Hairy black holes in a box
A bstract We do a systematic study of the phases of gravity coupled to an electromagnetic field and charged scalar in flat space, with box boundary conditions. The scalar-less box has previously been investigated by Braden, Brown, Whiting and York (and others) before AdS/CFT and we elaborate and ext...
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| Veröffentlicht in: | The journal of high energy physics 2016-11, Vol.2016 (11), p.1-24, Article 41 |
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| container_title | The journal of high energy physics |
| container_volume | 2016 |
| creator | Basu, Pallab Krishnan, Chethan Subramanian, P. N. Bala |
| description | A
bstract
We do a systematic study of the phases of gravity coupled to an electromagnetic field and charged scalar in flat space, with box boundary conditions. The scalar-less box has previously been investigated by Braden, Brown, Whiting and York (and others) before AdS/CFT and we elaborate and extend their results in a language more familiar from holography. The phase diagram of the system is analogous to that of AdS black holes, but we emphasize the differences and explain their origin. Once the scalar is added, we show that the system admits both boson stars as well as hairy black holes as solutions, providing yet another way to evade flat space no-hair theorems. Furthermore both these solutions can exist as stable phases in regions of the phase diagram. The final picture of the phases that emerges is strikingly similar to that found recently for holographic superconductors in global AdS,
arXiv:1602.07211
. Our construction lays bare certain previously unnoticed subtleties associated to the definition quasi-local charges for gravitating scalar fields in finite regions. |
| doi_str_mv | 10.1007/JHEP11(2016)041 |
| format | Article |
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bstract
We do a systematic study of the phases of gravity coupled to an electromagnetic field and charged scalar in flat space, with box boundary conditions. The scalar-less box has previously been investigated by Braden, Brown, Whiting and York (and others) before AdS/CFT and we elaborate and extend their results in a language more familiar from holography. The phase diagram of the system is analogous to that of AdS black holes, but we emphasize the differences and explain their origin. Once the scalar is added, we show that the system admits both boson stars as well as hairy black holes as solutions, providing yet another way to evade flat space no-hair theorems. Furthermore both these solutions can exist as stable phases in regions of the phase diagram. The final picture of the phases that emerges is strikingly similar to that found recently for holographic superconductors in global AdS,
arXiv:1602.07211
. Our construction lays bare certain previously unnoticed subtleties associated to the definition quasi-local charges for gravitating scalar fields in finite regions.</description><identifier>ISSN: 1029-8479</identifier><identifier>EISSN: 1029-8479</identifier><identifier>DOI: 10.1007/JHEP11(2016)041</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer Berlin Heidelberg</publisher><subject>Black holes ; Black holes (astronomy) ; Classical and Quantum Gravitation ; Electromagnetic fields ; Elementary Particles ; Gravitation ; High energy physics ; Mathematical analysis ; Phase diagrams ; Phases ; Physics ; Physics and Astronomy ; Quantum Field Theories ; Quantum Field Theory ; Quantum Physics ; Regular Article - Theoretical Physics ; Relativity Theory ; Scalars ; String Theory</subject><ispartof>The journal of high energy physics, 2016-11, Vol.2016 (11), p.1-24, Article 41</ispartof><rights>The Author(s) 2016</rights><rights>SISSA, Trieste, Italy 2016</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c384t-a41663d9574c37fdc4539fe1db41215572df408ef225260b2e1bbf40c242ad2f3</citedby><cites>FETCH-LOGICAL-c384t-a41663d9574c37fdc4539fe1db41215572df408ef225260b2e1bbf40c242ad2f3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/JHEP11(2016)041$$EPDF$$P50$$Gspringer$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://doi.org/10.1007/JHEP11(2016)041$$EHTML$$P50$$Gspringer$$Hfree_for_read</linktohtml><link.rule.ids>314,777,781,861,27905,27906,41101,42170,51557</link.rule.ids></links><search><creatorcontrib>Basu, Pallab</creatorcontrib><creatorcontrib>Krishnan, Chethan</creatorcontrib><creatorcontrib>Subramanian, P. N. Bala</creatorcontrib><title>Hairy black holes in a box</title><title>The journal of high energy physics</title><addtitle>J. High Energ. Phys</addtitle><description>A
bstract
We do a systematic study of the phases of gravity coupled to an electromagnetic field and charged scalar in flat space, with box boundary conditions. The scalar-less box has previously been investigated by Braden, Brown, Whiting and York (and others) before AdS/CFT and we elaborate and extend their results in a language more familiar from holography. The phase diagram of the system is analogous to that of AdS black holes, but we emphasize the differences and explain their origin. Once the scalar is added, we show that the system admits both boson stars as well as hairy black holes as solutions, providing yet another way to evade flat space no-hair theorems. Furthermore both these solutions can exist as stable phases in regions of the phase diagram. The final picture of the phases that emerges is strikingly similar to that found recently for holographic superconductors in global AdS,
