Massive neutron stars and &Lambda;-hypernuclei in relativistic mean field models

Ting-Ting Sun; Cheng-Jun Xia; Shi-Sheng Zhang; M. S. Smith

doi:10.1088/1674-1137/42/2/025101

Chinese Physics C> 2018, Vol. 42> Issue(2) : 025101 DOI: 10.1088/1674-1137/42/2/025101

Massive neutron stars and Λ-hypernuclei in relativistic mean field models

1.
School of Physics and Engineering and Henan Key Laboratory of Ion Beam Bioengineering, Zhengzhou University, Zhengzhou 450001, China
2.
School of Information Science and Engineering, Ningbo Institute of Technology, Zhejiang University, Ningbo 315100, China
3.
CAS Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, China
4.
School of Physics and Nuclear Energy Engineering, Beihang University, Beijing 100191, China
5.
Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee, 37831-6354, USA

Abstract
HTML
Reference
Related

PDF

Abstract：
Based on relativistic mean field (RMF) models, we study finite Λ-hypernuclei and massive neutron stars. The effective m N-m N interactions PK1 and TM1 are adopted, while the m N-Λ interactions are constrained by reproducing the binding energy of Λ-hyperon at 1s orbit of _Λ⁴⁰Ca. It is found that the Λ-meson couplings follow a simple relation, indicating a fixed Λ potential well for symmetric nuclear matter at saturation densities, i.e., around V_Λ=-29.786 MeV. With those interactions, a large mass range of Λ-hypernuclei can be described well. Furthermore, the masses of PSR J1614-2230 and PSR J0348+0432 can be attained adopting the Λ-meson couplings g_σΛ/g_σN≳ 0.73, g_ωΛ/g_ωN≳0.80 for PK1 and g_σΛ/g_σN≳ 0.81, g_ωΛ/g_ωN≳ 0.90 for TM1, respectively. This resolves the hyperon puzzle without introducing any additional degrees of freedom.
- massive neutron stars ,
- -hypernuclei ,
- relativistic mean field theory

