EPJ Web Conf.
Volume 184, 20189th European Summer School on Experimental Nuclear Astrophysics
|Number of page(s)||3|
|Published online||29 June 2018|
Development of the ELISSA array: prototype testing at Laboratori Nazionali del Sud
2 INFN, Laboratori Nazionali del Sud, Catania, Italy
3 Facoltá di Ingegneria e Architettura, Universitá Kore, Enna, Italy
4 Dipartimento di Fisica e Astronomia, Universitá degli Studi, Catania, Italy
* e-mail: firstname.lastname@example.org
Published online: 29 June 2018
The Extreme Light Infrastructure-Nuclear Physics (ELI-NP) facility, underconstruction in Magurele near Bucharest in Romania, will provide high-intensity andhigh-resolution gamma ray beams that can be used to address hotly debated problems in nuclear astrophysics, such as the accurate measurements of the cross sections of the24Mg(γ,α)20Ne reaction
For this purpose, a silicon strip detector array (named ELISSA) will be realized in acommon effort by ELI-NP and Laboratori Nazionali del Sud (INFN-LNS), in order to measure excitation functions and angular distributions over a wide energy and angular range. A prototype of ELISSA was built and tested at INFN-LNS in Catania (Italy) with the support of ELI-NP. In this occasion, we have carried out experiments with alpha sources and with a 11 MeV 7Li beam that show up a very good energy resolution (better than 1%) and very good position resolution, of the order of 1 mm. Moreover, a threshold of 150 keV can be easily achieved with no cooling.
© The Authors, published by EDP Sciences, 2018
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