Abstract
Bismuth capture of neutrons is the termination point of the s-process cycle of nucleosynthesis in stellar
environments. A new measurement is reported here for neutron activation of bismuth with an intense quasi-
Maxwellian neutron source at kT ∼ 30 keV. The measurement was performed at the SARAF phase I accelerator
facility by bombarding a 1.5-mA proton beam on the liquid-lithium larget. The cross section of the 209Bi(n,γ )
capture reaction leading to the 210Bi ground state was determined by combining β measurements from the 210gBi
decay and α and γ from the subsequent 210Po decay, along with detailed Monte Carlo simulations of the 7Li(p,n)
reaction kinematics and the activation experimental setup. Deduced Maxwellian averaged cross sections (MACS)
for 209Bi(n,γ )210gBi at kT = 30 keV using the ENDF and JENDL databases for the corrections and extrapolations
yielded a value of 1.86 ± 0.08 mb. A comparison is made with previous measurements, including time-of-flight
(TOF) measurements of the total bismuth capture cross section. Plans for obtaining the MACS for capture to the
bismuth-210 metastable state in the reaction 209Bi(n,γ )210mBi are discussed, along with estimates based on our
results in comparison with TOF measurements. The bismuth neutron activation cross section is also of importance
for design of GenIV reactor coolant and subcritical accelerator driven systems, especially in light of the 3 million
year half-life of the 210mBi isomer.
Original language | English |
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Article number | 055805 |
Number of pages | 14 |
Journal | Physical Review C |
Volume | 96 |
DOIs | |
State | Published - 15 Nov 2017 |