References

[1]	S. E. Woosley, A. Heger, and T. A. Weaver, Rev. Mod. Phys., 74:1015 (2002)
[2]	J. M. Lattimer, Annu. Rev. Nucl. Part. Sci., 62:485 (2012)
[3]	F. zel, D. Psaltis, T. Guver, G. Baym, C. Heinke, and S. Guillot, Astrophys. J. 820:28 (2016)
[4]	F. zel and P. Freire, Annu. Rev. Astron. Astrophys., 54:401 (2016)
[5]	K. Hotokezaka, K. Kyutoku, H. Okawa, M. Shibata, and K. Kiuchi, Phys. Rev. D, 83:124008 (2011)
[6]	P. Danielewicz, R. Lacey, and W. G. Lynch, Science, 298:1592 (2002)
[7]	B.-A. Li, L.-W. Chen, and C. M. Ko, Phys. Rep., 464:113 (2008)
[8]	F. Weber, Prog. Part. Nucl. Phys., 54:193 (2005)
[9]	L. McLerran, Nucl. Phys. B (Proc. Suppl.), 195:275 (2009), arXiv:0906.2651[hep-ph]
[10]	C. Ishizuka, A. Ohnishi, K. Tsubakihara, K. Sumiyoshi, and S. Yamada, J. Phys. G:Nucl. Part. Phys., 35:085201 (2008)
[11]	H. Shen, H. Toki, K. Oyamatsu, and K. Sumiyoshi, Astrophys. J., 197:20 (2011)
[12]	H. Noumi, P. K. Saha, D. Abe, S. Ajimura, K. Aoki, H. C. Bhang, T. Endo, Y. Fujii, T. Fukuda, H. C. Guo, K. Imai, O. Hashimoto, H. Hotchi, E. H. Kim, J. H. Kim, T. Kishimoto, A. Krutenkova, K. Maeda, T. Nagae, M. Nakamura, H. Outa, M. Sekimoto, T. Saito, A. Sakaguchi, Y. Sato, R. Sawafta, Y. Shimizu, T. Takahashi, L. Tang, H. Tamura, K. Tanida, T. Watanabe, H. H. Xia, S. H. Zhou, L. H. Zhu, and X. F. Zhu, Phys. Rev. Lett., 89:072301 (2002)
[13]	H. Noumi, P. K. Saha, D. Abe, S. Ajimura, K. Aoki, H. C. Bhang, T. Endo, Y. Fujii, T. Fukuda, H. C. Guo, K. Imai, O. Hashimoto, H. Hotchi, E. H. Kim, J. H. Kim, T. Kishimoto, A. Krutenkova, K. Maeda, T. Nagae, M. Nakamura, H. Outa, M. Sekimoto, T. Saito, A. Sakaguchi, Y. Sato, R. Sawafta, Y. Shimizu, T. Takahashi, L. Tang, H. Tamura, K. Tanida, T. Watanabe, H. H. Xia, S. H. Zhou, L. H. Zhu, and X. F. Zhu, Phys. Rev. Lett., 90:049902 (2003)
[14]	P. K. Saha, H. Noumi, D. Abe, S. Ajimura, K. Aoki, H. C. Bhang, K. Dobashi, T. Endo, Y. Fujii, T. Fukuda, H. C. Guo, O. Hashimoto, H. Hotchi, K. Imai, E. H. Kim, J. H. Kim, T. Kishimoto, A. Krutenkova, K. Maeda, T. Nagae, M. Nakamura, H. Outa, T. Saito, A. Sakaguchi, Y. Sato, R. Sawafta, M. Sekimoto, Y. Shimizu, T. Takahashi, H. Tamura, L. Tang, K. Tanida, T. Watanabe, H. H. Xia, S. H. Zhou, X. F. Zhu, and L. H. Zhu, Phys. Rev. C, 70:044613 (2004)
[15]	A. R. Bodmer, Q. N. Usmani, and J. Carlson, Phys. Rev. C, 29:684 (1984)
[16]	O. Hashimoto and H. Tamura, Prog. Part. Nucl. Phys., 57:564 (2006)
[17]	A. Gal, J. Soper, and R. Dalitz, Ann. Phys., 63:53 (1971)
