Characterization of a kg-scale archaeological lead-based PbWO

Cryogenic detectors Low-background Neutrino physics Supernovae

Journal

Applied radiation and isotopes : including data, instrumentation and methods for use in agriculture, industry and medicine
ISSN: 1872-9800
Titre abrégé: Appl Radiat Isot
Pays: England
ID NLM: 9306253

Informations de publication

Date de publication:
Apr 2023
Historique:
received: 29 05 2022
revised: 21 01 2023
accepted: 26 01 2023
pubmed: 3 2 2023
medline: 3 2 2023
entrez: 2 2 2023
Statut: ppublish

Résumé

Core-collapse Supernovae (SNe) are one of the most energetic events in the Universe, during which almost all the star's binding energy is released in the form of neutrinos. These particles are direct probes of the processes occurring in the stellar core and provide unique insights into the gravitational collapse. RES-NOVA will revolutionize how we detect neutrinos from astrophysical sources, by deploying the first ton-scale array of cryogenic detectors made from archaeological lead. Pb offers the highest neutrino interaction cross-section via coherent elastic neutrino-nucleus scattering (CEνNS). Such process will enable RES-NOVA to be equally sensitive to all neutrino flavours. For the first time, we propose the use archaeological Pb as sensitive target material in order to achieve an ultra-low background level in the region of interest (O(1 keV)). All these features make possible the deployment of the first cm-scale neutrino telescope for the investigation of astrophysical sources. In this contribution, we will characterize the radiopurity level and the performance of a small-scale proof-of-principle detector of RES-NOVA, consisting in a PbWO

Identifiants

DOI: 10.1016/j.apradiso.2023.110704 PMID: 36731392
pubmed: 36731392
pii: S0969-8043(23)00057-X
doi: 10.1016/j.apradiso.2023.110704
pii:
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

110704

Informations de copyright

Copyright © 2023 Elsevier Ltd. All rights reserved.

Déclaration de conflit d'intérêts

Declaration of Competing Interest The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.

Auteurs

J W Beeman (JW)

Lawrence Berkeley National Laboratory, Berkeley, 94720, CA, USA.

G Benato (G)

Laboratori Nazionali del Gran Sasso, Via G. Acitelli 22, Assergi, 67100, IT, Italy.

C Bucci (C)

Laboratori Nazionali del Gran Sasso, Via G. Acitelli 22, Assergi, 67100, IT, Italy.

L Canonica (L)

Max-Planck-Institut für Physik, Föhringer Ring 6, München, DE-80805, Germany.

P Carniti (P)

Dipartimento di Fisica, Università di Milano - Bicocca, Piazza della Scienza 3, Milano, I-20126, IT, Italy; INFN Sezione di Milano - Bicocca, Piazza della Scienza 3, Milano, I-20126, IT, Italy.

E Celi (E)

Laboratori Nazionali del Gran Sasso, Via G. Acitelli 22, Assergi, 67100, IT, Italy; Gran Sasso Science Institute, Viale F. Crespi 7, L'Aquila, 67100, IT, Italy.

M Clemenza (M)

INFN Sezione di Milano - Bicocca, Piazza della Scienza 3, Milano, I-20126, IT, Italy.

A D'Addabbo (A)

Laboratori Nazionali del Gran Sasso, Via G. Acitelli 22, Assergi, 67100, IT, Italy.

F A Danevich (FA)

Institute for Nuclear Research of NASU, Kyiv, 03028, Ukraine.

S Di Domizio (S)

INFN Sezione di Genova and Università di Genova, Via Dodecaneso 33, Genova, I-16146, IT, Italy.

S Di Lorenzo (S)

Laboratori Nazionali del Gran Sasso, Via G. Acitelli 22, Assergi, 67100, IT, Italy.

O M Dubovik (OM)

Institute of Scintillation Materials of NASU, Kharkiv, 61072, Ukraine.

N Ferreiro Iachellini (N)

Max-Planck-Institut für Physik, Föhringer Ring 6, München, DE-80805, Germany.

F Ferroni (F)

Gran Sasso Science Institute, Viale F. Crespi 7, L'Aquila, 67100, IT, Italy; INFN Sezione di Roma-1, P.le Aldo Moro 2, Roma, I-00185, IT, Italy.

E Fiorini (E)

Dipartimento di Fisica, Università di Milano - Bicocca, Piazza della Scienza 3, Milano, I-20126, IT, Italy; INFN Sezione di Milano - Bicocca, Piazza della Scienza 3, Milano, I-20126, IT, Italy.

S Fu (S)

Laboratori Nazionali del Gran Sasso, Via G. Acitelli 22, Assergi, 67100, IT, Italy.

A Garai (A)

Max-Planck-Institut für Physik, Föhringer Ring 6, München, DE-80805, Germany.

