Your browser doesn't support javascript.
loading
Mostrar: 20 | 50 | 100
Resultados 1 - 2 de 2
Filtrar
Más filtros

Bases de datos
Tipo de estudio
Tipo del documento
Intervalo de año de publicación
1.
Phys Rev Lett ; 120(6): 062502, 2018 Feb 09.
Artículo en Inglés | MEDLINE | ID: mdl-29481259

RESUMEN

Using Triumf's neutral atom trap, Trinat, for nuclear ß decay, we have measured the ß asymmetry with respect to the initial nuclear spin in ^{37}K to be A_{ß}=-0.5707(13)_{syst}(13)_{stat}(5)_{pol}, a 0.3% measurement. This is the best relative accuracy of any ß-asymmetry measurement in a nucleus or the neutron, and is in agreement with the standard model prediction -0.5706(7). We compare constraints on physics beyond the standard model with other ß-decay measurements, and improve the value of V_{ud} measured in this mirror nucleus by a factor of 4.

2.
Phys Rev Lett ; 108(16): 162502, 2012 Apr 20.
Artículo en Inglés | MEDLINE | ID: mdl-22680713

RESUMEN

A measurement of the final state distribution of the (8)B ß decay, obtained by implanting a (8)B beam in a double-sided silicon strip detector, is reported here. The present spectrum is consistent with a recent independent precise measurement performed by our collaboration at the IGISOL facility, Jyväskylä [O. S. Kirsebom et al., Phys. Rev. C 83, 065802 (2011)]. It shows discrepancies with previously measured spectra, leading to differences in the derived neutrino spectrum. Thanks to a low detection threshold, the neutrino spectrum is for the first time directly extracted from the measured final state distribution, thus avoiding the uncertainties related to the extrapolation of R-matrix fits. Combined with the IGISOL data, this leads to an improvement of the overall errors and the extension of the neutrino spectrum at high energy. The new unperturbed neutrino spectrum represents a benchmark for future measurements of the solar neutrino flux as a function of energy.

SELECCIÓN DE REFERENCIAS
DETALLE DE LA BÚSQUEDA