[18]	R. Dalitz and A. Gal, Ann. Phys., 116:167 (1978)
[19]	D. Millener, Nucl. Phys. A, 804:84 (2008), special Issue on Recent Advances in Strangeness Nuclear Physics
[20]	D. Millener, Nucl. Phys. A, 914:109 (2013), {XI} International Conference on Hypernuclear and Strange Particle Physics (HYP2012)
[21]	T. Motoba, H. Bando, and K. Ikeda, Prog. Theor. Phys., 70:189 (1983)
[22]	E. Hiyama, M. Kamimura, T. Motoba, T. Yamada, and Y. Yamamoto, Phys. Rev. C, 66:024007 (2002)
[23]	E. Hiyama, Y. Yamamoto, T. A. Rijken, and T. Motoba, Phys. Rev. C, 74:054312 (2006)
[24]	E. Hiyama, Y. Yamamoto, T. Motoba, and M. Kamimura, Phys. Rev. C, 80:054321 (2009)
[25]	H. Bando, T. Motoba, and J. Zofka, Int. J. Mod. Phys. A, 05:4021 (1990)
[26]	M. Isaka, M. Kimura, A. Dot, and A. Ohnishi, Phys. Rev. C, 87:021304 (2013)
[27]	J. N. Hu, A. Li, H. Toki, and W. Zuo, Phys. Rev. C, 89:025802 (2014)
[28]	R. Brockmann and W. Weise, Phys. Lett. B, 69:167 (1977)
[29]	J. Boguta and S. Bohrmann, Phys. Lett. B, 102:93 (1981)
[30]	J. Mares and J. Zofka, Z. Phys. A, 333:209 (1989)
[31]	J. Mares and B. K. Jennings, Phys. Rev. C, 49:2472 (1994)
[32]	Y. Sugahara and H. Toki, Prog. Theor. Phys., 92:803 (1994)
[33]	C. Y. Song, J. M. Yao, H.-F. Lv, and J. Meng, Int. J. Mod. Phys. E, 19:2538 (2010)
[34]	Y. Tanimura and K. Hagino, Phys. Rev. C, 85:014306 (2012)
[35]	X.-S. Wang, H.-Y. Sang, J.-H. Wang, and H.-F. Lv, Commun. Theor. Phys. 60:479 (2013)
[36]	X.-R. Zhou, H.-J. Schulze, H. Sagawa, C.-X. Wu, and E.-G. Zhao, Phys. Rev. C, 76:034312 (2007)
[37]	K. Tsushima, K. Saito, and A. Thomas, Phys. Lett. B, 411:9 (1997)
[38]	K. Tsushima, K. Saito, J. Haidenbauer, and A. Thomas, Nucl. Phys. A, 630:691 (1998)
[39]	P. A. Guichon, A. W. Thomas, and K. Tsushima, Nucl. Phys. A, 814:66 (2008)
[40]	H. Takahashi, J. K. Ahn, H. Akikawa, S. Aoki, K. Arai, S. Y. Bahk, K. M. Baik, B. Bassalleck, J. H. Chung, M. S. Chung, D. H. Davis, T. Fukuda, K. Hoshino, A. Ichikawa, M. Ieiri, K. Imai, Y. H. Iwata, Y. S. Iwata, H. Kanda, M. Kaneko, T. Kawai, M. Kawasaki, C. O. Kim, J. Y. Kim, S. J. Kim, S. H. Kim, Y. Kondo, T. Kouketsu, Y. L. Lee, J. W. C. McNabb, M. Mitsuhara, Y. Nagase, C. Nagoshi, K. Nakazawa, H. Noumi, S. Ogawa, H. Okabe, K. Oyama, H. M. Park, I. G. Park, J. Parker, Y. S. Ra, J. T. Rhee, A. Rusek, H. Shibuya, K. S. Sim, P. K. Saha, D. Seki, M. Sekimoto, J. S. Song, T. Takahashi, F. Takeutchi, H. Tanaka, K. Tanida, J. Tojo, H. Torii, S. Torikai, D. N. Tovee, N. Ushida, K. Yamamoto, N. Yasuda, J. T. Yang, C. J. Yoon, C. S. Yoon, M. Yosoi, T. Yoshida, and L. Zhu, Phys. Rev. Lett., 87:212502 (2001)