S Ghislandi (S)

Laboratori Nazionali del Gran Sasso, Via G. Acitelli 22, Assergi, 67100, IT, Italy; Gran Sasso Science Institute, Viale F. Crespi 7, L'Aquila, 67100, IT, Italy.

L Gironi (L)

Dipartimento di Fisica, Università di Milano - Bicocca, Piazza della Scienza 3, Milano, I-20126, IT, Italy; INFN Sezione di Milano - Bicocca, Piazza della Scienza 3, Milano, I-20126, IT, Italy.

P Gorla (P)

Laboratori Nazionali del Gran Sasso, Via G. Acitelli 22, Assergi, 67100, IT, Italy.

C Gotti (C)

Dipartimento di Fisica, Università di Milano - Bicocca, Piazza della Scienza 3, Milano, I-20126, IT, Italy; INFN Sezione di Milano - Bicocca, Piazza della Scienza 3, Milano, I-20126, IT, Italy.

P V Guillaumon (PV)

Laboratori Nazionali del Gran Sasso, Via G. Acitelli 22, Assergi, 67100, IT, Italy.

D L Helis (DL)

Laboratori Nazionali del Gran Sasso, Via G. Acitelli 22, Assergi, 67100, IT, Italy; Gran Sasso Science Institute, Viale F. Crespi 7, L'Aquila, 67100, IT, Italy.

G P Kovtun (GP)

National Science Center 'Kharkiv Institute of Physics and Technology', Kharkiv, 61108, Ukraine.

M Mancuso (M)

Max-Planck-Institut für Physik, Föhringer Ring 6, München, DE-80805, Germany.

L Marini (L)

Laboratori Nazionali del Gran Sasso, Via G. Acitelli 22, Assergi, 67100, IT, Italy; Gran Sasso Science Institute, Viale F. Crespi 7, L'Aquila, 67100, IT, Italy.

M Olmi (M)

Laboratori Nazionali del Gran Sasso, Via G. Acitelli 22, Assergi, 67100, IT, Italy.

L Pagnanini (L)

Laboratori Nazionali del Gran Sasso, Via G. Acitelli 22, Assergi, 67100, IT, Italy; Gran Sasso Science Institute, Viale F. Crespi 7, L'Aquila, 67100, IT, Italy.

L Pattavina (L)

Laboratori Nazionali del Gran Sasso, Via G. Acitelli 22, Assergi, 67100, IT, Italy; Technical University of Munich, JamesFranckStrasse 1, Garching, 85748, DE, Germany. Electronic address: luca.pattavina@lngs.infn.it.

G Pessina (G)

INFN Sezione di Milano - Bicocca, Piazza della Scienza 3, Milano, I-20126, IT, Italy.

F Petricca (F)

Max-Planck-Institut für Physik, Föhringer Ring 6, München, DE-80805, Germany.

S Pirro (S)

Laboratori Nazionali del Gran Sasso, Via G. Acitelli 22, Assergi, 67100, IT, Italy.

S Pozzi (S)

Dipartimento di Fisica, Università di Milano - Bicocca, Piazza della Scienza 3, Milano, I-20126, IT, Italy; INFN Sezione di Milano - Bicocca, Piazza della Scienza 3, Milano, I-20126, IT, Italy.

A Puiu (A)

Laboratori Nazionali del Gran Sasso, Via G. Acitelli 22, Assergi, 67100, IT, Italy; Gran Sasso Science Institute, Viale F. Crespi 7, L'Aquila, 67100, IT, Italy.

S Quitadamo (S)

Laboratori Nazionali del Gran Sasso, Via G. Acitelli 22, Assergi, 67100, IT, Italy; Gran Sasso Science Institute, Viale F. Crespi 7, L'Aquila, 67100, IT, Italy. Electronic address: simone.quitadamo@gssi.it.

J Rothe (J)

Technical University of Munich, JamesFranckStrasse 1, Garching, 85748, DE, Germany.

A P Scherban (AP)

National Science Center 'Kharkiv Institute of Physics and Technology', Kharkiv, 61108, Ukraine.

S Schönert (S)

Technical University of Munich, JamesFranckStrasse 1, Garching, 85748, DE, Germany.

D A Solopikhin (DA)

National Science Center 'Kharkiv Institute of Physics and Technology', Kharkiv, 61108, Ukraine.

R Strauss (R)

Technical University of Munich, JamesFranckStrasse 1, Garching, 85748, DE, Germany.

E Tarabini (E)

INFN Sezione di Milano - Bicocca, Piazza della Scienza 3, Milano, I-20126, IT, Italy.

V I Tretyak (VI)

Institute for Nuclear Research of NASU, Kyiv, 03028, Ukraine.

I A Tupitsyna (IA)

Institute of Scintillation Materials of NASU, Kharkiv, 61072, Ukraine.

V Wagner (V)

Technical University of Munich, JamesFranckStrasse 1, Garching, 85748, DE, Germany.

Classifications MeSH