CLEAN

(Cryogenic Low Energy Astrophysics with Noble gases)

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References

1 - Articles

[1-1]
Neutrino Detection With CLEAN, D. N. McKinsey, K. J. Coakley, Astropart. Phys. 22 (2005) 355, arXiv:astro-ph/0402007.
[McKinsey:2004rk]
[1-2]
Supernova observation via neutrino nucleus elastic scattering in the CLEAN detector, Charles J. Horowitz, K. J. Coakley, D. N. McKinsey, Phys. Rev. D68 (2003) 023005, arXiv:astro-ph/0302071.
[Horowitz:2003cz]

2 - Detector

[2-1]
Liquid Helium and Liquid Neon - Sensitive, Low Background Scintillation Media For the Detection of Low Energy Neutrinos, D. N. McKinsey, J. M. Doyle, J.Low.Temp.Phys. 118 (2000) 153-165, arXiv:astro-ph/9907314.
[McKinsey:1999yg]

3 - Conference Proceedings

[3-1]
CLEAN: A self-shielding detector for characterizing the low energy solar neutrino spectrum, D. N. McKinsey, 2000. Low energy solar neutrino detection, Tokyo, 2000.
[McKinsey:2000ra]

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Authors:
Stefano Gariazzo / gariazzo@to.infn.it
Carlo Giunti / giunti@to.infn.it
Marco Laveder / marco.laveder@pd.infn.it
Last Update: Wed 20 Sep 2017, 09:48:52 UTC