Black hole formation from massive scalar fields
Sergio M.C.V. Goncalves, Ian G. Moss

TL;DR
This paper demonstrates that under certain conditions, the gravitational collapse of a massive scalar field can be approximated as dust collapse, providing a criterion for black hole formation based on initial parameters.
Contribution
It introduces a new criterion for black hole formation from massive scalar fields by showing collapse can resemble dust under specific parameters.
Findings
Collapse can be approximated as dust in certain parameter ranges
Black hole formation depends on initial size, mass, and scalar field mass
Provides a criterion for black hole formation based on initial conditions
Abstract
It is shown that there exists a range of parameters in which gravitational collapse with a spherically symmetric massive scalar field can be treated as if it were collapsing dust. This implies a criterion for the formation of black holes depending on the size and mass of the initial field configuration and the mass of the scalar field.
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