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

Autor(en)

, C. Domingo-Pardo, V. Babiano-Suarez, J. Balibrea-Correa, L. Caballero, Ion Ladarescu, J. Lerendegui-Marco, J. L. Tain, F. Calvino, A. Casanovas, A. Segarra, A. E. Tarifeno-Saldivia, C. Guerrero, M. A. Millan-Callado, J. M. Quesada, M. T. Rodriguez-Gonzalez, 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. Caamano, M. Calviani, D. Cano-Ott, F. Cerutti, E. Chiaveri, N. Colonna, G. P. Cortes, M. A. Cortes-Giraldo, L. Cosentino, S. Cristallo, L. A. Damone, P. J. Davies, M. Diakaki, M. Dietz, R. Dressler, Q. Ducasse, E. Dupont, Adil Duran, Z. Eleme, B. Fernandez-Domingez, A. Ferrari, Ferro-Goncalves, A. Wallner, Andreas Pavlik

Abstrakt

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(en)

Isotopenphysik

Externe Organisation(en)

Instituto de Física Corpuscular (IFIC), Universidad Internacional de Valencia, Universidad de Sevilla, Universitat Politècnica de Catalunya, Centro de Investigaciones Energeticas Medioambientales y Tecnológica, Istituto Nazionale di Fisica Nucleare (INFN), Roma, Università degli Studi di Catania, Medical University of Lodz, Centre National de la Recherche Scientifique (CNRS), Reims, Centre National de la Recherche Scientifique (CNRS), Strasbourg , Icm & Sorbonne University, UMR EcoSys, European Organization for Nuclear Research (CERN), Technische Universität Wien, DIF, CEA, DAM, CEA, Manchester Metropolitan University, University of Zagreb, York University, Università degli Studi di Perugia, Universidade de Santiago de Compostela (USC), Instituto Nazionale die Astrofisica (INAF), Università degli Studi di Bari Aldo Moro, National Technical University of Athens (NTUA), University of Edinburgh, Physikalisch-Technische Bundesanstalt, University of Ioannina, Universidade Técnica de Lisboa, Instituto Superior Técnico, Australian National University

Journal

Journal of Physics: Conference Series

Band

1668

Anzahl der Seiten

13

ISSN

1742-6588

DOI

https://doi.org/10.1088/1742-6596/1668/1/012013

Publikationsdatum

2020

Peer-reviewed

Ja

ÖFOS 2012

103014 Kernphysik

Schlagwörter

ASJC Scopus Sachgebiete

Allgemeine Physik und Astronomie

Link zum Portal

https://ucrisportal.univie.ac.at/de/publications/c04ba653-e3dd-41b1-adc1-ec2a2e694483