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Article: Ultra-low background measurements in a large volume underground detector: Borexino Collaboration
Title | Ultra-low background measurements in a large volume underground detector: Borexino Collaboration |
---|---|
Authors | Alimonti, GAnghloher, GArpesella, CBalata, MBellini, GBenziger, JBonetti, SCadonati, LCalaprice, FPCecchet, GChen, MDarnton, NDe Bari, ADeutsch, MElisei, FVon Feilitzsch, FGalbiati, CGatti, FGiammarchi, MGGiugni, DGoldbrunner, TGolubchikov, AGoretti, AHagner, THartmann, FXVon Hentig, RHeusser, GIanni, AJochum, JJohnson, MLaubenstein, MLombardi, PMagni, SMalvezzi, SManno, IManuzio, GMasetti, FMazzucato, UMeroni, ENeff, MNostro, AOberauer, LPerotti, APreda, ARaghavan, RSRanucci, GResconi, ERuscitti, MScardaoni, RSchönert, SSmirnov, OTartaglia, RTestera, GUllucci, PVogelaar, RBVitale, SWojcik, MZaimidoroga, O |
Keywords | Low Background Experiments Low Radioactivity Solar Neutrino |
Issue Date | 1998 |
Publisher | Elsevier BV. The Journal's web site is located at http://www.elsevier.com/locate/astropartphys |
Citation | Astroparticle Physics, 1998, v. 8 n. 3, p. 141-157 How to Cite? |
Abstract | A large volume (4.8 m3) liquid scintillator detector has been running in Hall C of the Gran Sasso Underground Laboratory since February 1995. This detector is called the "Counting Test Facility" (CTF). The main goal of the detector facility is the measurement of ultralow background levels in scintillators and the development of processes able to purify them at this level. The detector has been designed to have exceptional sensitivity using a variety of methods to identify backgrounds. With the CTF, records were achieved in the domain of low background large volume detectors. Limits of 3.5 ± 1.3 × 10-16 g/g and 4.4+1.5 -1.2 × 10-16 g/g for the 238U and 232Th daughters, respectively, and 1.85 ± 0.13 ± 0.01 × 10-18 for the isotopic abundance of 14C relative to 12C were obtained. These results are very encouraging and point towards the feasibility of low energy, real time scintillation detectors for solar neutrinos, such as Borexino. © 1998 Elsevier Science B.V. |
Persistent Identifier | http://hdl.handle.net/10722/91391 |
ISSN | 2023 Impact Factor: 4.2 2023 SCImago Journal Rankings: 1.151 |
ISI Accession Number ID | |
References |
DC Field | Value | Language |
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dc.contributor.author | Alimonti, G | en_HK |
dc.contributor.author | Anghloher, G | en_HK |
dc.contributor.author | Arpesella, C | en_HK |
dc.contributor.author | Balata, M | en_HK |
dc.contributor.author | Bellini, G | en_HK |
dc.contributor.author | Benziger, J | en_HK |
dc.contributor.author | Bonetti, S | en_HK |
dc.contributor.author | Cadonati, L | en_HK |
dc.contributor.author | Calaprice, FP | en_HK |
dc.contributor.author | Cecchet, G | en_HK |
dc.contributor.author | Chen, M | en_HK |
dc.contributor.author | Darnton, N | en_HK |
dc.contributor.author | De Bari, A | en_HK |
dc.contributor.author | Deutsch, M | en_HK |
dc.contributor.author | Elisei, F | en_HK |
dc.contributor.author | Von Feilitzsch, F | en_HK |
dc.contributor.author | Galbiati, C | en_HK |
dc.contributor.author | Gatti, F | en_HK |
dc.contributor.author | Giammarchi, MG | en_HK |
dc.contributor.author | Giugni, D | en_HK |
dc.contributor.author | Goldbrunner, T | en_HK |
dc.contributor.author | Golubchikov, A | en_HK |
dc.contributor.author | Goretti, A | en_HK |
dc.contributor.author | Hagner, T | en_HK |
dc.contributor.author | Hartmann, FX | en_HK |
dc.contributor.author | Von Hentig, R | en_HK |
dc.contributor.author | Heusser, G | en_HK |
dc.contributor.author | Ianni, A | en_HK |
