In-Medium Effects on Neutron Stars

  • Using the Bonn potential plus the BR scaling parameter induced by in-medium effects,the modified relativistic mean field model proposed recently is applied to investigate the properties of neutron star. The obtained results show that the BR scaling parameter leads to the increasing of maximum masses and radii of neutron star.
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  • [1] Walecka J D. Ann. Phys., 1974,83:4918–5292 Serot B D, Walecka J D. Adv. Nucl. Phys. ,1986,16:1–321 3 Mailer H, Serot B D. Phys. Rev.,1995,C52:2072–2091 4 Müller H. Nucl. Phys., 1997,A615:349–3705 Mailer H,Serot B D.Nucl. Phys.,1996,A606:508–537 6 Delfino A,Coelho C T, Malheiro M. Phys. Rev., 1995,C51:2188–2195 7 Furnstahl R J, Serot B D. Phys. Rev., 1990, C41: 262–279; Phys. Rev., 1991,C43:105–129 8 Glendening N K. Nucl. Phys. ,1987,A469:600–616 9 Yoshida H, Sagawa H, Takigawa N. Phys. Rev., 1998, C58: 2796–280610 Malheiro M,Delfino A, Coelho C T.Phys. Rev.,1998,C58:426–43311 Haddad S, Weigel M K.Phys. Rev.,1994, C49:3228–3233 12 Fuchs C, Lenske H,Wolter H H.Phys. Rev.,1995,C52:3043–3060 13 Lenske H, Fuchs C. Phys. Rev.,1995, C52:3043–3060 14 Hofmann F, Keil C M, Lenske H. Phys. Lett.,1995,B345:335–36015 Type S, Wolter H H. Nucl. Phys.,1999, A656:331–36416 GUO Hua, LIU B, Toro M D. Phys. Rev.,2000, C62:035203(1) –035203(8)17 LIU B et at. Phys. Rev., 2002,C65:045201(1) –045201(11)18 Kaiser N, Fritseh S, Weise W. Nucl. Phys., 2002, A700:343–35819 LIU Bo et at. High Energy Phys. and Nucl. Phys. ,2002,26:1056–1064(in Chinese) (刘波等.高能物理与核物理,2002,26:1056–1064)20 Tanaka K,Bentz W,Arima A.Nucl. Phys.,1993,A555:151–21421 Bhattacharyya A,Ghosh S K,Phatak S C.Phys. Rev., 1999,C60:044903(1) –044903(5)22 Brown G E, Rho M. Phys. Rev. Lett., 1991,66:2720–2723 23 Song C. Phys. Rep., 2001, 347:289–37124 Song C, Min D P, Rho M.Phys. Lett.,1998, B424:226–234 25 Machleidt R. Adv. Nucl. Phys.,1989,19:189 26 LIU Bo, GUO Hua. High Energy Phys. and Nucl. Phys., 2003, 27(7) :590(in Chinese) (刘波,郭华.高能物理与核物理,2003,27(7) :590) 27 Baym G.Nucl.Phys. ,1995,A590:233c–248c
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LIU Bo and GUO Hua. In-Medium Effects on Neutron Stars[J]. Chinese Physics C, 2003, 27(8): 683-687.
LIU Bo and GUO Hua. In-Medium Effects on Neutron Stars[J]. Chinese Physics C, 2003, 27(8): 683-687. shu
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Received: 2002-11-04
Revised: 1900-01-01
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In-Medium Effects on Neutron Stars

    Corresponding author: LIU Bo,
  • Institute of High Energy Physics, CAS, Beijing 100039, China2 Department of Technical Physics, Peking University, Beijing 100871, China

Abstract: Using the Bonn potential plus the BR scaling parameter induced by in-medium effects,the modified relativistic mean field model proposed recently is applied to investigate the properties of neutron star. The obtained results show that the BR scaling parameter leads to the increasing of maximum masses and radii of neutron star.

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