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ISOSPIN EFFECTS STUDIED WITH THE CHIMERA DETECTOR AT 35 MeV/NUCLEON

机译:希美拉探测器以35 MeV /核研究的ISOSPIN效应

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摘要

The yield of light charged particles and intermediate mass fragments is studied for the neutron-rich, ~(124)Sn+~(64)Ni, and neutron-poor, ~(112)Sn+~(58)Ni, reactions at 35 MeVucleon as a function of the impact parameter. Our main observations are: (ⅰ) The yields of ~1H, ~3He and ~4He particles in the neutron-poor system are enhanced with respect to the neutron-rich system and the yield of ~3H is suppressed at all impact parameters, (ⅱ) The ratio of ~3H to ~3He yield is three times larger for neutron poor system, (ⅲ) The N/Z ratio of the emitted intermediate-mass fragments shows dependence on the isospin of the system, (ⅳ) The neutron richness of detected intermediate mass fragments depends strongly on their rapidity. The gross features of the experimental data are reproduced by quantum molecular dynamics model calculations.
机译:研究了在35 MeV / V下富中子的〜(124)Sn +〜(64)Ni和贫中子的〜(112)Sn +〜(58)Ni的荷电粒子和中间质量碎片的产率。核子作为影响参数的函数。我们的主要观察结果是:(ⅰ)相对于富中子系统,贫中子系统中〜1H,〜3He和〜4He粒子的产率提高,并且在所有撞击参数下〜3H的产率均得到抑制,( ⅱ)中子差系统的〜3H与〜3He产率之比是三倍,(ⅲ)发射的中间质量碎片的N / Z比显示出依赖于系统的同位旋,(ⅳ)中子富集度检测到的中间质量碎片的数量在很大程度上取决于其速度。实验数据的总体特征通过量子分子动力学模型计算得到。

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