[41]	S. Aoki, Prog. Part. Nucl. Phys., 66:687 (2011)
[42]	I. Vidana, AIP Conf. Proc., 1645:79 (2015)
[43]	P. B. Demorest, T. Pennucci, S. M. Ransom, M. S. E. Roberts, and J. W. T. Hessels, Nature, 467:1081 (2010)
[44]	E. Fonseca, T. T. Pennucci, J. A. Ellis, I. H. Stairs, D. J. Nice, S. M. Ransom, P. B. Demorest, Z. Arzoumanian, K. Crowter, T. Dolch, R. D. Ferdman, M. E. Gonzalez, G. Jones, M. L. Jones, M. T. Lam, L. Levin, M. A. McLaughlin, K. Stovall, J. K. Swiggum, and W. Zhu, Astrophys. J., 832:167 (2016)
[45]	J. Antoniadis, P. C. C. Freire, N. Wex, T. M. Tauris, R. S. Lynch, M. H. van Kerkwijk, M. Kramer, C. Bassa, V. S. Dhillon, T. Driebe, J. W. T. Hessels, V. M. Kaspi, V. I. Kondratiev, N. Langer, T. R. Marsh, M. A. McLaughlin, T. T. Pennucci, S. M. Ransom, I. H. Stairs, J. van Leeuwen, J. P. W. Verbiest, and D. G. Whelan, Science, 340:6131 (2013)
[46]	I. Vidana, J. Phys:Conf. Ser., 668:012031 (2016)
[47]	S. Weissenborn, D. Chatterjee, and J. Schaffner-Bielich, Phys. Rev. C, 85:065802 (2012)
[48]	Bednarek, I., Haensel, P., Zdunik, J. L., Bejger, M., and Mańka, R., Astron. Astrophys., 543:A157 (2012)
[49]	M. Oertel, C. Providencia, F. Gulminelli, and A. R. Raduta, J. Phys. G:Nucl. Part. Phys., 42:075202 (2015)
[50]	K. Maslov, E. Kolomeitsev, and D. Voskresensky, Phys. Lett. B, 748:369 (2015)
[51]	K. Maslov, E. Kolomeitsev, and D. Voskresensky, Nucl. Phys. A, 950:64 (2016)
[52]	T. Takatsuka, S. Nishizaki, and Y. Yamamoto, Eur. Phys. J. A, 13:213 (2002)
[53]	I. Vidana, D. Logoteta, C. Providncia, A. Polls, and I. Bombaci, Europhys. Lett., 94:11002 (2011)
[54]	Y. Yamamoto, T. Furumoto, N. Yasutake, and T. A. Rijken, Phys. Rev. C, 88:022801 (2013)
[55]	D. Lonardoni, A. Lovato, S. Gandolfi, and F. Pederiva, Phys. Rev. Lett., 114:092301 (2015)
[56]	H. Togashi, E. Hiyama, Y. Yamamoto, and M. Takano, Phys. Rev. C, 93:035808 (2016)
[57]	S. Weissenborn, I. Sagert, G. Pagliara, M. Hempel, and J. Schaffner-Bielich, Astrophys. J., 740:L14 (2011)
[58]	T. Klahn, R. Lastowiecki, and D. Blaschke, Phys. Rev. D, 88:085001 (2013)
[59]	T. Zhao, S.-S. Xu, Y. Yan, X.-L. Luo, X.-J. Liu, and H.-S. Zong, Phys. Rev. D, 92:054012 (2015)
[60]	T. Kojo, P. D. Powell, Y. Song, and G. Baym, Phys. Rev. D, 91:045003 (2015)
[61]	K. Masuda, T. Hatsuda, and T. Takatsuka, Eur. Phys. J. A, 52:65 (2016)
[62]	A. Li, W. Zuo, and G. X. Peng, Phys. Rev. C, 91:035803 (2015)