arXiv:1602.07211
. Our construction lays bare certain previously unnoticed subtleties associated to the definition quasi-local charges for gravitating scalar fields in finite regions.</description><subject>Black holes</subject><subject>Black holes (astronomy)</subject><subject>Classical and Quantum Gravitation</subject><subject>Electromagnetic fields</subject><subject>Elementary Particles</subject><subject>Gravitation</subject><subject>High energy physics</subject><subject>Mathematical analysis</subject><subject>Phase diagrams</subject><subject>Phases</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quantum Field Theories</subject><subject>Quantum Field Theory</subject><subject>Quantum Physics</subject><subject>Regular Article - Theoretical Physics</subject><subject>Relativity Theory</subject><subject>Scalars</subject><subject>String Theory</subject><issn>1029-8479</issn><issn>1029-8479</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><sourceid>C6C</sourceid><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNp1kMFLwzAUh4MoOKdnwVPByzzUvZcmbXOUMa0y0IOeQ5om2tm1M1nB_fem1MMQPL3H4_v9eHyEXCLcIkA2fyqWL4gzCpjeAMMjMkGgIs5ZJo4P9lNy5v0aADkKmJCrQtVuH5WN0p_RR9cYH9VtpKKy-z4nJ1Y13lz8zil5u1--Lop49fzwuLhbxTrJ2S5WDNM0qQTPmE4yW2nGE2ENViVDipxntLIMcmMp5TSFkhosy3DRlFFVUZtMyWzs3bruqzd-Jze116ZpVGu63kvM06FSiDSg13_Qdde7NnwXqCTjgeMsUPOR0q7z3hkrt67eKLeXCHJwJUdXcnAlg6uQgDHhA9m-G3fQ-0_kB5J1Z4M</recordid><startdate>20161101</startdate><enddate>20161101</enddate><creator>Basu, Pallab</creator><creator>Krishnan, Chethan</creator><creator>Subramanian, P. 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Bala</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c384t-a41663d9574c37fdc4539fe1db41215572df408ef225260b2e1bbf40c242ad2f3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>Black holes</topic><topic>Black holes (astronomy)</topic><topic>Classical and Quantum Gravitation</topic><topic>Electromagnetic fields</topic><topic>Elementary Particles</topic><topic>Gravitation</topic><topic>High energy physics</topic><topic>Mathematical analysis</topic><topic>Phase diagrams</topic><topic>Phases</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Quantum Field Theories</topic><topic>Quantum Field Theory</topic><topic>Quantum Physics</topic><topic>Regular Article - Theoretical Physics</topic><topic>Relativity Theory</topic><topic>Scalars</topic><topic>String Theory</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Basu, Pallab</creatorcontrib><creatorcontrib>Krishnan, Chethan</creatorcontrib><creatorcontrib>Subramanian, P. 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bstract
We do a systematic study of the phases of gravity coupled to an electromagnetic field and charged scalar in flat space, with box boundary conditions. The scalar-less box has previously been investigated by Braden, Brown, Whiting and York (and others) before AdS/CFT and we elaborate and extend their results in a language more familiar from holography. The phase diagram of the system is analogous to that of AdS black holes, but we emphasize the differences and explain their origin. Once the scalar is added, we show that the system admits both boson stars as well as hairy black holes as solutions, providing yet another way to evade flat space no-hair theorems. Furthermore both these solutions can exist as stable phases in regions of the phase diagram. The final picture of the phases that emerges is strikingly similar to that found recently for holographic superconductors in global AdS,
arXiv:1602.07211
. Our construction lays bare certain previously unnoticed subtleties associated to the definition quasi-local charges for gravitating scalar fields in finite regions.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer Berlin Heidelberg</pub><doi>10.1007/JHEP11(2016)041</doi><tpages>24</tpages><oa>free_for_read</oa></addata></record> |
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| ispartof | The journal of high energy physics, 2016-11, Vol.2016 (11), p.1-24, Article 41 |
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| language | eng |
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| source | DOAJ Directory of Open Access Journals; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; Alma/SFX Local Collection; Springer Nature OA/Free Journals |
| subjects | Black holes Black holes (astronomy) Classical and Quantum Gravitation Electromagnetic fields Elementary Particles Gravitation High energy physics Mathematical analysis Phase diagrams Phases Physics Physics and Astronomy Quantum Field Theories Quantum Field Theory Quantum Physics Regular Article - Theoretical Physics Relativity Theory Scalars String Theory |
| title | Hairy black holes in a box |
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