Neutrino processes and pair formation in massive stars and supernovae.

  title={Neutrino processes and pair formation in massive stars and supernovae.},
  author={William A. Fowler and Fred Sir Hoyle},
  journal={Astrophysical Journal Supplement Series},
  • W. Fowler, F. Hoyle
  • Published 1 December 1964
  • Physics
  • Astrophysical Journal Supplement Series
Abstract : The paper traces the physical properties of matter inside highly evolved stars, on the assumption that the whole material of the star is non-degenerate and that the star is in quasi-hydrostatic equilibrium. When these conditions are satisfied, the physical evolution of a particular element of material is insensitive to the stallar model but not to the total mass of the star. Our considerations refer explicity to stars of mass greater than approx. 10 micro sun but less than 1,000,000… 
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