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

Authors :
Algora A
Jordan D
Taín JL
Rubio B
Agramunt J
Perez-Cerdan AB
Molina F
Caballero L
Nácher E
Krasznahorkay A
Hunyadi MD
Gulyás J
Vitéz A
Csatlós M
Csige L
Aysto J
Penttilä H
Moore ID
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 AL
Yoshida T
Sonzogni AA
Peräjärvi K
Source :
Physical review letters [Phys Rev Lett] 2010 Nov 12; Vol. 105 (20), pp. 202501. Date of Electronic Publication: 2010 Nov 08.
Publication Year :
2010

Abstract

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.

Details

Language :
English
ISSN :
1079-7114
Volume :
105
Issue :
20
Database :
MEDLINE
Journal :
Physical review letters
Publication Type :
Academic Journal
Accession number :
21231223
Full Text :
https://doi.org/10.1103/PhysRevLett.105.202501