Isospin Effect on the Slope Temperature at Backward Angles in the Reactions 30MeV/u 40Ar+112,124Sn

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XIAO Zhi-Gang, WU He-Yu, WANG Hong-Wei, LI Zu-Yu, JIN Gen-Ming, DUAN Li-Min, ZHANG Bao-Guo, HU Rong-Jiang, WEI Zhi-Yong, LIU Yong-Ying, WANG Su-Fang, LU Zhao-Hui, ZHU Yong-Tai and ZHU Hai-Dong. Isospin Effect on the Slope Temperature at Backward Angles in the Reactions 30MeV/u 40Ar+112,124Sn[J]. Chinese Physics C, 2001, 25(7): 643-650.
XIAO Zhi-Gang, WU He-Yu, WANG Hong-Wei, LI Zu-Yu, JIN Gen-Ming, DUAN Li-Min, ZHANG Bao-Guo, HU Rong-Jiang, WEI Zhi-Yong, LIU Yong-Ying, WANG Su-Fang, LU Zhao-Hui, ZHU Yong-Tai and ZHU Hai-Dong. Isospin Effect on the Slope Temperature at Backward Angles in the Reactions 30MeV/u 40Ar+112,124Sn[J]. Chinese Physics C, 2001, 25(7): 643-650. shu
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Received: 2000-07-26
Revised: 1900-01-01
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Isospin Effect on the Slope Temperature at Backward Angles in the Reactions 30MeV/u 40Ar+112,124Sn

    Corresponding author: XIAO Zhi-Gang,
  • Institute of Modern Physics,The Chinese Academy of Sciences,Lanzhou 730000,China

Abstract: The coincidence measurements between residues and light particles have been carried out for the reactions 30MeV/u 40Ar+112,124Sn. The times of flight of the residues are measured by PPACs installed concentrically around the beam at forward angle. The spectra of 3He,α and 6He detected at backward angle in coincidence with residues having different average velocities are analyzed with moving source fit. The average excitation energy of hot nuclei is obtained in the incomplete fusion frame. It is shown that the slope temperature extracted from 3He(6He) spectra is higher (lower) in the neutron-rich system 40Ar+ 124Sn than that in the neutron-deficient system 40Ar+112Sn. For α particle. there is almost no difference between the two reaction systems. The possible causality of these systematic behaviors is discussed from the selectivity of the emitting particles along the decay chain of hot nuclei. The calculation of GEMINI can not repsoduce the experimental observations.

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