EPJ Web Conf.
Volume 165, 2017Nuclear Physics in Astrophysics VIII (NPA8 2017)
|Number of page(s)||4|
|Published online||30 December 2017|
A new method for the determination of very small Γγ partial widths
1 INFN-Sez.Catania, Catania, Italy
2 LNS-INFN, Catania, Italy
3 Dipartimento di Fisica e Astronomia Università di Catania, Catania, Italy
4 Dip. di Scienze Mat. e Inf., Scienze Fisiche e Scienze della Terra Università di Messina, Italy
5 Facoltà di Ingegneria e Architettura, Universit Kore, Enna, Italy
6 INFN sezione di Milano and Dip. di Fisica Università di Milano, Italy
7 Instituto de Fsica, Universidad Nacional Autnoma de Mexico, Mexico
8 INFN sezione di Firenze and Dip. di Fisica Università di Firenze, Italy
9 Institute of Nuclear Physics, Polish Academy of Sciences, Krakow, Poland
Published online: 30 December 2017
We present a new method for the measurement of very small Γγ partial width that is important for the synthesis of elements in astrophysics. The method is based on the simultaneous detection of scattered beam, residual nucleus and decay γ rays. This method is optimized for the use of the CHIMERA detector at LNS. Experimental details are described.
© The Authors, published by EDP Sciences, 2017
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. (http://creativecommons.org/licenses/by/4.0/).
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