Measurement of the 159Tb(n, γ) cross section at the CSNS Back-n facility

Subjects: Physics >> Nuclear Physics submitted time 2023-06-20

S. Zhang G. Li W. Jiang D.X. Wang J. Ren M. Huang E.T. Li J.Y. Tang X.C. Ruan H.W. Wang Z.H. Li Y.S. Chen L.X. Liu, X.X. Li Q.W. Fan R.R. Fan X.R. Hu J.C. Wang X. Li D.D. Niu

Abstract： The stellar (n, γ) cross section data for the mass numbers around A ≈ 160 are of key importance to nucleosynthesis in the main component of the slow neutron capture process, which occurs in the thermally pulsing asymptotic giant branch (TP–AGB). The new measurement of (n, γ) cross sections for ¹⁵⁹Tb was performed using the C6D6 detector system at the back streaming white neutron beam line (Back-n) of the China spallation neutron source (CSNS) with neutron energies ranging from 1 eV to 1 MeV. Experimental resonance capture kernels are reported up to 1.2 keV neutron energy with this capture measurement. Maxwellian-averaged cross sections (MACS) are derived from the measured 159Tb (n, γ) cross sections at kT = 5–100 keV and are in good agreement with the recommended data of KADoNiS-v0.3 and JEFF-3.3, while KADoNiS-v1.0 and ENDF-VIII.0 signifificantly overestimate the present MACS up to 40% and 20%, respectively. A sensitive test of the s-process nucleosynthesis is also performed with the stellar evolution code MESA. Signifificant changes in abundances around A ≈ 160 are observed between the ENDF/B-VIII.0 and present measured rate of ¹⁵⁹Tb(n, γ) ¹⁶⁰Tb in the MESA simulation.

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