Symmetry Energy in Nucleon and Quark Matter

CHEN Liewen

doi:10.11804/NuclPhysRev.34.01.020

Volume 34 Issue 1

Jan. 2017

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Article Navigation > Nuclear Physics Review > 2017 > 34(1): 20-28

CHEN Liewen. Symmetry Energy in Nucleon and Quark Matter[J]. Nuclear Physics Review, 2017, 34(1): 20-28. doi: 10.11804/NuclPhysRev.34.01.020

Citation:

CHEN Liewen. Symmetry Energy in Nucleon and Quark Matter[J]. Nuclear Physics Review, 2017, 34(1): 20-28. doi: 10.11804/NuclPhysRev.34.01.020

Symmetry Energy in Nucleon and Quark Matter

doi: 10.11804/NuclPhysRev.34.01.020

CHEN Liewen^1,2

1.
Department of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China;
2.
Center of Theoretical Nuclear Physics, National Laboratory of Heavy-Ion Accelerator, Lanzhou 730000, China

Funds: National Basic Research Program of China(973 Program)(2013CB834405, 2015CB856904); National Natural Science Foundation of China(11625521, 11275125, 11135011); Program for Professor of Special Appointment (Eastern Scholar) at Shanghai Institutions of Higher Learning; Key Laboratory for Particle Physics, Astrophysics and Cosmology, Ministry of Education, China; Program of Science and Technology Commission of Shanghai Municipality(11DZ2260700)

Received Date: 2016-10-12
Rev Recd Date: 2017-02-22
Publish Date: 2017-03-20

Abstract

The symmetry energy characterizes the isospin dependent part of the equation of state of isospin asymmetric strong interaction matter and it plays a critical role in many issues of nuclear physics and astrophysics. In this talk, we briefly review the current status on the determination of the symmetry energy in nucleon (nuclear) and quark matter. For nuclear matter, while the subsaturation density behaviors of the symmetry energy are relatively well-determined and significant progress has been made on the symmetry energy around saturation density, the determination of the suprasaturation density behaviors of the symmetry energy remains a big challenge. For quark matter, which is expected to appear in dense matter at high baryon densities, we briefly review the recent work about the effects of quark matter symmetry energy on the properties of quark stars and the constraint of possible existence of heavy quark stars on quark matter symmetry energy. The results indicate that the u and d quarks could feel very different interactions in isospin asymmetric quark matter, which may have important implications on the isospin effects of partonic dynamics in relativistic heavy-ion collisions.
- symmetry energy,
- equation of state for asymmetric nuclear matter,
- equation of state for asymmetric quark matter,
- neutron star

