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A sine-Gordon soliton star model with the action of exotic matter and dark energy is studied in this article, the solutions of state equation and mass of star are calculated by using field equation. We found that the density and pressure of matter are connected with the soliton state and the mass of star. Moreover, star equilibrium and stability of dark energy are analyzed and discussed, the result shown that the state of soliton star interior exist in the form of mixed state.
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Keywords:
- exotic matter /
- dark energy /
- sine-Gordon soliton star
[1] Perlmutter S, Turner M S, White M 1999 Phys. Rev. Lett. 83 670
[2] Riess A G, Nugent P E, Schmidt B P 2001 Astrophys. J. 560 49
[3] Bennett C L, Halpern, Hinshaw 2003 Astrophys. J. Suppl.148 1
[4] Chen J H, Wang Y J 2008 Chin. Phys. B 17 1184
[5] Wang Y T, Xu LX, Lu J B , Gui Y X 2010 Chin. Phys. B 19 019801
[6] Cui J L, Zhang L , Zhang J F, Zhang X 2010 Chin. Phys. B 19 019802
[7] Chapline G, Hohlfeld E, Laughlin R B, Santiago D I 2003 Int. J. Mod. Phys. A 18 3587
[8] Mazur P, Mottola E 2004 Proc. Nat. Acad. Sci. 101 9545
[9] Bertolami O, Paramos J 2005 Phys.Rev.D 72 123512
[10] Cattoen C, Faber T, Visser M 2005 Class. Quant. Grav. 22 4189
[11] Lobo F S N 2006 Class. Quant. Grav. 23 1525
[12] Liu L, Pei S Y 2006 Acta Phys. Sin. 55 4980 (in Chinese) [刘 辽、裴寿镛 2006 物理学报 55 4980]
[13] Lobo F, Arellano A 2007 Class. Quant. Grav. 24 1069
[14] DeBenedictis A, Garattini R, Lobo F 2008 Phys.Rev.D 78 104003
[15] Deng Q, Yan J 2008 Acta Phys. Sin. 57 3978 (in Chinese) [邓 强、颜 骏 2008 物理学报 57 3978]
[16] Yan J 2009 Commun. Theor. Phys. 52 1015
[17] T D Lee 1987 Phys.Rev.D 35 3637
[18] Cadoni M 2005 Class. Quant. Grav.22 409
[19] Yan J, Qiu X M 1998 Gen. Rel. Grav.30 1319
[20] Yan J, Wang S J, Tao B Y 2001 Commun. Theor. Phys. 35 19
[21] Yan J,Tao B Y 2003 High Energy Phys.Nucl Phys. 27 767 [颜 骏、陶必友 2003 高能物理与核物理 27 767]
[22] Stotzel B 1995 Phys.Rev.D 52 2192
[23] Yu Y Q 1987 Introduction of General Relativity (Beijing: Beijing University Press) p119 (in Chinese) [俞允强 1987 广义相对论引论 (北京:北京大学出版社)第119页]
[24] T D Lee, Y Pang 1992 Phys.Rep. 35 22125
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[1] Perlmutter S, Turner M S, White M 1999 Phys. Rev. Lett. 83 670
[2] Riess A G, Nugent P E, Schmidt B P 2001 Astrophys. J. 560 49
[3] Bennett C L, Halpern, Hinshaw 2003 Astrophys. J. Suppl.148 1
[4] Chen J H, Wang Y J 2008 Chin. Phys. B 17 1184
[5] Wang Y T, Xu LX, Lu J B , Gui Y X 2010 Chin. Phys. B 19 019801
[6] Cui J L, Zhang L , Zhang J F, Zhang X 2010 Chin. Phys. B 19 019802
[7] Chapline G, Hohlfeld E, Laughlin R B, Santiago D I 2003 Int. J. Mod. Phys. A 18 3587
[8] Mazur P, Mottola E 2004 Proc. Nat. Acad. Sci. 101 9545
[9] Bertolami O, Paramos J 2005 Phys.Rev.D 72 123512
[10] Cattoen C, Faber T, Visser M 2005 Class. Quant. Grav. 22 4189
[11] Lobo F S N 2006 Class. Quant. Grav. 23 1525
[12] Liu L, Pei S Y 2006 Acta Phys. Sin. 55 4980 (in Chinese) [刘 辽、裴寿镛 2006 物理学报 55 4980]
[13] Lobo F, Arellano A 2007 Class. Quant. Grav. 24 1069
[14] DeBenedictis A, Garattini R, Lobo F 2008 Phys.Rev.D 78 104003
[15] Deng Q, Yan J 2008 Acta Phys. Sin. 57 3978 (in Chinese) [邓 强、颜 骏 2008 物理学报 57 3978]
[16] Yan J 2009 Commun. Theor. Phys. 52 1015
[17] T D Lee 1987 Phys.Rev.D 35 3637
[18] Cadoni M 2005 Class. Quant. Grav.22 409
[19] Yan J, Qiu X M 1998 Gen. Rel. Grav.30 1319
[20] Yan J, Wang S J, Tao B Y 2001 Commun. Theor. Phys. 35 19
[21] Yan J,Tao B Y 2003 High Energy Phys.Nucl Phys. 27 767 [颜 骏、陶必友 2003 高能物理与核物理 27 767]
[22] Stotzel B 1995 Phys.Rev.D 52 2192
[23] Yu Y Q 1987 Introduction of General Relativity (Beijing: Beijing University Press) p119 (in Chinese) [俞允强 1987 广义相对论引论 (北京:北京大学出版社)第119页]
[24] T D Lee, Y Pang 1992 Phys.Rep. 35 22125
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