[63]	D. L. Whittenbury, H. H. Matevosyan, and A. W. Thomas, Phys. Rev. C, 93:035807 (2016)
[64]	K. Fukushima and T. Kojo, Astrophys. J., 817:180 (2016)
[65]	P.-G. Reinhard, Rep. Prog. Phys., 52:439 (1989)
[66]	P. Ring, Prog. Part. Nucl. Phys., 37:193 (1996)
[67]	J. Meng, H. Toki, S. Zhou, S. Zhang, W. Long, and L. Geng, Prog. Part. Nucl. Phys., 57:470 (2006)
[68]	N. Paar, D. Vretenar, E. Khan, and G. Col, Rep. Prog. Phys., 70:691 (2007)
[69]	J. Meng and S. G. Zhou, J. Phys. G:Nucl. Part. Phys., 42:093101 (2015)
[70]	J. Meng, ed., Relativistic Density Functional for Nuclear Structure, International Review of Nuclear Physics, Vol. 10:(World Scientific Singapore, 2016)
[71]	S. Typel and H. Wolter, Nucl. Phys. A, 656:331 (1999)
[72]	D. Vretenar, W. Pschl, G. A. Lalazissis, and P. Ring, Phys. Rev. C, 57:R1060 (1998)
[73]	B.-N. Lu, E.-G. Zhao, and S.-G. Zhou, Phys. Rev. C, 84:014328 (2011)
[74]	K. Hagino and J. Yao, arXiv:1410.7531 (2014)
[75]	T. T. Sun, E. Hiyama, H. Sagawa, H.-J. Schulze, and J. Meng, Phys. Rev. C, 94:064319 (2016)
[76]	N. Glendenning, Compact Stars. Nuclear Physics, Particle Physics, and General Relativity, 2nd ed., ISBN 978-0-387-98977-8 (Springer-Verlag, Berlin, 2000)
[77]	S. F. Ban, J. Li, S. Q. Zhang, H. Y. Jia, J. P. Sang, and J. Meng, Phys. Rev. C, 69:045805 (2004)
[78]	F. Weber, R. Negreiros, P. Rosenfield, and M. Stejner, Prog. Part. Nucl. Phys., 59:94 (2007)
[79]	W. H. Long, B. Y. Sun, K. Hagino, and H. Sagawa, Phys. Rev. C, 85:025806 (2012)
[80]	T. T. Sun, B. Y. Sun, and J. Meng, Phys. Rev. C, 86:014305 (2012)
[81]	S. Wang, H. F. Zhang, and J. M. Dong, Phys. Rev. C, 90:055801 (2014)
[82]	A. Fedoseew and H. Lenske, Phys. Rev. C, 91:034307 (2015)
[83]	W.-H. Long, J. Meng, N. V. Giai, and S.-G. Zhou, Phys. Rev. C, 69:034319 (2004)
[84]	Y. Sugahara and H. Toki, Nucl. Phys. A, 579:557 (1994)
[85]	C. Dover and A. Gal, Prog. Part. Nucl. Phys., 12:171 (1984)
[86]	Particle Data Group, Chin. Phys. C, 38:090001 (2014)
[87]	J. M. Weisberg, D. J. Nice, and J. H. Taylor, Astrophys. J., 722:1030 (2010)
[88]	R. P. Feynman, N. Metropolis, and E. Teller, Phys. Rev., 75:1561 (1949)
[89]	G. Baym, C. Pethick, and P. Sutherland, Astrophys. J., 170:299 (1971)
[90]	J. W. Negele and D. Vautherin, Nucl. Phys. A, 207:298 (1973)
[91]	LIGO Scientific Collaboration and Virgo Collaboration, Phys. Rev. Lett., 119:161101 (2017)
[92]	LIGO Scientific Collaboration and Virgo Collaboration, arXiv 1710.09320 (2017)

