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In this paper we mainly investigate, in the framework of effective mass bag model, how the coupling constant and the bag constant execute their effects on equations of state of strange quark matter, and on the properties of strange stars. Numerical results indicate that with the increase of strong coupling constant and bag constant, equations of state for strange quark matter turn softened, whereas gravitational mass and corresponding radius of strange stars become decreased. For instance the mass of the star decreases from 1.43M⊙(M⊙=1.991030 kg)to 1.25M⊙ and corresponding radius decreases from 8.3 km to 7.7 km while the coupling constant varies from 0.5 to 2.0. As for strange stars, the corresponding values decrease from 1.47M⊙to 1.22M⊙ and 8.6 km and 7.4 km respectively while the bag constant B1/4 increases from 160 MeV to 175 MeV.
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Keywords:
- model parameters /
- strange star /
- equations of state /
- mass-radius relations
[1] Witten E 1984 Phys. Rev.D 30 272
[2] [3] Dai Z G, Lu T 1994 Acta Phys. Sin. 43 198 (in Chinese) [戴子高、陆 埮 1994 43 198]
[4] [5] Dai Z G, Lu T, Peng Q H 1993 Acta Phys. Sin. 42 1210 (in Chinese) [戴子高、陆 埮、彭秋和 1993 42 1210]
[6] [7] Lai X J, Luo Z Q, Liu J J, Liu H L 2008 Acta Phys. Sin. 57 1535 (in Chinese) [赖祥军、罗志全、刘晶晶、刘宏林 2008 57 1535]
[8] [9] Chodos A, Jaffe R L, Johnson K 1974 Phys. Rev. D 9 3471
[10] [11] Fowler G N, Raha S, Weiner R M 1981 Z. Physics C 9 271
[12] Peng G X, Qiang H C, Zou B S, Ning P Z, Luo S J 2000 Phys. Rev. C 62 025801
[13] [14] [15] Peng G X, Qiang H C, Yang J J, Li L, Liu B 1999 Phys. Rev. C 61 015201
[16] [17] Nambu Y, Jona-Lasinio G 1961 Phys. Rev. 124 246
[18] Buballa M, Oertel M 1999 Phys. Lett. B 457 261
[19] [20] Schertler K, Greiner C, Thoma M H 1997 Nucl. Phys. A 616 659
[21] [22] [23] Bao T, Liu G Z, Zhao E G, Zhu M F 2008 Eur. Phys. J. A 38 287
[24] Oppenheimer J R, Schwinger J S 1939 Phys. Rev. 56 1066
[25] [26] Tolman R C 1939 Phys. Rev. 55 364
[27] -
[1] Witten E 1984 Phys. Rev.D 30 272
[2] [3] Dai Z G, Lu T 1994 Acta Phys. Sin. 43 198 (in Chinese) [戴子高、陆 埮 1994 43 198]
[4] [5] Dai Z G, Lu T, Peng Q H 1993 Acta Phys. Sin. 42 1210 (in Chinese) [戴子高、陆 埮、彭秋和 1993 42 1210]
[6] [7] Lai X J, Luo Z Q, Liu J J, Liu H L 2008 Acta Phys. Sin. 57 1535 (in Chinese) [赖祥军、罗志全、刘晶晶、刘宏林 2008 57 1535]
[8] [9] Chodos A, Jaffe R L, Johnson K 1974 Phys. Rev. D 9 3471
[10] [11] Fowler G N, Raha S, Weiner R M 1981 Z. Physics C 9 271
[12] Peng G X, Qiang H C, Zou B S, Ning P Z, Luo S J 2000 Phys. Rev. C 62 025801
[13] [14] [15] Peng G X, Qiang H C, Yang J J, Li L, Liu B 1999 Phys. Rev. C 61 015201
[16] [17] Nambu Y, Jona-Lasinio G 1961 Phys. Rev. 124 246
[18] Buballa M, Oertel M 1999 Phys. Lett. B 457 261
[19] [20] Schertler K, Greiner C, Thoma M H 1997 Nucl. Phys. A 616 659
[21] [22] [23] Bao T, Liu G Z, Zhao E G, Zhu M F 2008 Eur. Phys. J. A 38 287
[24] Oppenheimer J R, Schwinger J S 1939 Phys. Rev. 56 1066
[25] [26] Tolman R C 1939 Phys. Rev. 55 364
[27]
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