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Relativistic collapse of axion stars.

Michel, Florent and Moss, Ian G. (2018) 'Relativistic collapse of axion stars.', Physics letters B., 785 . pp. 9-13.

Abstract

We study the gravitational collapse of axion dark matter in null coordinates, assuming spherical symmetry. Compared with previous studies, we use a simpler numerical scheme which can run, for relevant parameters, in a few minutes or less on a desktop computer. We use it to accurately determine the domains of parameter space in which the axion field forms a black hole, an axion star or a relativistic Bosenova.

Item Type:Article
Full text:(VoR) Version of Record
First Live Deposit - 06 September 2018
Available under License - Creative Commons Attribution.
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Status:Peer-reviewed
Publisher Web site:https://doi.org/10.1016/j.physletb.2018.07.063
Publisher statement:© 2018 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).
Record Created:06 Sep 2018 15:13
Last Modified:06 Sep 2018 15:21

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