The next-generation liquid-scintillator neutrino observatory LENA

@article{Wurm2012TheNL,
  title={The next-generation liquid-scintillator neutrino observatory LENA},
  author={Michael Wurm and John F. Beacom and L. Bezrukov and Daniel Bick and Johannes Blumer and Sandhya Choubey and Christian Ciemniak and D. D’Angelo and Basudeb Dasgupta and Amol S. Dighe and G. V. Domogatsky and Stephen T. Dye and Sergey Eliseev and Timo Enqvist and A. N. Erykalov and F. v. Feilitzsch and Gianni Fiorentini and Tobias Fischer and Marianne Goger-Neff and P. Grabmayr and Caren Hagner and Dominikus Hellgartner and J. Hissa and Shunsaku Horiuchi and Hans-Thomas Janka and Claude Jaupart and Josef Jochum and Tuomo Kalliokoski and P. Kuusiniemi and Tobias Lachenmaier and Ionel Lazanu and John G. Learned and Timo Lewke and Paolo Lombardi and Sebastian Lorenz and Bayarto K. Lubsandorzhiev and Livia Ludhova and Kai Krister Loo and Jukka Maalampi and Fabio Mantovani and Michela Marafini and J. Maricic and Teresa Marrod'an Undagoitia and William F. McDonough and Lino Miramonti and Alessandro Mirizzi and Quirin Meindl and Olga Mena and Randolph Mollenberg and Rolf Nahnhauer and D.A. Nesterenko and Yu. N. Novikov and Guido Nuijten and Lothar Oberauer and Sandip Pakvasa and Sergio Palomares-Ruiz and Marco Pallavicini and Silvia Pascoli and Th. Patzak and Juha T. Peltoniemi and Walter Potzel and Tomi Samuli Raiha and Georg Raffelt and G. Ranucci and Soebur Razzaque and Kari Rummukainen and Juho Jaako Sarkamo and V. V. Sinev and Christian Spiering and Achim Stahl and Felicitas Andrea Thorne and Marc Tippmann and Alessandra Tonazzo and W. H. Trzaska and John D. Vergados and Christopher Wiebusch and Jurgen Winter},
  journal={Astroparticle Physics},
  year={2012},
  volume={35},
  pages={685-732}
}

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References

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Monte Carlo Study of the Fast Neutron Background in LENA

LENA (Low Energy Neutrino Astronomy) is a proposed next generation liquid-scintillator detector with about 50 kt target mass. Its main physics goals are the detection of solar neutrinos, supernova

Measurement of light emission in organic liquid scintillators and studies towards the search for proton decay in the future large-scale detector LENA

The LENA (Low Energy Neutrino Astronomy) detector is a proposed large liquid-scintillator neutrino observatory. Its main physics goals are the detection of low-energy neutrinos from the Sun, from

Towards the detection of low energy solar neutrinos in BOREXino

New challenging questions in astro-particlephysics are opened with the discovery of neutrino mass and mixing. Low energy solar neutrino spectroscopy plays now a fundamental role in understanding the

Detection potential for the diffuse supernova neutrino background in the large liquid-scintillator detector LENA

The large-volume liquid-scintillator detector LENA (low energy neutrino astronomy) will provide high-grade background discrimination and enable the detection of diffuse supernova neutrinos (DSN) in

Cosmic Background Discrimination for the Rare Neutrino Event Search in BOREXINO and LENA

Cosmogenic background has a large impact on the rare neutrino event search in liquid-scintillator detectors. In this work, an analysis of the BOREXINO muon veto efficiency and the development of a

Phenomenology of Supernova Neutrinos, Spatial Event Reconstruction, and Scintillation Light Yield Measurements for the

The LENA (Low Energy Neutrino Astronomy) project comprises a 50 kt organic liquid-scintillator detector that is in the current design planned to be of cylindrical shape with a length of ∼100 m and a
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