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| Author(s): Show less - |
Elersich, A.
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Agnes, P.
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Ahmad, I
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Albergo, S.
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Albuquerque, I. F. M.
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Alexander, T.
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Alton, A. K.
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Amaudruz, P.
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Corona, M. Atzori
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Ave, M.
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Avetisov, I. Ch.
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Azzolini, O.
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Back, H. O.
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Balmforth, Z.
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Barrado-Olmedo, A.
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Barrillon, P.
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Basco, A.
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Batignani, G.
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Bocci, V.
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Bonivento, W. M.
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Bottino, B.
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Boulay, M. G.
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Busto, J.
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Cadeddu, M.
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Caminata, A.
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Canci, N.
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Capra, A.
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Caprioli, S.
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Caravati, M.
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Cargioli, N.
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Carlini, M.
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Castello, P.
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Cavalcante, P.
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Cavuoti, S.
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Cebrian, S.
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Ruiz, J. M. Cela
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Chashin, S.
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Chepurnov, A.
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Chyhyrynets, E.
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Cifarelli, L.
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Cintas, D.
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Citterio, M.
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Cleveland, B.
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Cocco, V
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Colaiuda, D.
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Vilda, E. Conde
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Consiglio, L.
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Copello, S.
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Covone, G.
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Czubak, M.
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D'Aniello, M.
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D'Auria, S.
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Rolo, M. D. Da Rocha
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Davini, S.
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De Cecco, S.
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De Gruttola, D.
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De Pasquale, S.
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De Rosa, G.
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Dellacasa, G.
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Derbin, A. V.
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Devoto, A.
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Di Capua, F.
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Di Noto, L.
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Di Stefano, P.
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Dolganov, G.
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Dordei, F.
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Ellingwood, E.
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Erjavec, T.
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Diaz, M. Fernandez
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Fiorillo, G.
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Franchini, P.
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Franco, D.
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Funicello, N.
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Gabriele, F.
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Gahan, D.
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Galbiati, C.
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Gallina, G.
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Gallus, G.
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Garbini, M.
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Abia, P. Garcia
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Gendotti, A.
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Ghiano, C.
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Giganti, C.
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Giovanetti, G. K.
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Casanueva, V. Goicoechea
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Gola, A.
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Grauso, G.
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di Cortona, G. Grilli
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Grobov, A.
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Gromov, M.
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Guan, M.
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Guerzoni, M.
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Gulino, M.
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Guo, C.
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Hackett, B. R.
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Hallin, A. L.
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Hamer, A.
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Haranczyk, M.
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Hessel, T.
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Hill, S.
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Horikawa, S.
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Hubaut, F.
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Hucker, J.
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Hugues, T.
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Ianni, An
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Ippolito, V.
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Jillings, C.
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Jois, S.
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Kachru, P.
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Kemp, A. A.
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Kendziora, C. L.
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Kimura, M.
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Kochanek, I
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Kondo, K.
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Korga, G.
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Koulosousas, S.
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Kubankin, A.
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Kuss, M.
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Kuzniak, M.
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La Commara, M.
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Lai, M.
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Le Guirriec, E.
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Leason, E.
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Leoni, A.
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Lidey, L.
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Lissia, M.
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Luzzi, L.
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Lychagina, O.
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Macfadyen, O.
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Machulin, I. N.
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Manecki, S.
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Manthos, I
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Mapelli, L.
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Margotti, A.
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Mari, S. M.
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Mariani, C.
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Maricic, J.
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Marini, A.
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Martinez, M.
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Martoff, C. J.
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Matteucci, G.
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Mavrokoridis, K.
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McDonald, A. B.
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Messina, A.
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Milincic, R.
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Mitra, A.
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Moharana, A.
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Monroe, J.
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Moretti, E.
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Morrocchi, M.
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Mroz, T.
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Muratova, V. N.
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Muscas, C.
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Musico, P.
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Nania, R.
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Nessi, M.
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Nieradka, G.
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Nikolopoulos, K.
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Nowak, J.
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Olchansky, K.
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Oleinik, A.
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Oleynikov, V.
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Organtini, P.
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de Solorzano, A. Ortiz
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Pagani, L.
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Pallavicini, M.