References

[1]	LI B A, KO C M, BAUER W. Int J Mod Phys E, 1998, 7: 147.
[2]	LATTIMER J M, PRAKASH M. Science, 2004, 304: 536; LATTIMER J M, PRAKASH M. Phys Rep, 2007, 442: 109.
[3]	STEINER A W, PRAKASH M, LATTIMER J M, et al. Phys Rep, 2005, 411: 325.
[4]	BARAN V, COLONNA M, GRECO V, et al. Phys Rep, 2005, 410: 335.
[5]	CHEN L W, KO C M, LI B A et al. Front Phys China, 2007, 2: 327 [arXiv:0704.2340].
[6]	LI B A, CHEN L W, KO C M. Phys Rep, 2008, 464: 113.
[7]	TRAUTMAN W, WOLTER H H. Int J Mod Phys E, 2012, 21: 1230003.
[8]	TSANG B M, STONE J R, CAMERA F, et al. Phys Rev C, 2012, 86: 015803.
[9]	LATTIMER J M. Ann Rev Nucl Part Sci, 2012, 62: 485.
[10]	LI B A, CHEN L W, FATTOYEV F J, et al. J Phys: Conf Series, 2013, 413: 012021 [arXiv:1212.1178].
[11]	LI B A, RAMOS A, VERDE G, VIDANA I, Euro Phys. Journal A, 2014, 50.
[12]	HOROWITZ C J, BROWN E F, KIM Y, et al. J of Phys G, 2014, 41: 093001.
[13]	CHEN L W. Nucl Phys Rev, 2014, 37: 273[arXiv:1212.0284].
[14]	WANG R, CHEN L W. Phys Rev C, 2015, 92: 031303(R).
[15]	BALDO M, BURGIO G F. Prog Part Nucl Phys, 2016,[arXiv:1606.08838].
[16]	LI Z. Nucl Phys Rev, 2014, 31: 285.
[17]	JIANG W, YANG R, ZHANG D. Nucl Phys Rev, 2014, 31: 333.
[18]	DONG J, ZUO W, GU J, et al. Nucl Phys Rev, 2014, 31: 429.
[19]	WU Q, ZHANG Y, XIAO Z, et al. Nucl Phys Rev, 2016, 33: 251.
[20]	WANG H, XU C. Nucl Phys Rev, 2016, 33(1): 1; XU C. ibid, 2017, 34(1):.
[21]	HOROWITZ C J, POLLOCK S J, SOUDER P A, et al. Phys Rev C, 2001, 63: 025501.
[22]	SIL T, CENTELLES M, VI~NA S, et al. Phys Rev C, 2005, 71: 045502.
[23]	WEN D H, LI B A, CHEN L W. Phys Rev Lett, 2009, 103: 211102.
[24]	ZHENG H, ZHANG Z, CHEN L W. J Cosmo Astropart Phys, 2014, 08: 011.
[25]	CARLSON J, GANDOLFI S, PEDERIVA F, et al. Phys Rev C, 2015, 87: 1067.
[26]	XIAO Z G, LI B A, CHEN L W, et al. Phys Rev Lett, 2009, 102: 062502.
[27]	FENG Z Q, JIN G M. Phys Lett B, 2010, 683: 140.
[28]	RUSSOTTO P, WU P Z, ZORIC M, et al. Phys Lett B, 2011, 697: 471.
[29]	XU C, LI B A. Phys. Rev. C, 2010, 81: 064612.
[30]	WANG Y, GUO C, LI Q, et al. Nucl Phys Rev, 2015, 32(2): 154.
[31]	DI TORO M, BARAN V, COLONNA M, et al. Nucl Phys A, 2006, 775: 102.
[32]	DI TORO M, BARAN V, COLONNA M, GRECO V. J Phys G, 2010, 37: 083101.
[33]	PAGLIARA G, SCHAFFNER-BIELICH J. Phys Rev D, 2010, 81: 094024.
[34]	SHAO G Y, COLONNA M, DI TORO M, et al. Phys Rev D, 2012, 85: 114017.
[35]	CHU P C, CHEN L W. Astrophys J, 2014, 780: 135.
[36]	LIU H, XU J, CHEN L W, SUN K J. Phys Rev D, 2016, 94: 065032.
[37]	XIA Y H, XU C, ZONG H S. 2016, arXiv:1608.01724.
[38]	CAI B J, CHEN L W. Phys Rev C, 2012, 85: 024302.
[39]	ROCA-MAZA X, CENTELLES M, VINAS X, et al. Phys Rev Lett, 2011, 106: 252501.
[40]	CHEN L W. EPJ Web Conf, 2015, 88: 00017[arXiv:1506.09057].
[41]	VIDANA I, PROVIDENCIA C, POLLS A, et al. Phys Rev C, 2009, 80: 045806.
