A lower limit to the mass of neutral leptons as constituents of the dark halo around galaxies

Details A lower limit to the mass of neutral leptons as constituents of the dark halo around galaxies A lower limit to the mass of neutral leptons as constituents of the dark halo around galaxies

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.137...17c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 137, no. 1, Oct. 1987, p. 17-21.

Astronomy and Astrophysics

Astrophysics

2

Dark Matter, Leptons, Particle Mass, Range (Extremes), Spiral Galaxies, Neutral Particles, Plasma Equilibrium, Plasma Temperature

Scientific paper

The authors have found that the structural equations governing the hydrostatic equilibrium of a thermally relaxed, spherically-symmetric neutral lepton system with a density profile that can account for the dark matter distribution around spiral galaxies do not admit any physically reasonable solutions (namely, the temperature should be positive definite and monotonically decreasing with distance) if the lepton mass is L ⪉ 17 eV.

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