dc.contributor.author | Jochum, J | en_HK |
dc.contributor.author | Johnson, M | en_HK |
dc.contributor.author | Laubenstein, M | en_HK |
dc.contributor.author | Lombardi, P | en_HK |
dc.contributor.author | Magni, S | en_HK |
dc.contributor.author | Malvezzi, S | en_HK |
dc.contributor.author | Manno, I | en_HK |
dc.contributor.author | Manuzio, G | en_HK |
dc.contributor.author | Masetti, F | en_HK |
dc.contributor.author | Mazzucato, U | en_HK |
dc.contributor.author | Meroni, E | en_HK |
dc.contributor.author | Neff, M | en_HK |
dc.contributor.author | Nostro, A | en_HK |
dc.contributor.author | Oberauer, L | en_HK |
dc.contributor.author | Perotti, A | en_HK |
dc.contributor.author | Preda, A | en_HK |
dc.contributor.author | Raghavan, RS | en_HK |
dc.contributor.author | Ranucci, G | en_HK |
dc.contributor.author | Resconi, E | en_HK |
dc.contributor.author | Ruscitti, M | en_HK |
dc.contributor.author | Scardaoni, R | en_HK |
dc.contributor.author | Schönert, S | en_HK |
dc.contributor.author | Smirnov, O | en_HK |
dc.contributor.author | Tartaglia, R | en_HK |
dc.contributor.author | Testera, G | en_HK |
dc.contributor.author | Ullucci, P | en_HK |
dc.contributor.author | Vogelaar, RB | en_HK |
dc.contributor.author | Vitale, S | en_HK |
dc.contributor.author | Wojcik, M | en_HK |
dc.contributor.author | Zaimidoroga, O | en_HK |
dc.date.accessioned | 2010-09-17T10:18:32Z | - |
dc.date.available | 2010-09-17T10:18:32Z | - |
dc.date.issued | 1998 | en_HK |
dc.identifier.citation | Astroparticle Physics, 1998, v. 8 n. 3, p. 141-157 | en_HK |
dc.identifier.issn | 0927-6505 | en_HK |
dc.identifier.uri | http://hdl.handle.net/10722/91391 | - |
dc.description.abstract | A large volume (4.8 m3) liquid scintillator detector has been running in Hall C of the Gran Sasso Underground Laboratory since February 1995. This detector is called the "Counting Test Facility" (CTF). The main goal of the detector facility is the measurement of ultralow background levels in scintillators and the development of processes able to purify them at this level. The detector has been designed to have exceptional sensitivity using a variety of methods to identify backgrounds. With the CTF, records were achieved in the domain of low background large volume detectors. Limits of 3.5 ± 1.3 × 10-16 g/g and 4.4+1.5 -1.2 × 10-16 g/g for the 238U and 232Th daughters, respectively, and 1.85 ± 0.13 ± 0.01 × 10-18 for the isotopic abundance of 14C relative to 12C were obtained. These results are very encouraging and point towards the feasibility of low energy, real time scintillation detectors for solar neutrinos, such as Borexino. © 1998 Elsevier Science B.V. | en_HK |
dc.language | eng | en_HK |
dc.publisher | Elsevier BV. The Journal's web site is located at http://www.elsevier.com/locate/astropartphys | en_HK |
dc.relation.ispartof | Astroparticle Physics | en_HK |
dc.subject | Low Background Experiments | en_HK |
dc.subject | Low Radioactivity | en_HK |
dc.subject | Solar Neutrino | en_HK |
dc.title | Ultra-low background measurements in a large volume underground detector: Borexino Collaboration | en_HK |
dc.type | Article | en_HK |
dc.identifier.email | Chen, MZ:mzqchen@hku.hk | en_HK |
dc.identifier.authority | Chen, MZ=rp1317 | en_HK |
dc.description.nature | link_to_subscribed_fulltext | - |
dc.identifier.scopus | eid_2-s2.0-0031991777 | en_HK |
dc.relation.references | http://www.scopus.com/mlt/select.url?eid=2-s2.0-0031991777&selection=ref&src=s&origin=recordpage | en_HK |
dc.identifier.volume | 8 | en_HK |
dc.identifier.issue | 3 | en_HK |
dc.identifier.spage | 141 | en_HK |
dc.identifier.epage | 157 | en_HK |
dc.identifier.isi | WOS:000072088700003 | - |
dc.identifier.issnl | 0927-6505 | - |