Global Textures and The Formation of Self-Bound Gravitational Systems

Details Global Textures and The Formation of Self-Bound Gravitational Systems Global Textures and The Formation of Self-Bound Gravitational Systems

1999-06-09

arxiv.org/abs/astro-ph/9906172v1

Astronomy and Astrophysics

Astrophysics

6 pages, 4 figures, to be published in MNRAS

Scientific paper

10.1046/j.1365-8711.1999.02850.x

Using a Newtonian approximation, we developed a quantitative criterion for
the collapse of a spherical distribution of matter under an isolated texture
field. In particular, we found that the evolution of an overdense region is
strongly determined by two parameters: the energy scale of symmetry breaking
and the initial radius of the system.

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