Higgs meson emission from a star and a constraint on its mass

Details Higgs meson emission from a star and a constraint on its mass Higgs meson emission from a star and a constraint on its mass

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pthph..54.1564s&link_type=abstract

Progress of Theoretical Physics, vol. 54, Nov. 1975, p. 1564, 1565. Research supported by the Soryushi Shogakukai.

Physics

38

Mesons, Particle Emission, Particle Mass, Stellar Mass Ejection, Background Radiation, Range (Extremes), Stellar Evolution

Scientific paper

In Weinberg's (1967) unified theory of weak and electromagnetic interaction, Higgs mesons must necessarily be present, but their mass is arbitrary. In a previous discussion of the contribution of primordial Higgs mesons to the cosmic background radiation, it was shown that the mass cannot lie in the range from 0.1 to 100 eV. In the present paper, the emission of Higgs mesons from stars is analyzed, and it is argued that a mass range below 0.7 x (electron mass) must be ruled out; otherwise the emission process would have a drastic effect on the evolution of stars.

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