Chinese Physics C > 1999, Vol. 23 > Issue(7): 681-688

Study of the Equation of State of Nuclear Matter

Department of physics, Zhongshan University, Guangzhou 510275

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Abstract：
In this paper, the fomulations of the energy density and pressure density of nuclear matter are derived in detail in one loop approximation in the relativistic σ-ω model. The changing of the binding energy and pressure with density is calculated numerically, and the pressure density is calculated in thermodynamics and hydrodynamics respechvely. We conclude that the pressure density in these two formalisms are similar.

References

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Fetter A L, Walecka J D. Quantum Theory of Many–Particle systems. New York: McGraw–hillBookCompany, 1971, 341–348 2 Serot B D, Walecka J D. Rescent Progress in Quantum Hadrodynamics. 1996. To be published inInternational Journal of Modem Physics. 8–10 3 Chin S N Ann of Phys., 1977, 108: 301–3214 Serot B D, Walecka J D. The nuclear manybody problem In: Negele J w. Erich Vogt Adv. N. Phys., 16.New York: Plenum press, 1986. 11–45 5 Liu L G, Bentz W, Arima A. Ann of Phys., 1989, 194: 387–395 6 Furnstahl R J, Serot B D. Phys. Rev., 1990 C41:262–2797 Tauaha K, Bentz W. Nucl. Phys., 1992, A540: 383–389 8 Barbett R M, Carone C D, Groom C D et al. Phys. Rev., 1996, D54: 25–48 9 Mjamdar M M, Samadar S R. Phys. Rev., 1994, C49: 541–543 10 Cheng K S, Dai Z G, Yao C C. Astro. Jou., 1996, 464: 348–353

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Chen Wei, Mei Zhonghao and Liu Lianggang. Study of the Equation of State of Nuclear Matter[J]. Chinese Physics C, 1999, 23(7): 681-688.

Chen Wei, Mei Zhonghao and Liu Lianggang. Study of the Equation of State of Nuclear Matter[J]. Chinese Physics C, 1999, 23(7): 681-688. shu

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Received: 1998-05-20
Revised: 1900-01-01

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沈阳化工大学材料科学与工程学院沈阳 110142

Study of the Equation of State of Nuclear Matter

Corresponding author:Chen Wei,

Department of physics, Zhongshan University, Guangzhou 510275

Received Date:1998-05-20
Accepted Date:1900-01-01
Available Online:1999-07-05

Abstract:In this paper, the fomulations of the energy density and pressure density of nuclear matter are derived in detail in one loop approximation in the relativistic σ-ω model. The changing of the binding energy and pressure with density is calculated numerically, and the pressure density is calculated in thermodynamics and hydrodynamics respechvely. We conclude that the pressure density in these two formalisms are similar.