Fractionally Charged Heavy Leptons: Cosmological Implications of Their Existence, and a Prediction of Their Abundance

Details Fractionally Charged Heavy Leptons: Cosmological Implications of Their Existence, and a Prediction of Their Abundance Fractionally Charged Heavy Leptons: Cosmological Implications of Their Existence, and a Prediction of Their Abundance

May 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982phrvl..48.1518g&link_type=abstract

Physical Review Letters, Volume 48, Issue 22, May 31, 1982, pp.1518-1521

Physics

15

Elementary Particle Processes, Background Radiations, Origin And Formation Of The Universe

Scientific paper

Charge +/-13 heavy leptons can annihilate in heavy stars down to an abundance of 10-19, without generating an isotropic γ-ray background. Observation of such leptons with this abundance, and the observed flux of cosmic neutrinos imply that (1) there is no primordial hydrogen on earth, (a) the first stars were heavy (M>~15Msolar), and (3) their formation took place at a red shift 1+z>~20.

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