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Volume 34 Issue 3
Jul.  2017
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YAN Shengquan, LI Zhihong, WANG Youbao, K. Nishio, H. Maki, SU Jun, LI Yunju, I. Nishinaka, K. Hirose, HAN Yinlu, GUO Bing, ZENG Sheng, LIAN Gang, CHEN Yongshou, LIU Weiping. Indirect Measurement of 95Zr(n, γ)96Zr[J]. Nuclear Physics Review, 2017, 34(3): 420-424. doi: 10.11804/NuclPhysRev.34.03.420
Citation: YAN Shengquan, LI Zhihong, WANG Youbao, K. Nishio, H. Maki, SU Jun, LI Yunju, I. Nishinaka, K. Hirose, HAN Yinlu, GUO Bing, ZENG Sheng, LIAN Gang, CHEN Yongshou, LIU Weiping. Indirect Measurement of 95Zr(n, γ)96Zr[J]. Nuclear Physics Review, 2017, 34(3): 420-424. doi: 10.11804/NuclPhysRev.34.03.420

Indirect Measurement of 95Zr(n, γ)96Zr

doi: 10.11804/NuclPhysRev.34.03.420
Funds:  National Key Research and Development Plan(2016YFA0400502); National Natural Science Foundation of China (11375269, 11490560, 11321064); National Basic Research Program of China(973 Program)(2013CB834406)
  • Received Date: 2016-11-21
  • Rev Recd Date: 2017-04-13
  • Publish Date: 2017-07-18
  • 95Zr(n, γ)96Zr cross section is important for the study of stellar evolution and heavy elements nucleosynthesis because the reaction is the only way to produce the 96Zr in Asymptotic giant branch stars. The direct measurement of 95Zr(n, γ)96Zr is very difficult due to the short half-life of 95Zr, 64 days. The surrogate ratio method was carried out to measure 95Zr(n, γ)96Zr cross sections. We measured the 94Zr(18O, 16Oγ)96Zr and 90Zr(18O, 16Oγ)92Zr reactions and obtained the γ-decay probability ratio of compound nuclei 96Zr* and 92Zr*. The 95Zr(n, γ)96Zr cross section is determined by the obtained ratio multiplying the known 91Zr(n, γ)92Zr cross section at En=0~8 MeV.
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Indirect Measurement of 95Zr(n, γ)96Zr

doi: 10.11804/NuclPhysRev.34.03.420
Funds:  National Key Research and Development Plan(2016YFA0400502); National Natural Science Foundation of China (11375269, 11490560, 11321064); National Basic Research Program of China(973 Program)(2013CB834406)

Abstract: 95Zr(n, γ)96Zr cross section is important for the study of stellar evolution and heavy elements nucleosynthesis because the reaction is the only way to produce the 96Zr in Asymptotic giant branch stars. The direct measurement of 95Zr(n, γ)96Zr is very difficult due to the short half-life of 95Zr, 64 days. The surrogate ratio method was carried out to measure 95Zr(n, γ)96Zr cross sections. We measured the 94Zr(18O, 16Oγ)96Zr and 90Zr(18O, 16Oγ)92Zr reactions and obtained the γ-decay probability ratio of compound nuclei 96Zr* and 92Zr*. The 95Zr(n, γ)96Zr cross section is determined by the obtained ratio multiplying the known 91Zr(n, γ)92Zr cross section at En=0~8 MeV.

YAN Shengquan, LI Zhihong, WANG Youbao, K. Nishio, H. Maki, SU Jun, LI Yunju, I. Nishinaka, K. Hirose, HAN Yinlu, GUO Bing, ZENG Sheng, LIAN Gang, CHEN Yongshou, LIU Weiping. Indirect Measurement of 95Zr(n, γ)96Zr[J]. Nuclear Physics Review, 2017, 34(3): 420-424. doi: 10.11804/NuclPhysRev.34.03.420
Citation: YAN Shengquan, LI Zhihong, WANG Youbao, K. Nishio, H. Maki, SU Jun, LI Yunju, I. Nishinaka, K. Hirose, HAN Yinlu, GUO Bing, ZENG Sheng, LIAN Gang, CHEN Yongshou, LIU Weiping. Indirect Measurement of 95Zr(n, γ)96Zr[J]. Nuclear Physics Review, 2017, 34(3): 420-424. doi: 10.11804/NuclPhysRev.34.03.420
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