lett., 87:082502 (2001)
    [56] T. Otsuka, T. Suzuki, R. Fujimoto, H. Grawe, and Y. Akaishi, Phys. Rev. Lett., 95:232502 (2005)
    [57] O. Sorlin, M. G. Porquet, Prog. Part. Nucl. Phys., 61:602 (2008)
    [58] R. Y. Yang, W. Z. Jiang, D. R. Zhang, and S. N. Wei, Eur. Phys. J. A, 50:188 (2014)
    [59] R. Y. Yang, W. Z. Jiang, and S. N. Wei, Sci. Rep., 7:16695 (2017)
    [60] J. Mares, E. Friedman, and A. Gal, Nucl. Phys. A, 770:84 (2006)
    [61] X. H. Zhong, G. X. Peng, L. Li, and P. Z. Ning, Phys. Rev. C, 74:034321 (2006)
    [62] D. Gazda, E. Friedman, A. Gal, and J. Mares, Phys. Rev. C, 76:055204 (2007)
    [63] M. Agnello et al (FINUDA Collaboration), Phys. Rev. Lett., 94:212303 (2005)
    [64] V. K. Magas, E. Oset, A. Ramos, and H. Toki, Phys. Rev. C, 74:025206 (2006)
    [65] G. Bendiscioli, T. Bressani, A. Fontana et al, Nucl. Phys. A, 789:222 (2007)
    [66] T. Yamazaki et al (DISTO Collaboration), Phys. Rev. Lett., 104:132502 (2010)
    [67] S. Ajimura et al, Nucl. Phys. A, 914:315 (2013)
    [68] A. O. Tokiyasu et al (LEPS Collaboration), Phys. Lett. B, 728:616 (2014)
    [69] Y. Ichikawa et al, Prog. Theor. Exp. Phys., 2015:021D01 (2015)
    [70] A. Filippi and S. Piano, Hyperflne Interact., 233:151 (2015)
    [71] G. Agakishiev et al (HADES Collaboration), Phys. Lett. B, 742:242 (2015)
    [72] J. N. Ginocchio, Phys. Rev. Lett., 78:436 (1997)
    [73] H. Z. Liang, J. Meng, and S. G. Zhou, Phys. Rep., 570:1 (2015)
    [74] B. D. Serot and J. D. Walecka, Adv. Nucl. Phys., 16:1 (1986)
    [75] P. Ring, Prog. Part. Nucl. Phys., 37:193 (1996)
    [76] G. A. Lalazissis, J. Konig, and P. Ring, Phys. Rev. C, 55:540 (1997)
    [77] M. Bender, P. H. Heenen, and P. G. Reinhard, Rev. Mod. Phys., 75:121 (2003)
    [78] G. A. Lalazissis and M. M. Sharma, Nucl. Phys. A, 586:201 (1995)
    [79] J. Meng, H. Toki, S. G. Zhou, S. Q. Zhang, W. H. Long, and L. S. Geng, Prog. Part. Nucl. Phys., 57:470 (2006)
    [80] J. K. Zhang and X. J. Qiu, Phys. Lett. B, 152:153 (1985)
    [81] J. Mares and B. K. Jennings, Phys. Rev. C, 49:2472 (1994)
    [82] Z. Y. Ma, J. Speth, S. Krewld, B. Q. Chen and A. Reuber, Nucl. Phys. A, 608:305 (1996)
    [83] T. T. Sun, E. Hiyama, H. Sagawa, H. J. Schulze, and J. Meng, Phys. Rev. C, 94:064319 (2016)
    [84] T. T. Sun, W. L. Lu, and S. S. Zhang, Phys. Rev. C, 96:044312 (2017)
    [85] L. W. Chen, Phys. Rev. C, 83:044308 (2011)
    [86] C. J. Batty, Nucl. Phys. A, 372:418 (1981)
    [87] E. Friedman, A. Gal, and C. J. Batty, Nucl. Phys. A, 579:518 (1994)
    [88] C. J. Batty, E. Friedman, and A. Gal, Phys. Rep., 287:385 (1997)
    [89] E. Friedman, A. Gal, J. Mares, and A. Cieply, Phys. Rev. C, 60:024314 (1999)
    [90] A. Gal, Nucl. Phys. A, 691:268C (2001)
    [91] E. Friedman, and A. Gal, Phys. Rep., 452:89 (2007)
    [92] J. Schafiner-Bielich, I. N. Mishustin, and J. Bondorf, Nucl. Phys. A, 625:325 (1997)
    [93] A. Ramos, and E. Oset, Nucl. Phys. A, 671:481 (2000)
    [94] A. Cieply, E. Friedman, A. Gal, and J. Mares, Nucl. Phys. A, 696:173 (2001)
    [95] A. Cieply, E. Friedman, A. Gal, D. Gazda, J. Mares, Phys. Lett. B, 702:402 (2011)
    [96] T. Waas, N. Kaiser, and W. Weise, Phys. Lett. B, 365:12 (1996)
    [97] T. Waas, M. Rho, and W. Weise, Nucl. Phys. A, 617:(1997) 449
    [98] G. Q. Li, C. H. Lee, and G. E. Brown, Phys. Rev. Lett., 79:5214 (1997)
    [99] W. Cassing and E. L. Bratkovskaya, Phys. Rep., 308:65 (1999)
    [100] Z. Q. Feng, W. J. Xie, and G. M. Jin, Phys. Rev. C, 90:064604 (2014)
    [101] F. Laue et al, Phys. Rev. Lett., 82:1640 (1999)
    [102] A. Frster et al (KaoS Collaboration), Phys. Rev. Lett., 91:152301 (2003)
    [103] W. Scheinast et al, Phys. Rev. Lett., 96:072301 (2006)
    [104] Y. Sugahara and H. Toki, Nucl. Phys. A, 579:557 (1994)
    [105] M. M. Sharma, M. A. Nagarajan, and P. Ring, Phys. Lett. B, 312:377 (1993)
    [106] B. G. Todd-Rutel and J. Piekarewicz, Phys. Rev. Lett., 95:122501 (2005)
    [107] N. Kaiser, T. Waas, and W. Weise, Nucl. Phys. A, 612:297 (1997)
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Rongyao Yang, Sina Wei and Weizhou Jiang. Ground-state properties of light kaonic nuclei signaling symmetry energy at high densities[J]. Chinese Physics C, 2018, 42(2): 024102. doi: 10.1088/1674-1137/42/2/024102
Rongyao Yang, Sina Wei and Weizhou Jiang. Ground-state properties of light kaonic nuclei signaling symmetry energy at high densities[J]. Chinese Physics C, 2018, 42(2): 024102.  doi: 10.1088/1674-1137/42/2/024102 shu
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Received: 2017-10-28
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    Supported by National Natural Science Foundation of China (11775049, 11275048) and the China Jiangsu Provincial Natural Science Foundation (BK20131286)

