Campaign of measurements to probe the good performance of the new array FARCOS for spectroscopy and correlations.

39th Symposium on Nuclear Physics 2016

Acosta, L.^1,2 ; Andolina, R.^3 ; Auditore, L.^4 ; Boiano, C.^5 ; Cardella, G.^2 ; Castoldi, A.^5,6 ; D'Andrea, M.^2 ; De Filippo, E.^2 ; De Luca, S.^4 ; Dell'Aquila, D.^7 ; Francalanza, L.^7 ; Gnoffo, B.^2 ; Guazzoni, C.^5,6 ; Lanzalone, G.^8,9 ; Lombardo, I.^7 ; Martorana, N.^3,9 ; Minniti, T.^4 ; Norella, S.^4 ; Pagano, A.^2 ; Pagano, E.V.^3,9 ; Papa, M.^2 ; Parsani, T.^5,6 ; Pirrone, S.^2 ; Politi, G.^2,3 ; Porto, F.^3,9 ; Quattrocchi, L.^4 ; Rizzo, F.^3,9 ; Russotto, P.^2 ; Saccá, G.^2 ; Trifirò, A.^4 ; Trimarchi, M.^4 ; Verde, G.^2,10 ; Vigilante, M.^7 ; Zambon, P.^5,6,11

Instituto de Física, Universidad Nacional Autónoma de México, Cd.Mx., Mexico^1

INFN-Sezione di Catania, Catania, Italy^2

Dip. di Fisica e Astronomia, Università di Catania, Catania, Italy^3

Dip. di Scienze Matematiche e Informatiche, Scienze Fisiche e Scienze della Terra, Università di Messina, INFN Gruppo Collegato di Messina, Messina, Italy^4

INFN Sezione di Milano, Milan, Italy^5

Politecnico di Milano, Dip. di Elettronica, Informazione e Bioingegneria, Milan, Italy^6

INFN-Sezione di Napoli and Dip. di Fisica, Università di Napoli Federico II, Napoli, Italy^7

Università Kore Enna, Enna, Italy^8

INFN Laboratori Nazionali Del Sud, Catania, Italy

(10) Institute de Physique Nucléaire d'Orsay, Orsay, France

(11) Dectris Ltd, Baden, Switzerland^9

关键词: Present situation;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/730/1/012001/pdf
DOI  :  10.1088/1742-6596/730/1/012001

来源: IOP

【 摘 要 】

During the last four years, several measurements have been carried out where the capabilities of FARCOS array were tested. In some of this occasions, FARCOS was coupled to the 4π array CHIMERA, permanently placed at INFN-Laboratori Nazionali del Sud, Catania in order to be tested in real experimental measurements. At the present situation, the FARCOS demonstrator is formed by 4 telescopes out of the originally 20 that will constitute the final array. Here are presented some preliminary results obtained with the new array, probing its qualities and showing the effectiveness of FARCOS telescopes. The initial encouraging results support the construction of the complete array.