학술논문
New detection systems for an enhanced sensitivity in key stellar (n,γ) measurements.
Document Type
Article
Author
Lerendegui-Marco, J.; Babiano-Suárez, V.; Balibrea-Correa, J.; Domingo-Pardo, C.; Ladarescu, I.; Tarifeño-Saldivia, A.; Alcayne, V.; Cano-Ott, D.; González-Romero, E.; Martínez, T.; Mendoza, E.; Guerrero, C.; Calviño, F.; Casanovas, A.; Köster, U.; Chiera, N. M.; Dressler, R.; Maugeri, E. A.; Schumann, D.; Aberle, O.
Source
Subject
*NEUTRON capture
*NUCLEAR reactions
*NUCLEOSYNTHESIS
*NUCLEAR astrophysics
*SUPERGIANT stars
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Language
ISSN
2101-6275
Abstract
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 s-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 s-process branching points. Measurements on neutron magic nuclei, that act as s-process bottlenecks, are affected by low (n,γ) cross sections and a dominant neutron scattering background. Overcoming these experimental challenges requires the combination of facilities with high instantaneous flux, such as n_TOFEAR2, 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,γ) 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 s-process branching-point reaction 79Se(n,γ). [ABSTRACT FROM AUTHOR]