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Title: Some astrophysical consequences of the existence of a heavy stable neutral lepton

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/156335· OSTI ID:6650459

Recently, high-energy particle theorists have constructed new extended gauge theories which may fit experiment somewhat better than previous already very successful theories. One of the predictions which is often discussed is the possible existence of a stable neutral lepton, probably with a mass of a few GeV/c/sup 2/. Following this motivation we here investigate some cosmological consequences of the existence of any stable, massive, neutral lepton, and show that it could well dominate the present mass density in the universe. The contribution to the mass density depends on the mass of the lepton, which should eventually be determined with high-energy accelerators. It is interesting that the more massive the lepton, the smaller its contribution to the present mass density. It is unlikely that these leptons affect big bang nucleosynthesis or condense into stellar size objects. However, such a lepton is an excellent candidate for the material in galactic halos and for the mass required to bind the great clusters of galaxies. Annihilation radiation from these structures should be detectable. At the end of the paper a brief mention is made of the astrophysical constraints on the mass-lifetime relationship if the neutral lepton is unstable.

Research Organization:
California Institute of Technology (CalTech), Pasadena, CA (United States); and Institute of Astronomy, Cambridge, England
OSTI ID:
6650459
Journal Information:
Astrophys. J.; (United States), Vol. 223:3
Country of Publication:
United States
Language:
English