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Journal Articles Astroparticle Physics Year : 2012

The next-generation liquid-scintillator neutrino observatory LENA

Michael Wurm
  • Function : Author
John F. Beacom
  • Function : Author
Leonid B. Bezrukov
  • Function : Author
Daniel Bick
  • Function : Author
Johannes Blümer
  • Function : Author
Sandhya Choubey
  • Function : Author
Christian Ciemniak
  • Function : Author
Davide d'Angelo
  • Function : Author
Basudeb Dasgupta
  • Function : Author
Alexander Derbin
  • Function : Author
Amol Dighe
  • Function : Author
Grigorij Domogatsky
  • Function : Author
Steve Dye
  • Function : Author
Sergey Eliseev
  • Function : Author
Timo Enqvist
  • Function : Author
Alexey Erykalov
  • Function : Author
Franz von Feilitzsch
  • Function : Author
Gianni Fiorentini
  • Function : Author
Tobias Fischer
  • Function : Author
Marianne Göger-Neff
  • Function : Author
Peter Grabmayr
  • Function : Author
Caren Hagner
  • Function : Author
Dominikus Hellgartner
  • Function : Author
Johannes Hissa
  • Function : Author
Shunsaku Horiuchi
  • Function : Author
Hans-Thomas Janka
  • Function : Author
Claude Jaupart
  • Function : Author
Josef Jochum
  • Function : Author
Tuomo Kalliokoski
  • Function : Author
Alexei Kayunov
  • Function : Author
Pasi Kuusiniemi
  • Function : Author
Tobias Lachenmaier
  • Function : Author
Ionel Lazanu
  • Function : Author
John G. Learned
  • Function : Author
Timo Lewke
  • Function : Author
Paolo Lombardi
  • Function : Author
Sebastian Lorenz
  • Function : Author
Bayarto Lubsandorzhiev
  • Function : Author
Livia Ludhova
  • Function : Author
Kai Loo
  • Function : Author
Jukka Maalampi
  • Function : Author
Fabio Mantovani
  • Function : Author
Michela Marafini
  • Function : Author
Jelena Maricic
  • Function : Author
Teresa Marrodán Undagoitia
  • Function : Author
William F. Mcdonough
  • Function : Author
Lino Miramonti
  • Function : Author
Alessandro Mirizzi
  • Function : Author
Quirin Meindl
  • Function : Author
Olga Mena
  • Function : Author
Randolph Möllenberg
  • Function : Author
Valentina Muratova
  • Function : Author
Rolf Nahnhauer
  • Function : Author
Dmitry Nesterenko
  • Function : Author
Yuri N. Novikov
  • Function : Author
Guido Nuijten
  • Function : Author
Lothar Oberauer
  • Function : Author
Sandip Pakvasa
  • Function : Author
Sergio Palomares-Ruiz
  • Function : Author
Marco Pallavicini
  • Function : Author
Silvia Pascoli
  • Function : Author
T. Patzak
  • Function : Author
Juha Peltoniemi
  • Function : Author
Walter Potzel
  • Function : Author
Tomi Räihä
  • Function : Author
Georg G. Raffelt
  • Function : Author
Gioacchino Ranucci
  • Function : Author
Soebur Razzaque
  • Function : Author
Kari Rummukainen
  • Function : Author
Juho Sarkamo
  • Function : Author
Valerij Sinev
  • Function : Author
Christian Spiering
  • Function : Author
Achim Stahl
  • Function : Author
Felicitas Thorne
  • Function : Author
Marc Tippmann
  • Function : Author
A. Tonazzo
  • Function : Author
Wladyslaw H. Trzaska
  • Function : Author
John D. Vergados
  • Function : Author
Christopher Wiebusch
  • Function : Author
Jürgen Winter
  • Function : Author

Abstract

As part of the European LAGUNA design study on a next-generation neutrino detector, we propose the liquid-scintillator detector LENA (Low Energy Neutrino Astronomy) as a multipurpose neutrino observatory. The outstanding successes of the Borexino and KamLAND experiments demonstrate the large potential of liquid-scintillator detectors in low-energy neutrino physics. Low energy threshold, good energy resolution and efficient background discrimination are inherent to the liquid-scintillator technique. A target mass of 50 kt will offer a substantial increase in detection sensitivity.At low energies, the variety of detection channels available in liquid scintillator will allow for an energy - and flavor-resolved analysis of the neutrino burst emitted by a galactic Supernova. Due to target mass and background conditions, LENA will also be sensitive to the faint signal of the Diffuse Supernova Neutrino Background. Solar metallicity, time-variation in the solar neutrino flux and deviations from MSW-LMA survival probabilities can be investigated based on unprecedented statistics. Low background conditions allow to search for dark matter by observing rare annihilation neutrinos. The large number of events expected for geoneutrinos will give valuable information on the abundances of Uranium and Thorium and their relative ratio in the Earth's crust and mantle. Reactor neutrinos enable a high-precision measurement of solar mixing parameters. A strong radioactive or pion decay-at-rest neutrino source can be placed close to the detector to investigate neutrino oscillations for short distances and sub-MeV to MeV energies.At high energies, LENA will provide a new lifetime limit for the SUSY-favored proton decay mode into kaon and antineutrino, surpassing current experimental limits by about one order of magnitude. Recent studies have demonstrated that a reconstruction of momentum and energy of GeV particles is well feasible in liquid scintillator. Monte Carlo studies on the reconstruction of the complex event topologies found for neutrino interactions at multi-GeV energies have shown promising results. If this is confirmed, LENA might serve as far detector in a long-baseline neutrino oscillation experiment currently investigated in LAGUNA-LBNO.

Dates and versions

in2p3-00703319 , version 1 (01-06-2012)

Identifiers

Cite

Michael Wurm, John F. Beacom, Leonid B. Bezrukov, Daniel Bick, Johannes Blümer, et al.. The next-generation liquid-scintillator neutrino observatory LENA. Astroparticle Physics, 2012, 35, pp.685-732. ⟨10.1016/J.ASTROPARTPHYS.2012.02.011⟩. ⟨in2p3-00703319⟩
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