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Calculation of the structural properties of asymmetrical nuclear matter

Calculation of the structural properties of asymmetrical nuclear matter
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摘要 The structural properties of asymmetrical nuclear matter have been calculated,employing the AV 18 potential for different values of proton to neutron ratio.These calculations have also been made for the case of symmetrical nuclear matter with the UV14,AV14 and AV 18 potentials.In our calculations,we used the lowest order constrained variational method to compute the correlation function of the system. The structural properties of asymmetrical nuclear matter have been calculated,employing the AV 18 potential for different values of proton to neutron ratio.These calculations have also been made for the case of symmetrical nuclear matter with the UV14,AV14 and AV 18 potentials.In our calculations,we used the lowest order constrained variational method to compute the correlation function of the system.
出处 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2012年第3期345-358,共14页 天文和天体物理学研究(英文版)
基金 supported by the Research Institute for Astronomy and Astrophysics of Maragha
关键词 stars:neutron—dense matter—equation of state stars:neutron—dense matter—equation of state
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