Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Kuzminov, V. V. (V. V.)"'
Autor:
Enqvist, T. (T), Barabanov, R. (R), Bezrukov, L. B. (L B), Gangapshev, A. M. (A M), Gavrilyuk, Y. M. (Y M), Grishina, V. Y. (V Yu), Gurentsov, V. I. (V I), Hissa, J. (J), Joutsenvaara, J. (J), Kazalov, V. V. (V V), Krokhaleva, S. (S), Kutuniva, J. (J), Kuusiniemi, P. (P), Kuzminov, V. V. (V V), Kurlovich, A. S. (A S), Loo, K. (K), Lubsandorzhiev, B. K. (B K), Lubsandorzhiev, S. (S), Morgalyuk, V. P. (V P), Novikova, G. Y. (G Y), Pshukov, A. M. (A M), Sinev, V. V. (V V), Słupecki, M. (M), Trzaska, W. H. (W H), Umerov, S. I. (Sh I), Veresnikova, A. V. (A V), Virkajärvi, A. (A), Yanovich, Y. A. (Y A), Zavarzina, V. P. (V P)
A series of measurements has been started where the ¹⁴C concentration is determined from several liquid scintillator samples. A dedicated setup has been designed and constructed with the aim of measuring concentrations smaller than 10−18. Measur
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2423::02e1a92dc3308dcc7b52b90c6bd26a71
http://urn.fi/urn:nbn:fi-fe201803095138
http://urn.fi/urn:nbn:fi-fe201803095138
Autor:
Enqvist, T. (Timo), Barabanov, I. R. (I. R.), Bezrukov, L. B. (L. B.), Gangapshev, A. M. (A. M.), Gavrilyuk, Y. M. (Y. M.), Grishina, V. Y. (V. Yu.), Gurentsov, V. I. (V. I.), Hissa, J. (J.), Joutsenvaara, J. (Jari), Kazalov, V. V. (V. V.), Krokhaleva, S. (S.), Kutuniva, J. (Johanna), Kuusiniemi, P. (Pasi), Kuzminov, V. V. (V. V.), Kurlovich, A. S. (A. S.), Loo, K. (K.), Lubsandorzhiev, B. K. (B. K.), Lubsandorzhiev, S. (S.), Morgalyuk, V. P. (V. P.), Novikova, G. Y. (G. Y.), Pshukov, A. M. (A. M.), Sinev, V. V. (V. V.), Słupeckic, M. (M.), Trzaska, W. H. (W. H.), Umerov, S. I. (Sh. I.), Veresnikova, A. V. (A. V.), Virkajärvi, A. (A.), Yanovich, Y. A. (Y. A.), Zavarzina, V. P. (V. P.)
The main background hindering low-energy (≲ 200 keV) neutrino measurements with liquid scintillators comes from the minute remanence of the cosmogenic ¹⁴C (T₁/₂ ≃ 5700 a) present in the organic oil constituting the bulk of the scintillator
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2423::fccc87696e930a120cadadef148d2419
http://urn.fi/urn:nbn:fi-fe201701091076
http://urn.fi/urn:nbn:fi-fe201701091076
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