[1]	Shi-Yuan Ding , Wei Yang , Bao-Yuan Sun . Density-dependent relativistic mean field approach and its application to single-Λ hypernuclei in oxygen hyperisotopes. Chinese Physics C, 2023, 47(12): 124103. doi: 10.1088/1674-1137/acf91e
[2]	Kai-Wen Li , Xiu-Lei Ren , Li-Sheng Geng , Bing-Wei Long . Leading order relativistic hyperon-nucleon interactions in chiral effective field theory. Chinese Physics C, 2018, 42(1): 014105. doi: 10.1088/1674-1137/42/1/014105
[3]	Bin Hong , Huan-Yu Jia , Xue-Ling Mu , Xia Zhou . Influence of the weakly interacting light U boson on the properties of massive protoneutron stars. Chinese Physics C, 2016, 40(6): 065101. doi: 10.1088/1674-1137/40/6/065101
[4]	Hong-Bo Bai , Zhen-Hua Zhang , Xiao-Wei Li . Investigation of the Mg isotopes using the shell-model-like approach in relativistic mean field theory. Chinese Physics C, 2016, 40(11): 114101. doi: 10.1088/1674-1137/40/11/114101
[5]	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
[6]	ZHOU Xia , KANG Miao , WANG Na . Effect of magnetic field decay on the chemical heating of cooling neutron stars. Chinese Physics C, 2013, 37(8): 085102. doi: 10.1088/1674-1137/37/8/085102
[7]	JI Juan-Xia , LI Jia-Xing , HAN Rui , WANG Jian-Song , HU Qiang . The neutron halo structure of ¹⁷B studied with the relativistic Hartree-Bogoliubov theory. Chinese Physics C, 2012, 36(1): 43-47. doi: 10.1088/1674-1137/36/1/007
[8]	MEI Hua , CHEN Hong , YAO Jiang-Ming . Single-particle resonance states of ¹²²Zr in relativistic mean-field theory combined with real stabilization method. Chinese Physics C, 2009, 33(S1): 101-104. doi: 10.1088/1674-1137/33/S1/033
[9]	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
[10]	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
[11]	YAO Jiang-Ming , . Towards Lambda-nucleon coupling constants in relativistic mean field theory. Chinese Physics C, 2009, 33(S1): 64-66. doi: 10.1088/1674-1137/33/S1/021
[12]	SUN Bao-Yuan , MENG Jie . Neutron star equation of state in density dependent relativistic Hartree-Fock theory. Chinese Physics C, 2009, 33(S1): 73-75. doi: 10.1088/1674-1137/33/S1/024
[13]	ZHOU Xian-Rong . Properties of deformed Λ hypernuclei. Chinese Physics C, 2009, 33(S1): 82-85. doi: 10.1088/1674-1137/33/S1/027
[14]	LIU Jun , JIA Wen-Zhi , WANG Shun-Jin . Microscopic calculation of the magnetic field of neutron stars. Chinese Physics C, 2009, 33(9): 737-742. doi: 10.1088/1674-1137/33/9/005
[15]	JING Han-Tao , SHEN Peng-Nian , JIANG Huan-Qing . Production of Λ-hypernuclei in A(p,K⁺)_ΛB reactions. Chinese Physics C, 2008, 32(12): 962-971. doi: 10.1088/1674-1137/32/12/005
[16]	GUO Jian-You , SHENG Zong-Qiang , FANG Xiang-Zheng . A systematic study of the superdeformation of Pb isotopes with relativistic mean field theory. Chinese Physics C, 2008, 32(11): 886-891. doi: 10.1088/1674-1137/32/11/008
[17]	LIU Jing-Jing , LUO Zhi-Quan . Neutrino energy loss by electron capture in magnetic field at the crusts of neutron stars. Chinese Physics C, 2008, 32(2): 108-111. doi: 10.1088/1674-1137/32/2/007
[18]	NING Ping-Zhi , TAN Yu-Hong LI Lei , LUO Yan-An , . Relativistic Mean Field Theory for Hypernuclei. Chinese Physics C, 2004, 28(12): 1336-1342.
[19]	Shen Yaosong , Ren Zhongzhou . Relativistic Mean-field Calculation on Λ Hypernuclei. Chinese Physics C, 1997, 21(S4): 47-54.
[20]	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.

Access

Get Citation

Ting-Ting Sun, Cheng-Jun Xia, Shi-Sheng Zhang and M. S. Smith. Massive neutron stars and Λ-hypernuclei in relativistic mean field models[J]. Chinese Physics C, 2018, 42(2): 025101. doi: 10.1088/1674-1137/42/2/025101

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 2017-10-23

Fund

Supported by National Natural Science Foundation of China (11525524, 11505157, 11375022, 11705163, 11621131001), National Key Basic Research Program of China (2013CB834400), the Physics Research and Development Program of Zhengzhou University (32410017) and the Office of Nuclear Physics in the U.S. Dept. of Energy. The computation for this work was supported by the HPC Cluster of SKLTP/ITP-CAS and the Supercomputing Center, CNIC, of the CAS

Article Metric

Article Views(1609)
PDF Downloads(40)
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

Massive neutron stars and Λ-hypernuclei in relativistic mean field models

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

Massive neutron stars and Λ-hypernuclei in relativistic mean field models

Corresponding author: Cheng-Jun Xia,

HTML

目录