String-seeded spirals - Origin of rotation and the density of the halo

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Galactic Evolution, Galactic Rotation, Space Density, Spiral Galaxies, String Theory, Density Distribution, Gravitational Collapse, Halos, Missing Mass (Astrophysics)

Scientific paper

Galactic halos seeded by loops of string in a universe dominated by dark matter fall into two categories: (1) Non-self-intersecting loops precipitate nearly spherically symmetric collapse and lead to a halo with low angular momentum J and a density profile ρ ≡ r-9/4. (2) Progeny of a self-intersecting primary loop recollapse into a single object which acquires J through tidal interactions. Its density profile, ρ ≡ r-2, is consistent with "flat rotation profiles" observed in spiral galaxies. It is tempting to identify these two types of string-seeded objects with (1) elliptical and (2) spiral galaxies.

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