First Results of the 140Ce(n,γ)141Ce Cross-Section Measurement at n_TOF

An accurate measurement of the Ce-140(n,gamma) energy-dependent cross-section was performed at the n_TOF facility at CERN. This cross-section is of great importance because it represents a bottleneck for the s-process nucleosynthesis and determines to a large extent the cerium abundance in stars. The measurement was motivated by the significant difference between the cerium abundance measured in globular clusters and the value predicted by theoretical stellar models. This discrepancy can be ascribed to an overestimation of the Ce-140 capture cross-section due to a lack of accurate nuclear data. For this measurement, we used a sample of cerium oxide enriched in Ce-140 to 99.4%. The experimental apparatus consisted of four deuterated benzene liquid scintillator detectors, which allowed us to overcome the difficulties present in the previous measurements, thanks to their very low neutron sensitivity. The accurate analysis of the p-wave resonances and the calculation of their average parameters are fundamental to improve the evaluation of the Ce-140 Maxwellian-averaged cross-section.

Automated summary

The accurate measurement of the Ce-140(n,gamma) energy-dependent cross-section provides crucial insights into the cerium abundance in stars. By using a sample enriched in Ce-140 to 99.4%, the study aimed to address the discrepancy between measured cerium abundance in globular clusters and the predictions from theoretical models. The analysis of p-wave resonances and calculation of their parameters are essential in improving the evaluation of the Ce-140 Maxwellian-averaged cross-section.