Galaxy formation by dissipationless particles heavier than neutrinos

Astronomy and Astrophysics – Astronomy

Scientific paper

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Cosmology, Galactic Evolution, Neutral Particles, Particle Mass, Astronomical Models, Baryons, Particle Interactions, Spiral Galaxies

Scientific paper

The 'gravitino', a spin 3/2 supersymmetric partner of the graviton which has been shown by Pagels and Primack (1982) to have a mass not greater than about 1 keV if stable, is considered as a candidate to be counted among neutral particles interacting more weakly than neutrinos, decoupling earlier, having a smaller number density today, and therefore possessing a mass greater than 50 eV without exceeding the observational mass density limit. The Jeans mass for a 1 keV noninteracting particle is about one billion solar masses, comparable to the mass of a typical spiral galaxy, including the nonluminous halo. It is suggested that a gravitino-dominated universe can produce galaxies by gravitational instability, while avoiding the observational difficulties associated with the neutrino-dominated universe.

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