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Volume 34 Issue 3
Jul.  2017
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QIAO Chunyuan, MA Chunwang, NIU Fei, XU Jingli, DING Tiantian, SONG Yidan. Study of the Nuclear Matter Symmetry Energy in the Simulated 140 AMeV 58,64Ni+9Be Reactions by Isoscaling Method[J]. Nuclear Physics Review, 2017, 34(3): 525-528. doi: 10.11804/NuclPhysRev.34.03.525
Citation: QIAO Chunyuan, MA Chunwang, NIU Fei, XU Jingli, DING Tiantian, SONG Yidan. Study of the Nuclear Matter Symmetry Energy in the Simulated 140 AMeV 58,64Ni+9Be Reactions by Isoscaling Method[J]. Nuclear Physics Review, 2017, 34(3): 525-528. doi: 10.11804/NuclPhysRev.34.03.525

Study of the Nuclear Matter Symmetry Energy in the Simulated 140 AMeV 58,64Ni+9Be Reactions by Isoscaling Method

doi: 10.11804/NuclPhysRev.34.03.525
Funds:  Science and Technology Innovation Talents Program in Universities of Henan Province(13HASTIT046)
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  • Corresponding author: 10.11804/NuclPhysRev.34.03.525
  • Received Date: 2016-12-06
  • Rev Recd Date: 2017-05-02
  • Publish Date: 2017-07-18
  • We have simulated the reactions 140 AMeV 58,64Ni+9Be by antisymmetric molecular dynamics model (AMD) and studied the evolution of △μn(p)/T with collision time from 20 fm/c to 1 000 fm/c. To study nuclear symmetry energy influencing factors, a comparative analysis has been proceed among theses results with different impact parameters and the difference reactions system. The results show that the impact parameters have a great influence on the symmetry energy of the heavy nucleus, and the greater the asymmerty degree of the system, the greater the influence on the symmetry energy. These results are helpful for the indirect study of the energy dependence of the symmetry energy coefficient of the excited nuclear system.
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Study of the Nuclear Matter Symmetry Energy in the Simulated 140 AMeV 58,64Ni+9Be Reactions by Isoscaling Method

doi: 10.11804/NuclPhysRev.34.03.525
Funds:  Science and Technology Innovation Talents Program in Universities of Henan Province(13HASTIT046)
    Corresponding author: 10.11804/NuclPhysRev.34.03.525

Abstract: We have simulated the reactions 140 AMeV 58,64Ni+9Be by antisymmetric molecular dynamics model (AMD) and studied the evolution of △μn(p)/T with collision time from 20 fm/c to 1 000 fm/c. To study nuclear symmetry energy influencing factors, a comparative analysis has been proceed among theses results with different impact parameters and the difference reactions system. The results show that the impact parameters have a great influence on the symmetry energy of the heavy nucleus, and the greater the asymmerty degree of the system, the greater the influence on the symmetry energy. These results are helpful for the indirect study of the energy dependence of the symmetry energy coefficient of the excited nuclear system.

QIAO Chunyuan, MA Chunwang, NIU Fei, XU Jingli, DING Tiantian, SONG Yidan. Study of the Nuclear Matter Symmetry Energy in the Simulated 140 AMeV 58,64Ni+9Be Reactions by Isoscaling Method[J]. Nuclear Physics Review, 2017, 34(3): 525-528. doi: 10.11804/NuclPhysRev.34.03.525
Citation: QIAO Chunyuan, MA Chunwang, NIU Fei, XU Jingli, DING Tiantian, SONG Yidan. Study of the Nuclear Matter Symmetry Energy in the Simulated 140 AMeV 58,64Ni+9Be Reactions by Isoscaling Method[J]. Nuclear Physics Review, 2017, 34(3): 525-528. doi: 10.11804/NuclPhysRev.34.03.525
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