Thermonuclear Pion Production and High Temperature Stars

Details Thermonuclear Pion Production and High Temperature Stars Thermonuclear Pion Production and High Temperature Stars

Aug 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969natur.223..725f&link_type=abstract

Nature, Volume 223, Issue 5207, pp. 725-726 (1969).

Mathematics

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Scientific paper

PIONS may be produced in thermonuclear interactions between nucleons in material at a temperature >~1010 K. Pion production followed by secondary interaction is among the many processes contributing to the statistical equilibrium of a high temperature astrophysical system. Charged pions do, however, undergo decay as an alternative to secondary interaction, producing μ-neutrinos (vμ) if these neutrinos have a high escape probability, their emission may cause an appreciable energy loss from the system.

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