Physics
Scientific paper
Oct 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...273..330s&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 273, Oct. 1, 1983, p. 330-345.
Physics
4
Flavor (Particle Physics), Neutrinos, Particle Emission, Plasma Density, Pressure Distribution, Stellar Atmospheres, Stellar Temperature, Energy Distribution, Gravitational Collapse, Hydrostatics
Scientific paper
The authors have solved the problem of a plane-parallel, static neutrino atmosphere in which all three flavors of neutrinos (electron, μ, and τ) and antineutrinos transport energy, momentum, and their respective lepton numbers. The authors have assumed a gas consisting of free, nondegenerate, nonrelativistic nucleons, extreme relativistic electrons and positrons of arbitrary degeneracy, and photons. The transport equations for electron, μ, and τ neutrinos and antineutrinos are solved subject to the constraints of hydrostatic equilibrium, conservation of energy flux, and conservation of electron, μ, and τ lepton number fluxes. It is found that three-flavored atmospheres are cooler and denser than the electron flavored atmospheres described in an earlier paper.
Schinder Paul J.
Shapiro Stuart L.
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