New detection systems for an enhanced sensitivity in key stellar (n,) measurements
J. Lerendegui-Marco · V. Babiano-Suárez · J. Balibrea-Correa · C. Domingo-Pardo · I. Ladarescu · A. Tarifeño-Saldivia · V. Alcayne · D. Cano-Ott · E. González-Romero · T. Martínez · E. Mendoza · C. Guerrero and 8 other authors
Neutron capture cross-section measurements are fundamental in the study of astrophysical phenomena, such as the slow neutron capture (s-) process of nucleosynthesis operating in red-giant and massive stars. However, neutron capture measurements via the time-of-flight (TOF) technique on key -process nuclei are often challenging. Difficulties arise from the limited mass (mg) available and the high sample-related background in the case of the unstable -process branching points. Measurements on neutron magic nuclei, that act as -process bottlenecks, are affected by low (n,) cross sections and a dominant neutron scattering background. Overcoming these experimental challenges requires the combination of facilities with high instantaneous flux, such as n\_TOF-EAR2, with detection systems with an enhanced detection sensitivity and high counting rate capabilities. This contribution reviews some of the latest detector developments in detection systems for (n,) measurements at n\_TOF, such as i-TED, an innovative detection system which exploits the Compton imaging technique to reduce the dominant neutron scattering background and s-TED, a highly segmented total energy detector intended for high flux facilities. The discussion will be illustrated with results of the first measurement of key the -process branching-point reaction Se(n,).