arXiv · hep-ph/9710404
Neutrino helicity flip by Cerenkov emission and absorption of plasmons in supernova
Abstract
We show that in a supernova core the longitudinal photon (plasmon) has a space-like dispersion and Cerenkov absorption and emission of such photons is kinematically allowed. If the neutrino has a non-zero magnetic moment, then helicity flipping Cerenkov absorption of a plasmon $ν_L+γ\toν_R$ is the most efficient cooling mechanism of the supernova core, and this allows us to put a restrictive bound on the neutrino magnetic moment $μ_ν~<~0.7\times 10^{-13}μ_B$.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Subhendra Mohanty, Sarira Sahu. 1997-10-20. Neutrino helicity flip by Cerenkov emission and absorption of plasmons in supernova. https://arxiv.org/abs/hep-ph/9710404
Cite the original work for its findings. Save a collection to share your selection of sources.