Astronomical observations at the x-ray, optical, and radio frequencies are used to show that the lifetime of neutrinos for radiative decay divided by the rest mass, Τ0/mν, exceeds 1017 sec/eV. If one makes the further assumption that mν>10-3 eV, then Τ0>~1019 sec. If there are other competing decays of neutrinos, it is then shown that Γνe(νe→x+γ)/Γνe(total)<~10-15 and Γνμ(νμ→x+γ)/Γνμ(total)<~3×10-6
12 pages, LaTeX 2e (epsf) with 9 postscript figures and one logo. Some comments and references added...
AbstractWe propose that supernova relic neutrino (SRN) observation can be used to set constraints on...
We investigate the radiative decay of the cosmic neutrino background and its impact on the spectrum ...
Astronomical observations at the x-ray, optical, and radio frequencies are used to show that the lif...
Neutrino oscillation experiments and direct bounds on absolute masses constrain neutrino mass differ...
Neutrino oscillation experiments and direct bounds on absolute masses constrain neutrino mass differ...
It is pointed out that the cores of massive stars reach temperatures of the order of 10 MeV during t...
The long baseline between Earth and the Sun makes solar neutrinos an excellent test beam for explori...
The long baseline between Earth and the Sun makes solar neutrinos an excellent test beam for explori...
Restricted AccessWe calculate constraints on radiatively decaying neutrinos from the recent detectio...
Discovering neutrino decay would be strong evidence of new physics. Presently, there are only lax lo...
Astronomical observations of SN1987A, such as the light curve, spectral intensities of lines, the X-...
We consider the decay of massive neutrinos which couple to electrons and are, therefore, produced in...
Double beta decay of 128Te has been confirmed and the ratio of half-lives for ββ decay of ...
The radiative lifetime tau for the decay of massious neutrinos was calculated using various physical...
12 pages, LaTeX 2e (epsf) with 9 postscript figures and one logo. Some comments and references added...
AbstractWe propose that supernova relic neutrino (SRN) observation can be used to set constraints on...
We investigate the radiative decay of the cosmic neutrino background and its impact on the spectrum ...
Astronomical observations at the x-ray, optical, and radio frequencies are used to show that the lif...
Neutrino oscillation experiments and direct bounds on absolute masses constrain neutrino mass differ...
Neutrino oscillation experiments and direct bounds on absolute masses constrain neutrino mass differ...
It is pointed out that the cores of massive stars reach temperatures of the order of 10 MeV during t...
The long baseline between Earth and the Sun makes solar neutrinos an excellent test beam for explori...
The long baseline between Earth and the Sun makes solar neutrinos an excellent test beam for explori...
Restricted AccessWe calculate constraints on radiatively decaying neutrinos from the recent detectio...
Discovering neutrino decay would be strong evidence of new physics. Presently, there are only lax lo...
Astronomical observations of SN1987A, such as the light curve, spectral intensities of lines, the X-...
We consider the decay of massive neutrinos which couple to electrons and are, therefore, produced in...
Double beta decay of 128Te has been confirmed and the ratio of half-lives for ββ decay of ...
The radiative lifetime tau for the decay of massious neutrinos was calculated using various physical...
12 pages, LaTeX 2e (epsf) with 9 postscript figures and one logo. Some comments and references added...
AbstractWe propose that supernova relic neutrino (SRN) observation can be used to set constraints on...
We investigate the radiative decay of the cosmic neutrino background and its impact on the spectrum ...