Reactor decay heat in 239Pu: solving the γ discrepancy in the 4-3000-s cooling period

The β feeding probability of (102,104,105,106,107)Tc, 105Mo, and 101Nb nuclei, which are important contributors to the decay heat in nuclear reactors, has been measured using the total absorption technique. We have coupled for the first time a total absorption spectrometer to a Penning trap in order...

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Veröffentlicht in:Physical review letters 2010-11, Vol.105 (20), p.202501-202501
Hauptverfasser: Algora, A, Jordan, D, Taín, J L, Rubio, B, Agramunt, J, Perez-Cerdan, A B, Molina, F, Caballero, L, Nácher, E, Krasznahorkay, A, Hunyadi, M D, Gulyás, J, Vitéz, A, Csatlós, M, Csige, L, Aysto, J, Penttilä, H, Moore, I D, Eronen, T, Jokinen, A, Nieminen, A, Hakala, J, Karvonen, P, Kankainen, A, Saastamoinen, A, Rissanen, J, Kessler, T, Weber, C, Ronkainen, J, Rahaman, S, Elomaa, V, Rinta-Antila, S, Hager, U, Sonoda, T, Burkard, K, Hüller, W, Batist, L, Gelletly, W, Nichols, A L, Yoshida, T, Sonzogni, A A, Peräjärvi, K
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container_end_page 202501
container_issue 20
container_start_page 202501
container_title Physical review letters
container_volume 105
creator Algora, A
Jordan, D
Taín, J L
Rubio, B
Agramunt, J
Perez-Cerdan, A B
Molina, F
Caballero, L
Nácher, E
Krasznahorkay, A
Hunyadi, M D
Gulyás, J
Vitéz, A
Csatlós, M
Csige, L
Aysto, J
Penttilä, H
Moore, I D
Eronen, T
Jokinen, A
Nieminen, A
Hakala, J
Karvonen, P
Kankainen, A
Saastamoinen, A
Rissanen, J
Kessler, T
Weber, C
Ronkainen, J
Rahaman, S
Elomaa, V
Rinta-Antila, S
Hager, U
Sonoda, T
Burkard, K
Hüller, W
Batist, L
Gelletly, W
Nichols, A L
Yoshida, T
Sonzogni, A A
Peräjärvi, K
description The β feeding probability of (102,104,105,106,107)Tc, 105Mo, and 101Nb nuclei, which are important contributors to the decay heat in nuclear reactors, has been measured using the total absorption technique. We have coupled for the first time a total absorption spectrometer to a Penning trap in order to obtain sources of very high isobaric purity. Our results solve a significant part of a long-standing discrepancy in the γ component of the decay heat for 239Pu in the 4-3000 s range.
doi_str_mv 10.1103/PhysRevLett.105.202501
format Article
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source American Physical Society Journals
subjects ABSORPTION
FEEDING
national nuclear data center
NUCLEAR PHYSICS AND RADIATION PHYSICS
NUCLEI
PROBABILITY
REACTORS
SPECTROMETERS
title Reactor decay heat in 239Pu: solving the γ discrepancy in the 4-3000-s cooling period
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