Physical Review Letters · 1988 · 503 citations · 15 references
Natural SciencesPhysicsAstrophysicsNuclear PhysicsParticle PhysicsNeutrino PhysicsNeutron StarsNuclear ForcesStrong InteractionAxion PhysicsDirac NeutrinosElementary Particle InteractionsNeutrino Emission ProcessesNeutrino Mass ConstraintsNeutron Star PhysicsParticle InteractionsParticle-particle Interactions
The observation of a neutrino pulse from the supernova SN1987A constrains the production of light exotic particles in the proto neutron star. We derive a new bound on the axion decay constant, ${f}_{a}$\ensuremath{\gtrsim}${10}^{10}$ GeV. If right-handed (RH) neutrinos exist, the ``RH Fermi constant'' is ${G}_{\mathrm{RH}\ensuremath{\lesssim}{10}^{\mathrm{\ensuremath{-}}4}{G}_{\mathrm{F}}}$, 2 orders of magnitude below laboratory bounds. The Dirac mass of ${\ensuremath{\nu}}_{\ensuremath{\mu}}$ can be constrained below laboratory limits.
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Observation of a neutrino burst from the supernova SN1987A
Keiko Hirata, T. Kajita, M. Koshiba et al. · Physical Review Letters · 1987 · 2K citations · Full text
Michael S. Turner · Physical Review Letters · 1988 · 383 citations
Mark Srednicki · Nuclear Physics B · 1985 · 357 citations
Neutrino emissivities of neutron stars
Bengt Friman, O.V. Maxwell · The Astrophysical Journal · 1979 · 342 citations
Natural Sciences, Astronomy, Physics +13