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

Rongyao Yang; Sina Wei; Weizhou Jiang

doi:10.1088/1674-1137/42/2/024102

Chinese Physics C> 2018, Vol. 42> Issue(2) : 024102 DOI: 10.1088/1674-1137/42/2/024102

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

1.
School of Physics, Southeast University, Nanjing 211189, China

Abstract
HTML
Reference
Related

PDF

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 1S_1/2 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.
- symmetry energy ,
- neutron skin thickness ,
- kaonic nuclei ,
- relativistic mean-field theory

References

[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)

[1]	Shi-Hui Cheng , Jing Wen , Li-Gang Cao , Feng-Shou Zhang . Neutron skin thickness of ⁹⁰Zr and symmetry energy constrained by charge exchange spin-dipole excitations. Chinese Physics C, 2023, 47(2): 024102. doi: 10.1088/1674-1137/aca38e
[2]	Nai-Bo Zhang , Bin Qi , Shou-Yu Wang . Key factor for determining relation between radius and tidal deformability of neutron stars: Slope of symmetry energy. Chinese Physics C, 2020, 44(6): 064103. doi: 10.1088/1674-1137/44/6/064103
[3]	W. M. Seif , A. Abdurrahman . Influence of proton-skin thickness on the α decays of heavy nuclei. Chinese Physics C, 2018, 42(1): 014106. doi: 10.1088/1674-1137/42/1/014106
[4]	W. M. Seif , A. S. Hashem . Constraints on the nuclear symmetry energy and its density slope from the α decay process. Chinese Physics C, 2018, 42(6): 064104. doi: 10.1088/1674-1137/42/6/064104
[5]	Mariana Dutra , Odilon Louren , Or Hen , Eliezer Piasetzky , Débora P. Menezes . The symmetry energy γ parameter of relativistic mean-field models. Chinese Physics C, 2018, 42(6): 064105. doi: 10.1088/1674-1137/42/6/064105
[6]	Su-Ya-La-Tu Zhang , Mei-Rong Huang , R. Wada , Xing-Quan Liu , Wei-Ping Lin , Jian-Song Wang . Symmetry energy and experimentally observed cold fragments in intermediate heavy-ion collisions. Chinese Physics C, 2017, 41(4): 044001. doi: 10.1088/1674-1137/41/4/044001
[7]	Ya-Fei Guo , Peng-Hui Chen , Fei Niu , Hong-Fei Zhang , Gen-Ming Jin , Zhao-Qing Feng . Isospin splitting of nucleon effective mass and symmetry energy in isotopic nuclear reactions. Chinese Physics C, 2017, 41(10): 104104. doi: 10.1088/1674-1137/41/10/104104
[8]	Jun-Long Tian , Hai-Tao Cui , Teng Gao , Ning Wang . Effect of Wigner energy on the symmetry energy coefficient in nuclei. Chinese Physics C, 2016, 40(9): 094101. doi: 10.1088/1674-1137/40/9/094101
[9]	FAN Guang-Wei , DONG Tie-Kuang , D. Nishimura . Nonlinear relativistic mean-field theory studies on He isotopes. Chinese Physics C, 2014, 38(12): 124102. doi: 10.1088/1674-1137/38/12/124102
[10]	GUAN Xin , LI Hang , TAN Qi , PAN Feng . Nilsson mean-field plus the extended pairing model description of rare earth nuclei. Chinese Physics C, 2011, 35(8): 747-752. doi: 10.1088/1674-1137/35/8/009
[11]	SUN Xiao-Yan , FANG De-Qing , MA Yu-Gang , CAI Xiang-Zhou , CHEN Jin-Gen , GUO Wei , TIAN Wen-Dong , WANG Hong-Wei , ZHANG Guo-Qiang , ZHOU Pei . A new probe of neutron skin thickness. Chinese Physics C, 2011, 35(6): 555-560. doi: 10.1088/1674-1137/35/6/009
[12]	MA Chun-Wang , WANG Shan-Shan . Isospin dependence of projectile fragmentation and neutron-skin thickness of neutron-rich nuclei. Chinese Physics C, 2011, 35(11): 1017-1021. doi: 10.1088/1674-1137/35/11/007
[13]	LIU Min , LI Zhu-Xia , WANG Ning , ZHANG Feng-Shou . Exploring nuclear symmetry energy with isospin dependence in neutron skin thickness of nuclei. Chinese Physics C, 2011, 35(7): 629-634. doi: 10.1088/1674-1137/35/7/006
[14]	MA Chun-Wang , WEI Hui-Ling , ZHANG Yan-Fang , LIU Gao-Jie , WANG Jun-Yang , TANG Kai . A revisit to the neutron skin thickness of neutron-rich nuclei in the statistical abrasion ablation model. Chinese Physics C, 2010, 34(9): 1469-1471. doi: 10.1088/1674-1137/34/9/074
[15]	GAO Yuan , DONG Jian-Min , ZHANG Hong-Fei , ZUO Wei , LI Jun-Qing . Properties and structure of N=Z nuclei within relativistic mean field theory. Chinese Physics C, 2009, 33(10): 848-853. doi: 10.1088/1674-1137/33/10/006
[16]	LI Yi-He , WU Shi-Shu . Deeply bound kaonic states in nuclei. Chinese Physics C, 2009, 33(S1): 76-78. doi: 10.1088/1674-1137/33/S1/025
[17]	YAO Jiang-Ming , MENG Jie , Pena Arteaga , Ring Peter . Restoration of rotational symmetry in deformed relativistic mean-field theory. Chinese Physics C, 2009, 33(S1): 21-23. doi: 10.1088/1674-1137/33/S1/007
[18]	Shen Yaosong , Ren Zhongzhou . Relativistic Mean-field Calculation on Λ Hypernuclei. Chinese Physics C, 1997, 21(S4): 47-54.
[19]	Chen Baoqiu , Ma Zhongyu . Description of the Properties of Nuclei Far From the β Stability Line in the Relativistic Mean Field Theory. Chinese Physics C, 1994, 18(Z1): 87-94.
[20]	Liu Baohua , Li Jiarong . The Mean-Field Analysis for Chiral Symmetry Phase Transition. Chinese Physics C, 1988, 12(S4): 373-378.

Access

Get Citation

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

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 2017-10-28

Fund

Supported by National Natural Science Foundation of China (11775049, 11275048) and the China Jiangsu Provincial Natural Science Foundation (BK20131286)

Article Metric

Article Views(1592)
PDF Downloads(20)
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

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

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

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

Corresponding author: Weizhou Jiang,

HTML

目录