Abstract
The Solar Maximum Mission satellite did not record any γ-ray counts in excess of the background for a time interval of 223 s after the arrival of the first νe's from the supernova 1987A. On the basis of the original data we derive a new 3σ upper limit on the γ fluence for this period and derive improved bounds on the νi → νjγ and νT → νee-e+γ radiative decay channels for neutrino masses up to the experimentally allowed value of around 30 MeV.
| Original language | English |
|---|---|
| Pages (from-to) | 377-386 |
| Number of pages | 10 |
| Journal | Astroparticle Physics |
| Volume | 1 |
| Issue number | 4 |
| DOIs | |
| State | Published - Dec 1993 |
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