| Issue |
EPJ Web Conf.
Volume 165, 2017
Nuclear Physics in Astrophysics VIII (NPA8 2017)
|
|
|---|---|---|
| Article Number | 01011 | |
| Number of page(s) | 4 | |
| DOI | https://doi.org/10.1051/epjconf/201716501011 | |
| Published online | 30 December 2017 | |
https://doi.org/10.1051/epjconf/201716501011
Characterization of X3 Silicon Detectors for the ELISSA Array at ELI-NP
1 ELI-NP/IFIN-HH, 30 Reactorului Street, 077125, Magurele, Romania
2 INFN, Laboratori Nazionali del Sud, Via Santa Sofia 62, 95123 Catania, Italy
* e-mail: svetlana.chesnevskaya@eli-np.ro
Published online: 30 December 2017
Position-sensitive silicon strip detectors represent one of the best solutions for the detection of charged particles as they provide good energy and position resolution over a large range of energies. A silicon array coupled with the gamma beams at the ELI-NP facility would allow measuring photodissociation reactions of interest for Big Bang Nucleosynthesis and on heavy nuclei intervening in the p-process. Forty X3 detectors for our ELISSA (ELI-NP Silicon Strip Detectors Array) project have been recently purchased and tested. We investigated several specifications, such as leakage currents, depletion voltage, and detector stability under vacuum. The energy and position resolution, and ballistic deficit were measured and analyzed. This paper presents the main results of our extensive testing. The measured energy resolution for the X3 detectors is better than results published for similar arrays (ANASEN or ORRUBA).
© 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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