A new detection array called GASTLY (GAs-Silicon Two-Layer sYstem) has been designed to detect and identify low-energy light particles emitted in nuclear reactions of astrophysical interest. Devoted to the measurement of nanobarn cross-sections, the system is optimised for large solid angle coverage and for low-energy detection thresholds. The array consists of eight modules, each comprising an ionisation chamber and a large area silicon strip detector. Its modularity and versatility allow for use in a variety of experiments. Here we report on the performance of the array as obtained during its commissioning phase with standard α -particle sources and during in-beam tests with an intense 12C beam. Typical energy resolutions Δ(FWHM)/ of about 3% and 2% were obtained for the ionisation chambers and the silicon detectors, respectively. The status of the development of individual strip readout, based on ASIC technology, is also presented.

Development of a two-stage detection array for low-energy light charged particles in nuclear astrophysics applications / Romoli, M., Morales-Gallegos, L., Aliotta, M., Bruno, C.G., Buompane, R., D’Onofrio, A., Davinson, T., De Cesare, M., Di Leva, A., Di Meo, P., Duarte, J., Gasques, L., Gialanella, L., Imbriani, G., Porzio, G., Rapagnani, D., Vanzanella, A.. - In: THE EUROPEAN PHYSICAL JOURNAL. A, HADRONS AND NUCLEI. - ISSN 1434-6001. - 54:8(2018). [10.1140/epja/i2018-12575-5]

Development of a two-stage detection array for low-energy light charged particles in nuclear astrophysics applications

Di Leva, A.
Writing – Original Draft Preparation
;
Imbriani, G.
Writing – Original Draft Preparation
;
Rapagnani, D.
Writing – Original Draft Preparation
;
2018

Abstract

A new detection array called GASTLY (GAs-Silicon Two-Layer sYstem) has been designed to detect and identify low-energy light particles emitted in nuclear reactions of astrophysical interest. Devoted to the measurement of nanobarn cross-sections, the system is optimised for large solid angle coverage and for low-energy detection thresholds. The array consists of eight modules, each comprising an ionisation chamber and a large area silicon strip detector. Its modularity and versatility allow for use in a variety of experiments. Here we report on the performance of the array as obtained during its commissioning phase with standard α -particle sources and during in-beam tests with an intense 12C beam. Typical energy resolutions Δ(FWHM)/ of about 3% and 2% were obtained for the ionisation chambers and the silicon detectors, respectively. The status of the development of individual strip readout, based on ASIC technology, is also presented.
2018
Development of a two-stage detection array for low-energy light charged particles in nuclear astrophysics applications / Romoli, M., Morales-Gallegos, L., Aliotta, M., Bruno, C.G., Buompane, R., D’Onofrio, A., Davinson, T., De Cesare, M., Di Leva, A., Di Meo, P., Duarte, J., Gasques, L., Gialanella, L., Imbriani, G., Porzio, G., Rapagnani, D., Vanzanella, A.. - In: THE EUROPEAN PHYSICAL JOURNAL. A, HADRONS AND NUCLEI. - ISSN 1434-6001. - 54:8(2018). [10.1140/epja/i2018-12575-5]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11588/732610
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