[42]	LI Z H, SCHULZE H J. Phys Rev C, 2008, 78: 028801.
[43]	KLAHN T, BLASCHKE D, TYPEL S, et al. Phys Rev C, 2006, 74: 035802.
[44]	SAMMARRUCA F. Int J Mod Phys E, 2010, 19: 1259.
[45]	AKMAL A, PANDHARIPANDE V R, RAVENHALL D G. Phys Rev C, 1998, 58: 1804.
[46]	FRIEDMAN B, PANDHARIPANDE V R. Nucl Phys A, 1981, 361: 502.
[47]	WIRINGA R B, FIKS V, FABROCINI A. Phys Rev C, 1988, 38: 1010.
[48]	CHEN L W. Phys Rev C, 2011, 83: 044308.
[49]	ZHANG Z, CHEN L W. Phys Lett B, 2013, 726: 234.
[50]	LATTIMER J M, STEINER A W. Eur Phys J A, 2014, 50: 40.
[51]	KORTELAINEN M, LESINSKI T, MORE J, et al. Phys Rev C, 2010, 82: 024313.
[52]	CHEN L W, KO C M, LI B A,et al. Phys Rev C, 2010, 82: 024321.
[53]	TAMⅡ A, POLTORATSKA I, von NEUMANN-COSEL Pet al. Phys Rev Lett, 2011, 107: 062502.
[54]	TRIPPA L, COLO G, VIGEZZI E, Phys Rev C, 2008, 77: 061304.
[55]	TSANG M B, ZHANG Y X, DANIELEWICZ, et al. Phys Rev Lett, 2009, 102: 122701.
[56]	DANIELEWICZ P, LEE J. Nucl Phys A, 2014, 922: 1.
[57]	STEINER A W, GANDOLFI S. Phys Rev Lett, 2012, 108: 081102.
[58]	HEBELER K, LATTIMER J, PETHICK C, et al. Phys Rev Lett, 2010, 105: 161102.
[59]	GANDOLFI S, CARLSON J, REDDY S. Phys Rev C, 2012, 85: 032801(R).
[60]	HOROWITZ C J, PIEKAREWICZ J. Phys Rev Lett, 2001, 86: 5647.
[61]	FURNSTAHL R J, Nucl Phys A, 2002, 706: 85.
[62]	WANG N, OU L, LIU M. Phys Rev C, 2013, 87: 034327.
[63]	BROWN B A. Phys Rev Lett, 2013, 111: 232502.
[64]	ZHANG Z, CHEN L W. Phys Rev C, 2015, 92: 031301(R).
[65]	CENTELLES M, ROCA-MAZA X, VINAS X, et al. Phys Rev Lett, 2009, 102: 122502; WARDA M, VINAS X, ROCA-MAZA X, et al. Phys Rev C, 2009, 80: 024316.
[66]	ALAM N, AGRAWAL B K, DE J N, et al. Phys Rev C, 2014, 90: 054317.
[67]	TYPEL S, ROPKE G, KLAHN T, et al. Phys Rev C, 2010, 81: 015803.
[68]	ROCA-MAZA X, BRENNA M, AGRAWAL B K, et al. Phys Rev C, 2013, 87: 034301.
[69]	CAO L G, MA Z Y. Chin Phys Lett, 2008, 25: 1625.
[70]	NATOWITZ J B, ROPKE G, TYPEL S, et al. Phys Rev Lett, 2010, 104: 202501; KOWALSKI S, NATOWITZ J B, SHLOMO S, et al. Phys Rev C, 2007, 75: 014601; WADA R, HAGEL K, QIN L, et al. Phys Rev C, 2012, 85: 064618.
[71]	DRISCHLER C, SOMA V, SCHWENK A. Phys Rev C, 2014, 89: 025806.
[72]	WELLENHOFER C, HOLT J W, KAISER N. Phys Rev C, 2015, 92: 015801.
[73]	XIE W J, SU J, ZHU L, ZHANG F S, Phys Lett B, 2013, 718: 1510.
[74]	XU J, CHEN L W, KO C M, et al. Phys Rev C, 2013, 87: 067601.
[75]	HONG J, DANIELEWICZ P. Phys Rev C, 2014, 90: 024605.
[76]	SONG T, KO C M. Phys Rev C, 2015, 91: 014901.
[77]	COZMA M D, LEIFELS Y, TRAUTMANN W, et al. arXiv:1305.5417v1, 2013.
[78]	RUSSOTTO P, GANNON S, KUPNY S, et al. Phys Rev C, 2016, 94: 034608.
[79]	DEMOREST P, PENNUCCI T, RANSOM, S, et al. Nature, 2010, 467: 1081.
[80]	ANTONIADIS J, FREIRE P C C, WEX N, et al. Science, 2013, 340: 6131.
[81]	REHBERG P, KLEVANSKY S P, Hufner J. Phys Rev C, 1996, 53: 410.

