http://arxiv.org/abs/1907.08193
In this manuscript the three types of late-time behavior of spherically symmetric Boson Stars are presented, these are: stable configurations, unstable bounded that collapse to form black holes and unstable unbounded that explode. The results are found by solving the spherically symmetric Einstein-Klein-Gordon system of equations for a complex scalar field with initial conditions corresponding to a Boson Star. The solution is based on a constrained evolution that uses the method of lines for the scalar field and solves the constraint equations for the geometry on the fly.
F. Guzman
Mon, 22 Jul 19
3/45
Comments: 8 pages. Academic paper published in the Mexican Journal of Physics back in 2009. arXiv admin note: text overlap with arXiv:1007.1162
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