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arXiv · gr-qc/9506044

The spherically symmetric collapse of a massless scalar field

Rufus S. Hamade·John M. Stewart
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Abstract

We report on a numerical study of the spherically symmetric collapse of a self-gravitating massless scalar field. Earlier results of Choptuik(1992, 1994) are confirmed. The field either disperses to infinity or collapses to a black hole, depending on the strength of the initial data. For evolutions where the strength is close to but below the strength required to form a black hole, we argue that there will be a region close to the axis where the scalar curvature and field energy density can reach arbitrarily large levels, and which is visible to distant observers

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Rufus S. Hamade, John M. Stewart. 1995-06-22. The spherically symmetric collapse of a massless scalar field. https://doi.org/10.1088/0264-9381%2F13%2F3%2F014

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