論文

査読有り
2010年4月

Observation of geo-neutrinos

PHYSICS LETTERS B
  • G. Bellini
  • J. Benziger
  • S. Bonetti
  • M. Buizza Avanzini
  • B. Caccianiga
  • L. Cadonati
  • F. Calaprice
  • C. Carraro
  • A. Chavarria
  • F. Dalnoki-Veress
  • D. D'Angelo
  • S. Davini
  • H. de Kerret
  • A. Dubin
  • A. Etenko
  • G. Fiorentini
  • K. Fomenko
  • D. Franco
  • C. Galbiati
  • S. Gazzana
  • C. Ghiano
  • M. Giammarchi
  • M. Goeger-Neff
  • A. Goretti
  • E. Guardincerri
  • S. Hardy
  • Aldo Ianni
  • Andrea Ianni
  • M. Joyce
  • V. V. Kobychev
  • Y. Koshio
  • G. Korga
  • D. Kryn
  • M. Laubenstein
  • M. Leung
  • T. Lewke
  • E. Litvinovich
  • B. Loer
  • P. Lombardi
  • L. Ludhova
  • I. Machulin
  • S. Manecki
  • W. Maneschg
  • G. Manuzio
  • Q. Meindl
  • E. Meroni
  • L. Miramonti
  • M. Misiaszek
  • D. Montanari
  • V. Muratova
  • L. Oberauer
  • M. Obolensky
  • F. Ortica
  • M. Pallavicini
  • L. Papp
  • L. Perasso
  • S. Perasso
  • A. Pocar
  • R. S. Raghavan
  • G. Ranucci
  • A. Razeto
  • A. Re
  • B. Ricci
  • P. Risso
  • A. Romani
  • D. Rountree
  • A. Sabelnikov
  • R. Saldanha
  • C. Salvo
  • S. Schoenert
  • H. Simgen
  • M. Skorokhvatov
  • O. Smirnov
  • A. Sotnikov
  • S. Sukhotin
  • Y. Suvorov
  • R. Tartaglia
  • G. Testera
  • D. Vignaud
  • R. B. Vogelaar
  • F. von Feilitzsch
  • J. Winter
  • M. Wojcik
  • A. Wright
  • M. Wurm
  • J. Xu
  • O. Zaimidoroga
  • S. Zavatarelli
  • G. Zuzel
  • 全て表示

687
4-5
開始ページ
299
終了ページ
304
記述言語
英語
掲載種別
研究論文(学術雑誌)
DOI
10.1016/j.physletb.2010.03.051
出版者・発行元
ELSEVIER SCIENCE BV

Geo-neutrinos, electron anti-neutrinos produced in beta decays of naturally occurring radioactive isotopes in the Earth, are a unique direct probe of our planet's interior. We report the first observation at more than 3 sigma C.L. of geo-neutrinos, performed with the Borexino detector at Laboratori Nazionali del Gran Sasso. Anti-neutrinos are detected through the neutron inverse beta decay reaction. With a 252.6 ton yr fiducial exposure after all selection cuts, we detected 9.9(-3.4)(+4.1)((+14.6)(-8.2))geo-neutrino events, wills errors corresponding to a 68.3% (99.73%) C.L. From the In C.. profile, the statistical significance of the Borexino geo-neutrino observation corresponds to a 99.997% C.L.
Our measurement of the geo-neutrinos rate is 3.9(-1.3)(+1.6)((+5.8)(-3.2)) events/(100 ton yr).
The observed prompt positron spectrum above 2.6 MeV is compatible with that expected from European nuclear reactors (mean base line of approximately 1000 km). Our measurement of reactor anti-neutrinos excludes the non-oscillation hypothesis at 99.60% C.L. This measurement rejects the hypothesis of an active geo-reactor in the Earth's core with a power above 3 TW at 95% C.L. (C) 2010 Elsevier B.V. All rights reserved.

リンク情報
DOI
https://doi.org/10.1016/j.physletb.2010.03.051
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000277247200005&DestApp=WOS_CPL
ID情報
  • DOI : 10.1016/j.physletb.2010.03.051
  • ISSN : 0370-2693
  • Web of Science ID : WOS:000277247200005

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