Experimental limit on a 17 keV neutrino branch in the beta decay of 177Lu

1992 ◽  
Vol 28 (1) ◽  
pp. 176-178
Author(s):  
S. Schönert ◽  
K. Schreckenbach ◽  
S. Neumaier ◽  
F.v. Feilitzsch
1983 ◽  
Vol 121 (1) ◽  
pp. 72-76 ◽  
Author(s):  
E. Bellotti ◽  
E. Fiorini ◽  
C. Liguori ◽  
A. Pullia ◽  
A. Sarracino ◽  
...  

2007 ◽  
Vol 2007 ◽  
pp. 1-15 ◽  
Author(s):  
Alexander Merle ◽  
Werner Rodejohann

We consider the possibility to gain information on the lepton mixing matrix element|Ue3|from an improved experimental limit on the effective neutrino mass governing neutrinoless double beta decay. We show that typically a lower limit on|Ue3|as a function of the smallest neutrino mass can be set. Furthermore, we give the values of the sum of neutrino masses and|Ue3|which are allowed and forbidden by an experimental upper limit on the effective mass. Alternative explanations for neutrinoless double beta decay, Dirac neutrinos or unexplained cosmological features would be required if future measurements showed that the values lie in the respective regions. Moreover, we show that a measurement of|Ue3|from neutrinoless double beta decay is very difficult due to the expected errors on the effective mass and the oscillation parameters.


1982 ◽  
Vol 43 (C8) ◽  
pp. C8-261-C8-300
Author(s):  
E. Amaldi
Keyword(s):  

1977 ◽  
Vol 123 (12) ◽  
pp. 692 ◽  
Author(s):  
B.G. Erozolimskii
Keyword(s):  

Author(s):  
Roger H. Stuewer

Serious contradictions to the existence of electrons in nuclei impinged in one way or another on the theory of beta decay and became acute when Charles Ellis and William Wooster proved, in an experimental tour de force in 1927, that beta particles are emitted from a radioactive nucleus with a continuous distribution of energies. Bohr concluded that energy is not conserved in the nucleus, an idea that Wolfgang Pauli vigorously opposed. Another puzzle arose in alpha-particle experiments. Walther Bothe and his co-workers used his coincidence method in 1928–30 and concluded that energetic gamma rays are produced when polonium alpha particles bombard beryllium and other light nuclei. That stimulated Frédéric Joliot and Irène Curie to carry out related experiments. These experimental results were thoroughly discussed at a conference that Enrico Fermi organized in Rome in October 1931, whose proceedings included the first publication of Pauli’s neutrino hypothesis.


1988 ◽  
Vol 330 (3) ◽  
pp. 341-342 ◽  
Author(s):  
D. Barn�oud ◽  
J. Blachot ◽  
J. Genevey ◽  
A. Gizon ◽  
R. B�raud ◽  
...  
Keyword(s):  

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