Chin. Phys. Lett.  2010, Vol. 27 Issue (12): 121202    DOI: 10.1088/0256-307X/27/12/121202
THE PHYSICS OF ELEMENTARY PARTICLES AND FIELDS |
The Renormalized Equation of State and Quark Star
LI Hua1, LUO Xin-Lian2, JIANG Yu1, ZONG Hong-Shi1,3**
1Department of Physics, Nanjing University, Nanjing 210093
2Department of Astronomy, Nanjing University, Nanjing 210093
3Joint Center for Particle, Nuclear Physics and Cosmology, Nanjing 210093
Cite this article:   
LI Hua, LUO Xin-Lian, JIANG Yu et al  2010 Chin. Phys. Lett. 27 121202
Download: PDF(583KB)  
Export: BibTeX | EndNote | Reference Manager | ProCite | RefWorks
Abstract By means of the EOS of QCD at zero temperature and finite quark chemical potential we proposed [Phys. Rev. D 78 (2008) 054001] in the framework of rainbow-ladder approximation of Dyson–Schwinger approach, we investigate the structure of quark star and its property. It is found that the mass-radius relation in our model is very different from that of usual quark star models, but similar to neutron star models. The obtained mass of quark star is about 1.75Mʘ ∼ 2.2Mʘ. The obtained radius of quark star is 2226 km, which is obviously larger than the results in other models. The reason for this discrepancy is analyzed.
Keywords: 12.38.Lg      21.65.Qr      26.60.Kp     
Received: 05 August 2010      Published: 23 November 2010
PACS:  12.38.Lg (Other nonperturbative calculations)  
  21.65.Qr (Quark matter)  
  26.60.Kp (Equations of state of neutron-star matter)  
TRENDMD:   
URL:  
https://cpl.iphy.ac.cn/10.1088/0256-307X/27/12/121202       OR      https://cpl.iphy.ac.cn/Y2010/V27/I12/121202
Service
E-mail this article
E-mail Alert
RSS
Articles by authors
LI Hua
LUO Xin-Lian
JIANG Yu
ZONG Hong-Shi
[1] Witten E 1984 Phys. Rev. D 30 272
[2] Farhi E and Jaffe R L 1984 Phys. Rev. D 30 2379
[3] Alcock C et al 1986 Astrophys. J. 310 261
[4] Haensel P et al 1986 Astron. Astrophys. 160 121
[5] Hanauske M et al 2001 Phys. Rev. D 64 043005
[6] Glendenning N K and Kettner C 2000 Astron. Astrophys. 353 L9
[7] Dey M, Bombaci I et al 1998 Phys. Lett. B 438 123.
[8] Prakash M, Baron E and Prakash M 1990 Phys. Lett. B 243 175
[9] Steiner A, Prakash M and Lattimer J M 2000 Phys. Lett. B 486 239
[10] Glendenning N K 2000 Compact Stars: Nuclear Physics, Particle Physics, and General Relativity (New York: Springer)
[11] Alford M and Reddy S 2003 Phys. Rev. D 67 074024
[12] Rehberg P, Klevansky S P and Hüfner J 1996 Phys. Rev. C 53 410
[13] Rüster S B and Rischke D H 2004 Phys. Rev. D 69 045011
[14] Fraga E S et al 2001 Phys. Rev. D 63 121702
[15] Zdunik J L 2000 Astron. Astrophys. 359 311
[16] Harko T and Cheng K S 2002 Astron. Astrophys. 385 947
[17] Zong H S and Sun W M 2008 Phys. Rev. D 78 054001
[18] Roberts C D and Williams A G 1994 Prog. Part. Nucl. Phys. 33 477
[19] Roberts C D and Schmidt S M 2000 Prog. Part. Nucl. Phys. 45 S1 1
[20] Maris P and Roberts C D 2003 Int. J. Mod. Phys. E 12 297
[21] Alkofer R and Smekal L Von 2001 Phys. Rep. 353 281
[22] Zong H S et al 2005 Phys. Rev. C 71 015205
[23] Hou F Y et al 2005 Phys. Rev. C 72 034901
