Core Collapse via Coarse Dynamic Renormalization

Details Core Collapse via Coarse Dynamic Renormalization Core Collapse via Coarse Dynamic Renormalization

2005-04-25

arxiv.org/abs/astro-ph/0504546v2

Phys.Rev.Lett. 95 (2005) 081102

Astronomy and Astrophysics

Astrophysics

5 pages, 3 figures

Scientific paper

10.1103/PhysRevLett.95.081102

In the context of the recently developed "equation-free" approach to computer-assisted analysis of complex systems, we extract the self-similar solution describing core collapse of a stellar system from numerical experiments. The technique allows us to side-step the core "bounce" that occurs in direct N-body simulations due to the small-N correlations that develop in the late stages of collapse, and hence to follow the evolution well into the self-similar regime.

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