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Pandola, L.
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Pantic, E.
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Paoloni, E.
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Paternoster, G.
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Pegoraro, P. A.
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Pelczar, K.
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Pellegrino, C.
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Pesudo, V
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Piacentini, S.
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Pietrofaccia, L.
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Pino, N.
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Pocar, A.
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Poehlmann, D. M.
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Pordes, S.
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Pralavorio, P.
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Price, D.
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Ragusa, F.
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Ramachers, Y.
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Razeti, M.
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Renshaw, A. L.
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Rescigno, M.
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Retiere, F.
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Rignanese, L. P.
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Ripoli, C.
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Rivetti, A.
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Roberts, A.
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Roberts, C.
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Rode, J.
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Rogers, G.
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Romero, L.
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Rossi, M.
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Rubbia, A.
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Sabia, M. A.
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Salomone, P.
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Sandford, E.
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Sanfilippo, S.
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Santone, D.
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Santorelli, R.
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Savarese, C.
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Scapparone, E.
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Schillaci, G.
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Schuckman, F. G., II
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Scioli, G.
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Simeone, M.
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Skensved, P.
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Skorokhvatov, M. D.
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Smirnov, O.
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Smirnova, T.
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Smith, B.
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Spadoni, F.
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Spangenberg, M.
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Stefanizzi, R.
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Steri, A.
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Stornelli, V.
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Stracka, S.
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Stringer, M.
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Sulis, S.
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Sung, A.
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Suvorov, Y.
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Szelc, A. M.
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Tartaglia, R.
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Taylor, A.
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Taylor, J.
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Tedesco, S.
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Testera, G.
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Thieme, K.
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Thorpe, T. N.
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Tonazzo, A.
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Tricomi, A.
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Unzhakov, E. V.
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John, T. Vallivilayil
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Van Uffelen, M.
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Viant, T.
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Viel, S.
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Vogelaar, R. B.
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Vossebeld, J.
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Wada, M.
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Walczak, M. B.
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Wang, H.
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Wang, Y.
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Westerdale, S.
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Williams, L.
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Wingerter-Seez, I
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Wojaczynski, R.
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Wojcik, Ma. M.
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Wright, T.
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Xie, Y.
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Yang, C.
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Zabihi, A.
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Zakhary, P.
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Zani, A.
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Zichichi, A.
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Zuzel, G.
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Zykova, M. P.
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DarkSide-20k Collaborat
Total Authors: 261
|
| Document type: | Journal article |
| Source: | Astroparticle Physics; v. 152, p. 12-pg., 2023-10-01. |
| Abstract | |
The activation of materials due to exposure to cosmic rays may become an important background source for experiments investigating rare event phenomena. DarkSide-20k, currently under construction at the Laboratori Nazionali del Gran Sasso, is a direct detection experiment for galactic dark matter particles, using a two-phase liquid-argon Time Projection Chamber (TPC) filled with 49.7 tonnes (active mass) of Underground Argon (UAr) depleted in 39Ar. Despite the outstanding capability of discriminating ������/������ background in argon TPCs, this background must be considered because of induced dead time or accidental coincidences mimicking dark-matter signals and it is relevant for low-threshold electron-counting measurements. Here, the cosmogenic activity of relevant long-lived radioisotopes induced in the experiment has been estimated to set requirements and procedures during preparation of the experiment and to check that it is not dominant over primordial radioactivity; particular attention has been paid to the activation of the 120 t of UAr used in DarkSide-20k. Expected exposures above ground and production rates, either measured or calculated, have been considered in detail. From the simulated counting rates in the detector due to cosmogenic isotopes, it is concluded that activation in copper and stainless steel is not problematic. The activity of 39Ar induced during extraction, purification and transport on surface is evaluated to be 2.8% of the activity measured in UAr by DarkSide-50 experiment, which used the same underground source, and thus considered acceptable. Other isotopes in the UAr such as 37Ar and 3H are shown not to be relevant due to short half-life and assumed purification methods. (AU) | |
| FAPESP's process: | 17/26238-4 - Direct dark matter detection within the Darkside program |
| Grantee: | Maximo David Ave Pernas |
| Support Opportunities: | Research Grants - Young Investigators Grants |