On instabilities of scalar hairy regular compact reflecting stars
Abstract We study the system constructed by charged scalar fields linearly coupled to asymptotically flat horizonless compact reflecting stars. We obtain bounds on the charge of the scalar field, below which the scalar hairy star is expected to suffer from nonlinear instabilities. It means that scal...
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Format: | Article |
Language: | English |
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SpringerOpen
2018-10-01
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Series: | Journal of High Energy Physics |
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Online Access: | http://link.springer.com/article/10.1007/JHEP10(2018)185 |
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author | Yan Peng |
author_facet | Yan Peng |
author_sort | Yan Peng |
collection | DOAJ |
description | Abstract We study the system constructed by charged scalar fields linearly coupled to asymptotically flat horizonless compact reflecting stars. We obtain bounds on the charge of the scalar field, below which the scalar hairy star is expected to suffer from nonlinear instabilities. It means that scalar hairy regular configurations are unstable for scalar fields of small charge. For the highly-charged star, there are also bounds on radii of regular compact reflecting stars. When the star radius is below the bound, the hairy star is always unstable. |
first_indexed | 2024-12-13T07:48:58Z |
format | Article |
id | doaj.art-b00b47fa423041adbde3558308b9ab06 |
institution | Directory Open Access Journal |
issn | 1029-8479 |
language | English |
last_indexed | 2024-12-13T07:48:58Z |
publishDate | 2018-10-01 |
publisher | SpringerOpen |
record_format | Article |
series | Journal of High Energy Physics |
spelling | doaj.art-b00b47fa423041adbde3558308b9ab062022-12-21T23:54:44ZengSpringerOpenJournal of High Energy Physics1029-84792018-10-012018101910.1007/JHEP10(2018)185On instabilities of scalar hairy regular compact reflecting starsYan Peng0School of Mathematical Sciences, Qufu Normal UniversityAbstract We study the system constructed by charged scalar fields linearly coupled to asymptotically flat horizonless compact reflecting stars. We obtain bounds on the charge of the scalar field, below which the scalar hairy star is expected to suffer from nonlinear instabilities. It means that scalar hairy regular configurations are unstable for scalar fields of small charge. For the highly-charged star, there are also bounds on radii of regular compact reflecting stars. When the star radius is below the bound, the hairy star is always unstable.http://link.springer.com/article/10.1007/JHEP10(2018)185Black HolesClassical Theories of Gravity |
spellingShingle | Yan Peng On instabilities of scalar hairy regular compact reflecting stars Journal of High Energy Physics Black Holes Classical Theories of Gravity |
title | On instabilities of scalar hairy regular compact reflecting stars |
title_full | On instabilities of scalar hairy regular compact reflecting stars |
title_fullStr | On instabilities of scalar hairy regular compact reflecting stars |
title_full_unstemmed | On instabilities of scalar hairy regular compact reflecting stars |
title_short | On instabilities of scalar hairy regular compact reflecting stars |
title_sort | on instabilities of scalar hairy regular compact reflecting stars |
topic | Black Holes Classical Theories of Gravity |
url | http://link.springer.com/article/10.1007/JHEP10(2018)185 |
work_keys_str_mv | AT yanpeng oninstabilitiesofscalarhairyregularcompactreflectingstars |