4.4 Article

Neutron-capture rates for explosive nucleosynthesis: the case of 68Ni(n,γ)69Ni

出版社

IOP Publishing Ltd
DOI: 10.1088/1361-6471/aa5ae7

关键词

nuclear astrophysics; r process; nucleosynthesis; neutron-capture reactions; nuclear level density,gamma-ray strength function

资金

  1. Research Council of Norway [205528, 210007]
  2. ERC-STG [637686]
  3. LLNL [DE-AC52-07NA27344]
  4. NNSA of the US Department of Energy at Los Alamos National Laboratory [DE-AC52-06NA25396]
  5. National Science Foundation [PHY.1102511, PHY.1430152, PHY.1350234]
  6. Department of Energy/National Nuclear Security Administration [DE-NA0003221, DE-NA-0000979, DE-NA-0002132]
  7. Division Of Physics
  8. Direct For Mathematical & Physical Scien [1430152, 1350234, 1565546] Funding Source: National Science Foundation

向作者/读者索取更多资源

Neutron-capture reactions play an important role in heavy element nucleosynthesis, since they are the driving force for the two processes that create the vast majority of the heavy elements. When a neutron capture occurs on a short-lived nucleus, it is extremely challenging to study the reaction directly and therefore the use of indirect techniques is essential. The present work reports on such an indirect measurement that provides strong constraints on the Ni-68(n,gamma) Ni-69 reaction rate. This is done by populating the compoundnucleus Ni-69 via the beta decay of Co-69 and measuring the.-ray deexcitation of excited states in 69Ni. The beta-Oslo method was used to extract the gamma-ray strength function and the nuclear level density. In addition the half-life of 69Co was extracted and found to be in agreement with previous literature values. Before the present results, the Ni-68(n,gamma) 69Ni reaction was unconstrained and the purely theoretical reaction rate was highly uncertain. The new uncertainty on the reaction rate based on the present experiment (variation between upper and lower limit) is approximately a factor of 3. The commonly used reaction libraries JINA-REACLIB and BRUSLIB are in relatively good agreement with the experimental rate. The impact of the new rate on weak r-process calculations is discussed.

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