The next-generation liquid-scintillator neutrino observatory LENA

M Wurm, JF Beacom, LB Bezrukov, D Bick, J Blümer… - Astroparticle …, 2012 - Elsevier
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 …

Liquid helium and liquid neon-sensitive, low background scintillation media for the detection of low energy neutrinos

DN McKinsey, JM Doyle - Journal of Low Temperature Physics, 2000 - Springer
The use of liquid helium and neon as scintillators for neutrino detection is investigated.
Several unique properties of these cryogens make them promising candidates for real-time …

Review of the technical issues associated with the construction of a solar neutrino TPC

G Bonvicini, D Naples, V Paolone - Nuclear Instruments and Methods in …, 2002 - Elsevier
Review of the technical issues associated with the construction of a solar neutrino TPC -
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[HTML][HTML] Physics results from RICH detectors

S Stone - Nuclear Instruments and Methods in Physics Research …, 1999 - Elsevier
RICH detectors have become extraordinarily useful. Results include measurement of solar
neutrino rates, evidence for neutrino oscillations, measurement of TeV γ-rays from …

[HTML][HTML] Towards low-threshold, real-time solar neutrino detectors

G Gratta, YF Wang - Nuclear Instruments and Methods in Physics Research …, 1999 - Elsevier
We discuss an alternative approach to the detection of solar neutrinos using a coarsely
segmented detector based on inverse-beta decay onto 160Gd or 176Yb. While it is known …

[PDF][PDF] PoS (Texas 2010) 209 Direct dark matter search using liquid noble gases

TM Undagoitia - 2010 - s3.cern.ch
Indirect evidence for cold dark matter is well established from astronomical observations but
the nature of this matter is still unknown. One very popular candidate is the Weakly …

[PDF][PDF] Puzzling out neutrino mixing through golden measurements

OM Requejo - 2002 - inspirehep.net
As it has been shown in the last chapter, the oscillation probabilities for three light neutrino
generations are described by two squared mass differences (∆ m2 12 and∆ m2 13), three …