Publications

Review and new concepts for neutron-capture measurements of astrophysical interest

Author(s)
C. Domingo-Pardo, V. Babiano-Suarez, J. Balibrea-Correa, L. Caballero, I. Ladarescu, J. Lerendegui-Marco, J. L. Tain, F. Calviño, A. Casanovas, A. Segarra, A. E. Tarifeño-Saldivia, C. Guerrero, M. A. Millán-Callado, J. M. Quesada, M.T. Rodríguez-González, O. Aberle, V. Alcayne, S. Amaducci, J. Andrzejewski, L. Audouin, M. Bacak, M. Barbagallo, S. Bennett, E. Berthoumieux, D. Bosnar, A. S. Brown, M. Busso, M. Caamaño, M. Calviani, D. Cano-Ott, F. Cerutti, E. Chiaveri, N. Colonna, G. P. Cortés, M. A. Cortés-Giraldo, L. Cosentino, S. Cristallo, L. A. Damone, P. J. Davies, M. Diakaki, M. Dietz, R. Dressler, Q. Ducasse, E. Dupont, I. Durán, Z. Eleme, B. Fernández-Domíngez, A. Ferrari, I. Ferro-Gonçalves, P. Finocchiaro, V. Furman, R. Garg, A. Gawlik, S. Gilardoni, K. Göbel, E. González-Romero, F. Gunsing, J. Heyse, D. G. Jenkins, E. Jericha, U. Jiri, A. Junghans, Y. Kadi, F. Käppeler, A. Kimura, I. Knapová, M. Kokkoris, Y. Kopatch, M. Krticka, D. Kurtulgil, C. Lederer-Woods, S.-J. Lonsdale, D. Macina, A. Manna, T. Martínez, A. Masi, C. Massimi, P. F. Mastinu, M. Mastromarco, E. Maugeri, A. Mazzone, E. Mendoza, A. Mengoni, V. Michalopoulou, P. M. Milazzo, F. Mingrone, J. Moreno-Soto, A. Musumarra, A. Negret, F. Ogállar, A. Oprea, N. Patronis, A. Pavlik, J. Perkowski, C. Petrone, L. Piersanti, E. Pirovano, I. Porras, J. Praena, D. Ramos Doval, R. Reifarth, D. Rochman, C. Rubbia, M. Sabaté-Gilarte, A. Saxena, P. Schillebeeckx, D. Schumann, A. Sekhar, A. G. Smith, N. Sosnin, P. Sprung, A. Stamatopoulos, G. Tagliente, L. Tassan-Got, B. Thomas, P. Torres-Sánchez, A. Tsinganis, S. Urlass, S. Valenta, G. Vannini, V. Variale, P. Vaz, A. Ventura, D. Vescovi, V. Vlachoudis, R. Vlastou, A. Wallner, P. J. Woods, T. J. Wright, P. Žugec
Abstract

The idea of slow-neutron capture nucleosynthesis formulated in 1957 triggered a tremendous experimental effort in different laboratories worldwide to measure the relevant nuclear physics input quantities, namely (n, γ) cross sections over the stellar temperature range (from few eV up to several hundred keV) for most of the isotopes involved from Fe up to Bi. A brief historical review focused on total energy detectors will be presented to illustrate how advances in instrumentation have led to the assessment of new aspects of s-process nucleosynthesis and to the progressive refinement of stellar models. A summary will be presented on current efforts to develop new detection concepts, such as the Total-Energy Detector with γ-ray imaging capability (i-TED). The latter is based on the simultaneous combination of Compton imaging with neutron time-of-flight (TOF) techniques, in order to achieve a superior level of sensitivity and selectivity in the measurement of stellar neutron capture rates.

Organisation(s)
Isotope Physics
External organisation(s)
Gran Sasso Science Institute (GSSI), Australian National University
Journal
Journal of Physics: Conference Series
Volume
1668
No. of pages
13
ISSN
1742-6588
DOI
https://doi.org/10.1088/1742-6596/1668/1/012013
Publication date
2020
Peer reviewed
Yes
Austrian Fields of Science 2012
103014 Nuclear physics
Portal url
https://ucris.univie.ac.at/portal/en/publications/review-and-new-concepts-for-neutroncapture-measurements-of-astrophysical-interest(c04ba653-e3dd-41b1-adc1-ec2a2e694483).html