Journal
PHYSICS LETTERS B
Volume 785, Issue -, Pages 9-13Publisher
ELSEVIER
DOI: 10.1016/j.physletb.2018.07.063
Keywords
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Funding
- Government of Canada through the Department of Innovation, Science and Economic Development
- Province of Ontario through the Ministry of Research and Innovation
- Leverhulme grant [RPG-2016-233]
- Science and Facilities Council of the United Kingdom [ST/P000371/1]
- STFC [ST/P000371/1] Funding Source: UKRI
- Science and Technology Facilities Council [ST/P000371/1] Funding Source: researchfish
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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. (C) 2018 The Author(s). Published by Elsevier B.V.
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