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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

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Symmetry Energy in Nucleon and Quark Matter

1. Department of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China;

2. Center of Theoretical Nuclear Physics, National Laboratory of Heavy-Ion Accelerator, Lanzhou 730000, China

Received Date: 2016-10-12

Rev Recd Date: 2017-02-22

Publish Date: 2017-03-20

Key words:

symmetry energy /
equation of state for asymmetric nuclear matter /
equation of state for asymmetric quark matter /
neutron star

Abstract: The symmetry energy characterizes the isospin dependent part of the equation of state of isospin asymmetric strong interaction matter and it plays a critical role in many issues of nuclear physics and astrophysics. In this talk, we briefly review the current status on the determination of the symmetry energy in nucleon (nuclear) and quark matter. For nuclear matter, while the subsaturation density behaviors of the symmetry energy are relatively well-determined and significant progress has been made on the symmetry energy around saturation density, the determination of the suprasaturation density behaviors of the symmetry energy remains a big challenge. For quark matter, which is expected to appear in dense matter at high baryon densities, we briefly review the recent work about the effects of quark matter symmetry energy on the properties of quark stars and the constraint of possible existence of heavy quark stars on quark matter symmetry energy. The results indicate that the u and d quarks could feel very different interactions in isospin asymmetric quark matter, which may have important implications on the isospin effects of partonic dynamics in relativistic heavy-ion collisions.

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Reference (81)

