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Remarks on the Beta Stability in Neutron Stars

1981
4 pages
Published in:
  • Phys.Lett.B 106 (1981) 255-258
  • Published: 1981
DOI:
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Abstract: (Elsevier)
We show that in a relativistic theory of nuclear matter the usually suppressed beta decay of neutrons n → p + e − + g ̄ n e is allowed. It can serve as a cooling mechanism. The theory also predicts the existence of real pions inside dense neutron stars. These conclusions rest primarily on the correct phenomenological description of symmetry energy in symmetric ( N = Z ) nuclear matter.
  • NUCLEAR MATTER: FIELD THEORY
  • N: SEMILEPTONIC DECAY
  • SEMILEPTONIC DECAY: N
  • DEPENDENCE: TEMPERATURE
  • APPROXIMATION: MEAN FIELD
  • PI: CONDENSATION
  • N --> P ELECTRON ANTINEUTRINO
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