論文

査読有り
2011年1月

Study of solar and other unknown anti-neutrino fluxes with Borexino at LNGS

PHYSICS LETTERS B
  • G. Bellini
  • J. Benziger
  • S. Bonetti
  • M. Buizza Avanzini
  • B. Caccianiga
  • L. Cadonati
  • F. Calaprice
  • C. Carraro
  • A. Chavarria
  • A. Chepurnov
  • D. D'Angelo
  • S. Davini
  • A. Derbin
  • A. Etenko
  • 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
  • D. Korablev
  • Y. Koshio
  • G. Korga
  • D. Kryn
  • M. Laubenstein
  • 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
  • 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 Feilitzschk
  • J. Winter
  • M. Wojcik
  • A. Wright
  • M. Wurm
  • J. Xu
  • O. Zaimidoroga
  • S. Zavatarelli
  • G. Zuzel
  • 全て表示

696
3
開始ページ
191
終了ページ
196
記述言語
英語
掲載種別
研究論文(学術雑誌)
DOI
10.1016/j.physletb.2010.12.030
出版者・発行元
ELSEVIER SCIENCE BV

We report on the search for anti-neutrinos of yet unknown origin with the Borexino detector at the Laboratori Nazionali del Gran Sasso. In particular, a hypothetical anti-neutrino flux from the Sun is investigated. Anti-neutrinos are detected through the neutron inverse beta decay reaction in a large liquid organic scintillator target. We set a new upper limit for a hypothetical solar (v) over bare flux of 760 cm(-2) s(-1), obtained assuming an undistorted solar (8)B energy spectrum. This corresponds to a limit on the transition probability of solar neutrinos to anti-neutrinos of 1.3 x 10(-4) (90% C.L.) for E ((v) over bar) > 1.8 MeV, covering the entire (8)B spectrum. Best differential limits on anti-neutrino fluxes from unknown sources are also obtained between the detection energy threshold of 1.8 MeV and 17.8 MeV with more than 2 years of data. (C) 2010 Elsevier B.V. All rights reserved.

リンク情報
DOI
https://doi.org/10.1016/j.physletb.2010.12.030
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000287176500003&DestApp=WOS_CPL
ID情報
  • DOI : 10.1016/j.physletb.2010.12.030
  • ISSN : 0370-2693
  • Web of Science ID : WOS:000287176500003

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