[1]	LI B A, KO C M, BAUER W. Int J Mod Phys E, 1998, 7: 147.
[2]	LATTIMER J M, PRAKASH M. Science, 2004, 304: 536; LATTIMER J M, PRAKASH M. Phys Rep, 2007, 442: 109.
[3]	STEINER A W, PRAKASH M, LATTIMER J M, et al. Phys Rep, 2005, 411: 325.
[4]	BARAN V, COLONNA M, GRECO V, et al. Phys Rep, 2005, 410: 335.
[5]	CHEN L W, KO C M, LI B A et al. Front Phys China, 2007, 2: 327 [arXiv:0704.2340].
[6]	LI B A, CHEN L W, KO C M. Phys Rep, 2008, 464: 113.
[7]	TRAUTMAN W, WOLTER H H. Int J Mod Phys E, 2012, 21: 1230003.
[8]	TSANG B M, STONE J R, CAMERA F, et al. Phys Rev C, 2012, 86: 015803.
[9]	LATTIMER J M. Ann Rev Nucl Part Sci, 2012, 62: 485.
[10]	LI B A, CHEN L W, FATTOYEV F J, et al. J Phys: Conf Series, 2013, 413: 012021 [arXiv:1212.1178].
[11]	LI B A, RAMOS A, VERDE G, VIDANA I, Euro Phys. Journal A, 2014, 50.
[12]	HOROWITZ C J, BROWN E F, KIM Y, et al. J of Phys G, 2014, 41: 093001.
[13]	CHEN L W. Nucl Phys Rev, 2014, 37: 273[arXiv:1212.0284].
[14]	WANG R, CHEN L W. Phys Rev C, 2015, 92: 031303(R).
[15]	BALDO M, BURGIO G F. Prog Part Nucl Phys, 2016,[arXiv:1606.08838].
[16]	LI Z. Nucl Phys Rev, 2014, 31: 285.
[17]	JIANG W, YANG R, ZHANG D. Nucl Phys Rev, 2014, 31: 333.
[18]	DONG J, ZUO W, GU J, et al. Nucl Phys Rev, 2014, 31: 429.
[19]	WU Q, ZHANG Y, XIAO Z, et al. Nucl Phys Rev, 2016, 33: 251.
[20]	WANG H, XU C. Nucl Phys Rev, 2016, 33(1): 1; XU C. ibid, 2017, 34(1):.
[21]	HOROWITZ C J, POLLOCK S J, SOUDER P A, et al. Phys Rev C, 2001, 63: 025501.
[22]	SIL T, CENTELLES M, VI~NA S, et al. Phys Rev C, 2005, 71: 045502.
[23]	WEN D H, LI B A, CHEN L W. Phys Rev Lett, 2009, 103: 211102.
[24]	ZHENG H, ZHANG Z, CHEN L W. J Cosmo Astropart Phys, 2014, 08: 011.
[25]	CARLSON J, GANDOLFI S, PEDERIVA F, et al. Phys Rev C, 2015, 87: 1067.
[26]	XIAO Z G, LI B A, CHEN L W, et al. Phys Rev Lett, 2009, 102: 062502.
[27]	FENG Z Q, JIN G M. Phys Lett B, 2010, 683: 140.
[28]	RUSSOTTO P, WU P Z, ZORIC M, et al. Phys Lett B, 2011, 697: 471.
[29]	XU C, LI B A. Phys. Rev. C, 2010, 81: 064612.
[30]	WANG Y, GUO C, LI Q, et al. Nucl Phys Rev, 2015, 32(2): 154.
[31]	DI TORO M, BARAN V, COLONNA M, et al. Nucl Phys A, 2006, 775: 102.
[32]	DI TORO M, BARAN V, COLONNA M, GRECO V. J Phys G, 2010, 37: 083101.
[33]	PAGLIARA G, SCHAFFNER-BIELICH J. Phys Rev D, 2010, 81: 094024.
[34]	SHAO G Y, COLONNA M, DI TORO M, et al. Phys Rev D, 2012, 85: 114017.
[35]	CHU P C, CHEN L W. Astrophys J, 2014, 780: 135.
[36]	LIU H, XU J, CHEN L W, SUN K J. Phys Rev D, 2016, 94: 065032.
[37]	XIA Y H, XU C, ZONG H S. 2016, arXiv:1608.01724.
[38]	CAI B J, CHEN L W. Phys Rev C, 2012, 85: 024302.
[39]	ROCA-MAZA X, CENTELLES M, VINAS X, et al. Phys Rev Lett, 2011, 106: 252501.
[40]	CHEN L W. EPJ Web Conf, 2015, 88: 00017[arXiv:1506.09057].
[41]	VIDANA I, PROVIDENCIA C, POLLS A, et al. Phys Rev C, 2009, 80: 045806.
[42]	LI Z H, SCHULZE H J. Phys Rev C, 2008, 78: 028801.
[43]	KLAHN T, BLASCHKE D, TYPEL S, et al. Phys Rev C, 2006, 74: 035802.
