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Autor:
Aittola, M. (Marko), Enqvist, T. (Timo), Bezrukov, L. B. (L. B.), Gangapshev, A. M. (A. M.), Gavrilyuk, Y. M. (Y. M.), Hissa, J. (Johannes), Joutsenvaara, J. (Jari), Kazalov, V. V. (V. V.), Kutuniva, J. (Johanna), Kuusiniemi, P. (Pasi), Kuzminov, V. V. (V. V.), Loo, K. (K.), Lubsandorzhiev, B. K. (B. K.), Morgalyuk, V. P. (V. P.), Novikova, G. Y. (G. Y.), Sinev, V. V. (V. V.), Slupecki, M. (M.), Trzaska, W. H. (W. H.), Virkajärvi, A. (Antto), Yanovich, Y. A. (Y. A.)
In order to detect low-energy neutrinos, for example the solar neutrinos from the ppchain (with the maximum neutrino energy of approximately 400 keV) requires that the intrinsic ¹⁴C content in a liquid scintillator is at extremely low level. In th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2423::623de815c56f822ac07339f77233ea54
http://urn.fi/urn:nbn:fi-fe201701101095
http://urn.fi/urn:nbn:fi-fe201701101095