The laboratory and astrophysical constraints on the neutrino charge radius

Details The laboratory and astrophysical constraints on the neutrino charge radius The laboratory and astrophysical constraints on the neutrino charge radius

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aph.....2..269s&link_type=abstract

Astroparticle Physics, Volume 2, Issue 3, p. 269-290.

Physics

9

Scientific paper

If the properties of neutrino magnetic moments have been extensively studied, the consequences of a non-vanishing charge radius have drawn little attention so far. The laboratory bounds are reviewed. They are fairly comparable to the constraints set by the cooling of red-giant stars. The relevance of anapole neutrinos to the explosion mechanism of massive stars is also discussed. As a matter of fact, if neutrinos have an anomalous charge radius, they can drag some fraction of the gravitational energy released during the collapse of a compact object. As they transfer it to the envelope of the supernova, neutrinos revitalize the stalled shock wave.

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