[24] Alkofer R et al 2004 Phys. Rev. D 70 014014
[25] Halasz M A et al 1998 Phys. Rev. D 58 096007
[26] Blaschke D et al 1999 Phys. Lett. B 450 207
[27] Peshier A, Kämpfer B and Soff G 2000 Phys. Rev. C 61 045203
[28] Schertler K, Greiner C, Schaffner-Bielich J and Thoma M H 2000 Nucl. Phys. A 677 463
[29] Özel F 2006 Nature 441 1115
[30] Alford M and Braby M 2005 Astrophys. J. 629 969
[31] Lattimer J M and Prakash M 2001 Astrophys. J. 550 426
[32] Bublla M et al 2004 Phys. Lett. B 595 36
Related articles from Frontiers Journals
[1] ZHAO Xian-Feng. The Surface Gravitational Redshift of a Proto Neutron Star[J]. Chin. Phys. Lett., 2010, 27(9): 121202
[2] GUO Xiao-Bo, TAO Jun, LI Lei, WANG Shun-Jin,. Light Flavor Vector and Pseudo Vector Mesons from a Light-Cone QCD Inspired Effective Hamiltonian Model with SU(3) Flavor Mixing Interactions[J]. Chin. Phys. Lett., 2010, 27(6): 121202
[3] FU Yong-Ping, LI Yun-De . Intermediate Mass Dileptons from the Passage of Jets and High Energy Photons through Quark-Gluon Plasma[J]. Chin. Phys. Lett., 2010, 27(10): 121202
[4] GUO Xiao-Bo, TAO Jun, LI Lei, ZHOU Shan-Gui, WANG Shun-Jin,. A Light-Cone QCD Inspired Effective Hamiltonian Model with SU(3) Flavor Mixing[J]. Chin. Phys. Lett., 2009, 26(4): 121202
[5] FU Yong-Ping, LI Yun-De. Jet-Photon Production at RHIC and LHC[J]. Chin. Phys. Lett., 2009, 26(11): 121202
[6] TAO Jun, LI Lei, ZHOU Shan-Gui, WANG Shun-Jin. A Light-Cone QCD Inspired Effective Hamiltonian Model for Pseudoscalar and Scalar Mesons[J]. Chin. Phys. Lett., 2008, 25(9): 121202
[7] WANG Guo-Hua, FU Wei-Jie and LIU Yu-Xin,. Comparison of Properties of the Simplest Neutron Stars in Three RMF Models[J]. Chin. Phys. Lett., 2008, 25(8): 121202
[8] JIN Hong-Ying, LIU Shao-Min, ZHANG Zhu-Feng, LI Xue-Qian. Chiral Suppression and SU(3) Symmetry in Scalar Glueball Decays[J]. Chin. Phys. Lett., 2008, 25(5): 121202
[9] ZHANG Ying, WANG Qing. Gauge Covariant Fermion Propagator in the Presence of Arbitrary External Gauge Field and Its Schwinger--Dyson Equation[J]. Chin. Phys. Lett., 2008, 25(4): 121202
[10] WANG Zhi-Gang, WANG Zhi-Bin. Analysis of Vertex D*D*ρ with Light-Cone QCD Sum Rules[J]. Chin. Phys. Lett., 2008, 25(2): 121202
[11] HE Deng-Ke, JIANG Yu, FENG Hong-Tao, SUN Wei-Min, ZONG Hong-Shi,. Quark-Number Susceptibility at Finite Chemical Potential and Zero Temperature[J]. Chin. Phys. Lett., 2008, 25(2): 121202
[12] ZENG Dai-Min, WU Xing-Gang, FANG Zhen-Yun. B→K Transition Form Factor with Tensor Current within the kT Factorization Approach[J]. Chin. Phys. Lett., 2008, 25(2): 121202
[13] WANG Zhi-Gang. Reanalysis of the (0+,1+) States Bs0 and Bs1 with QCD Sum Rules[J]. Chin. Phys. Lett., 2008, 25(11): 121202
[14] HUANG Tao, ZUO Fen. Remarks on Two-Dimensional Power Correction in Soft Wall Model[J]. Chin. Phys. Lett., 2008, 25(10): 121202
[15] LI Lei, WANG Shun-Jin, ZHOU Shan-Gui, ZHANG Guang-Biao. A Light-Cone QCD Inspired Meson Model with a Relativistic Confining Potential in Momentum Space[J]. Chin. Phys. Lett., 2007, 24(2): 121202
Viewed
Full text


Abstract