Charged particle production rate from cosmic censorship in dilaton black hole spacetimes
Abstract Hiscock and Weems showed that under Hawking evaporation, an isolated asymptotically flat Reissner-Nordström (RN) black hole evolves in a surprising manner: if it starts with a relatively small value of charge-to-mass ratio Q/M, then said value will temporarily increase along its evolutionar...
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| Format: | Article |
| Language: | English |
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SpringerOpen
2019-10-01
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| Series: | Journal of High Energy Physics |
| Subjects: | |
| Online Access: | http://link.springer.com/article/10.1007/JHEP10(2019)129 |
| _version_ | 1818336963855384576 |
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| author | Yen Chin Ong Yuan Yao |
| author_facet | Yen Chin Ong Yuan Yao |
| author_sort | Yen Chin Ong |
| collection | DOAJ |
| description | Abstract Hiscock and Weems showed that under Hawking evaporation, an isolated asymptotically flat Reissner-Nordström (RN) black hole evolves in a surprising manner: if it starts with a relatively small value of charge-to-mass ratio Q/M, then said value will temporarily increase along its evolutionary path, before finally decreases towards zero. This contrasts with highly charged ones that simply radiate away its charge steadily. The combination of these two effects is the cosmic censor at work: there exists an attractor that flows towards the Schwazschild limit, which ensures that extremality — and hence naked singularity — can never be reached under Hawking evaporation. We apply the scheme of Hiscock and Weems to model the evaporation of an asymptotically flat dilatonic charge black hole known as the Garfinkle-Horowitz-Strominger (GHS) black hole. We found that upholding the cosmic censorship requires us to modify the charged particle production rate, which remarkably agrees with the expression obtained independently via direct computation of charged particle production rate on curved spacetime background. This not only strengthens the case for cosmic censorship, but also provides an example in which cosmic censorship can be a useful principle to deduce other physics. We also found that the attractor behavior is not necessarily related to the specific heat, contrary to the claim by Hiscock and Weems. |
| first_indexed | 2024-12-13T14:47:40Z |
| format | Article |
| id | doaj.art-1a148d5c47eb4d41acff746d99a88f65 |
| institution | Directory Open Access Journal |
| issn | 1029-8479 |
| language | English |
| last_indexed | 2024-12-13T14:47:40Z |
| publishDate | 2019-10-01 |
| publisher | SpringerOpen |
| record_format | Article |
| series | Journal of High Energy Physics |
| spelling | doaj.art-1a148d5c47eb4d41acff746d99a88f652022-12-21T23:41:25ZengSpringerOpenJournal of High Energy Physics1029-84792019-10-0120191012510.1007/JHEP10(2019)129Charged particle production rate from cosmic censorship in dilaton black hole spacetimesYen Chin Ong0Yuan Yao1Center for Gravitation and Cosmology, College of Physical Science and Technology, Yangzhou UniversitySchool of Aeronautics and Astronautics, Shanghai Jiao Tong UniversityAbstract Hiscock and Weems showed that under Hawking evaporation, an isolated asymptotically flat Reissner-Nordström (RN) black hole evolves in a surprising manner: if it starts with a relatively small value of charge-to-mass ratio Q/M, then said value will temporarily increase along its evolutionary path, before finally decreases towards zero. This contrasts with highly charged ones that simply radiate away its charge steadily. The combination of these two effects is the cosmic censor at work: there exists an attractor that flows towards the Schwazschild limit, which ensures that extremality — and hence naked singularity — can never be reached under Hawking evaporation. We apply the scheme of Hiscock and Weems to model the evaporation of an asymptotically flat dilatonic charge black hole known as the Garfinkle-Horowitz-Strominger (GHS) black hole. We found that upholding the cosmic censorship requires us to modify the charged particle production rate, which remarkably agrees with the expression obtained independently via direct computation of charged particle production rate on curved spacetime background. This not only strengthens the case for cosmic censorship, but also provides an example in which cosmic censorship can be a useful principle to deduce other physics. We also found that the attractor behavior is not necessarily related to the specific heat, contrary to the claim by Hiscock and Weems.http://link.springer.com/article/10.1007/JHEP10(2019)129Black HolesSpacetime SingularitiesBlack Holes in String Theory |
| spellingShingle | Yen Chin Ong Yuan Yao Charged particle production rate from cosmic censorship in dilaton black hole spacetimes Journal of High Energy Physics Black Holes Spacetime Singularities Black Holes in String Theory |
| title | Charged particle production rate from cosmic censorship in dilaton black hole spacetimes |
| title_full | Charged particle production rate from cosmic censorship in dilaton black hole spacetimes |
| title_fullStr | Charged particle production rate from cosmic censorship in dilaton black hole spacetimes |
| title_full_unstemmed | Charged particle production rate from cosmic censorship in dilaton black hole spacetimes |
| title_short | Charged particle production rate from cosmic censorship in dilaton black hole spacetimes |
| title_sort | charged particle production rate from cosmic censorship in dilaton black hole spacetimes |
| topic | Black Holes Spacetime Singularities Black Holes in String Theory |
| url | http://link.springer.com/article/10.1007/JHEP10(2019)129 |
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