Ta(n,) cross-section measurement and the astrophysical origin of Ta isotope
R. Garg (1 and 2)🇮🇳 · S. Dellmann (3)🇩🇪 · C. Lederer-Woods (1)🇬🇧 · C. G. Bruno (1)🇬🇧 · K. Eberhardt (4) · C. Geppert (4) · T. Heftrich (3)🇩🇪 · I. Kajan (5) · F. Käppeler (6)🇩🇪 · B. Phoenix (7)🇬🇧 · R. Reifarth (3)🇩🇪 · D. Schumann (5)🇨🇭 · M. Weigand (3)🇩🇪 · C. Wheldon (7) ((1) School of Physics and Astronomy, University of Edinburgh, Edinburgh, EH9 3FD, UK, (2) Facility for Rare Isotope Beams, Michigan State University, East Lansing, Michigan, 48824, USA, (3) Goethe Universität Frankfurt, Frankfurt, 60438, Germany, (4) Johannes Gutenberg Universität Mainz, Mainz, 55128, Germany, (5) Paul Scherrer Institute, Villigen, 5232, Switzerland, (6) Karlsruhe Institute of Technology, Campus North, Karlsruhe, 76021, Germany, (7) School of Physics and Astronomy, University of Birmingham, Birmingham, B15 2TT, UK)🇬🇧
Tantalum-180m is nature's rarest (quasi) stable isotope and its astrophysical origin is an open question. A possible production site of this isotope is the slow neutron capture process in Asymptotic Giant Branch stars, where it can be produced via neutron capture reactions on unstable Ta. We report a new measurement of the Ta()Ta cross section at thermal neutron energies via the activation technique. Our results for the thermal and resonance-integral cross-sections are 952 57 b and 2013 148 b, respectively. The thermal cross section is in good agreement with the only previous measurement (Phys. Rev C {\bf 60} 025802, 1999), while the resonance integral is different by a factor of 1.7. While neutron energies in this work are smaller than the energies in a stellar environment, our results may lead to improvements in theoretical predictions of the stellar cross section.