[44]	SAMMARRUCA F. Int J Mod Phys E, 2010, 19: 1259.
[45]	AKMAL A, PANDHARIPANDE V R, RAVENHALL D G. Phys Rev C, 1998, 58: 1804.
[46]	FRIEDMAN B, PANDHARIPANDE V R. Nucl Phys A, 1981, 361: 502.
[47]	WIRINGA R B, FIKS V, FABROCINI A. Phys Rev C, 1988, 38: 1010.
[48]	CHEN L W. Phys Rev C, 2011, 83: 044308.
[49]	ZHANG Z, CHEN L W. Phys Lett B, 2013, 726: 234.
[50]	LATTIMER J M, STEINER A W. Eur Phys J A, 2014, 50: 40.
[51]	KORTELAINEN M, LESINSKI T, MORE J, et al. Phys Rev C, 2010, 82: 024313.
[52]	CHEN L W, KO C M, LI B A,et al. Phys Rev C, 2010, 82: 024321.
[53]	TAMⅡ A, POLTORATSKA I, von NEUMANN-COSEL Pet al. Phys Rev Lett, 2011, 107: 062502.
[54]	TRIPPA L, COLO G, VIGEZZI E, Phys Rev C, 2008, 77: 061304.
[55]	TSANG M B, ZHANG Y X, DANIELEWICZ, et al. Phys Rev Lett, 2009, 102: 122701.
[56]	DANIELEWICZ P, LEE J. Nucl Phys A, 2014, 922: 1.
[57]	STEINER A W, GANDOLFI S. Phys Rev Lett, 2012, 108: 081102.
[58]	HEBELER K, LATTIMER J, PETHICK C, et al. Phys Rev Lett, 2010, 105: 161102.
[59]	GANDOLFI S, CARLSON J, REDDY S. Phys Rev C, 2012, 85: 032801(R).
[60]	HOROWITZ C J, PIEKAREWICZ J. Phys Rev Lett, 2001, 86: 5647.
[61]	FURNSTAHL R J, Nucl Phys A, 2002, 706: 85.
[62]	WANG N, OU L, LIU M. Phys Rev C, 2013, 87: 034327.
[63]	BROWN B A. Phys Rev Lett, 2013, 111: 232502.
[64]	ZHANG Z, CHEN L W. Phys Rev C, 2015, 92: 031301(R).
[65]	CENTELLES M, ROCA-MAZA X, VINAS X, et al. Phys Rev Lett, 2009, 102: 122502; WARDA M, VINAS X, ROCA-MAZA X, et al. Phys Rev C, 2009, 80: 024316.
[66]	ALAM N, AGRAWAL B K, DE J N, et al. Phys Rev C, 2014, 90: 054317.
[67]	TYPEL S, ROPKE G, KLAHN T, et al. Phys Rev C, 2010, 81: 015803.
[68]	ROCA-MAZA X, BRENNA M, AGRAWAL B K, et al. Phys Rev C, 2013, 87: 034301.
[69]	CAO L G, MA Z Y. Chin Phys Lett, 2008, 25: 1625.
[70]	NATOWITZ J B, ROPKE G, TYPEL S, et al. Phys Rev Lett, 2010, 104: 202501; KOWALSKI S, NATOWITZ J B, SHLOMO S, et al. Phys Rev C, 2007, 75: 014601; WADA R, HAGEL K, QIN L, et al. Phys Rev C, 2012, 85: 064618.
[71]	DRISCHLER C, SOMA V, SCHWENK A. Phys Rev C, 2014, 89: 025806.
[72]	WELLENHOFER C, HOLT J W, KAISER N. Phys Rev C, 2015, 92: 015801.
[73]	XIE W J, SU J, ZHU L, ZHANG F S, Phys Lett B, 2013, 718: 1510.
[74]	XU J, CHEN L W, KO C M, et al. Phys Rev C, 2013, 87: 067601.
[75]	HONG J, DANIELEWICZ P. Phys Rev C, 2014, 90: 024605.
[76]	SONG T, KO C M. Phys Rev C, 2015, 91: 014901.
[77]	COZMA M D, LEIFELS Y, TRAUTMANN W, et al. arXiv:1305.5417v1, 2013.
[78]	RUSSOTTO P, GANNON S, KUPNY S, et al. Phys Rev C, 2016, 94: 034608.
[79]	DEMOREST P, PENNUCCI T, RANSOM, S, et al. Nature, 2010, 467: 1081.
[80]	ANTONIADIS J, FREIRE P C C, WEX N, et al. Science, 2013, 340: 6131.
[81]	REHBERG P, KLEVANSKY S P, Hufner J. Phys Rev C, 1996, 53: 410.

Symmetry Energy in Nucleon and Quark Matter

doi: 10.11804/NuclPhysRev.34.01.020

Abstract

References

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通讯作者: 陈斌, bchen63@163.com

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