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Ground-state properties of light kaonic nuclei signaling symmetry energy at high densities

    Corresponding author: Weizhou Jiang,
  • 1. School of Physics, Southeast University, Nanjing 211189, China
Fund Project:  Supported by National Natural Science Foundation of China (11775049, 11275048) and the China Jiangsu Provincial Natural Science Foundation (BK20131286)

Abstract: A sensitive correlation between the ground-state properties of light kaonic nuclei and the symmetry energy at high densities is constructed under the framework of relativistic mean-field theory. Taking oxygen isotopes as an example, we see that a high-density core is produced in kaonic oxygen nuclei, due to the strongly attractive antikaon-nucleon interaction. It is found that the 1S1/2 state energy in the high-density core of kaonic nuclei can directly probe the variation of the symmetry energy at supranormal nuclear density, and a sensitive correlation between the neutron skin thickness and the symmetry energy at supranormal density is established directly. Meanwhile, the sensitivity of the neutron skin thickness to the low-density slope of the symmetry energy is greatly increased in the corresponding kaonic nuclei. These sensitive relationships are established upon the fact that the isovector potential in the central region of kaonic nuclei becomes very sensitive to the variation of the symmetry energy. These findings might provide another perspective to constrain high-density symmetry energy, and await experimental verification in the future.

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