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Snapping swallowtails in accelerating black hole thermodynamics
The thermodynamic behaviour of a charged and accelerating AdS black hole is studied in the context of extended phase space with variable cosmological constant. When compared to the charged AdS black hole without acceleration, a remarkable new feature of 'snapping swallowtails' appears. Nam...
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Published in: | Classical and quantum gravity 2019-05, Vol.36 (10), p.104001 |
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container_title | Classical and quantum gravity |
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creator | Abbasvandi, Niloofar Cong, Wan Kubiz ák, David Mann, Robert B |
description | The thermodynamic behaviour of a charged and accelerating AdS black hole is studied in the context of extended phase space with variable cosmological constant. When compared to the charged AdS black hole without acceleration, a remarkable new feature of 'snapping swallowtails' appears. Namely, for any black hole with charge Q and any string tension causing the acceleration of the black hole, there exists a transition pressure at which the standard swallowtail 'snaps', causing the branch of low temperature black holes to completely disappear, leading to a pressure induced zeroth order phase transition between small and large black holes. For intermediate values of the string tension, we also observe a reentrant phase transition, as the small black hole changes to a large one and then back to small, as the pressure decreases, crossing the coexistence line of the two phases several times. We also find a new class of 'mini-entropic' black holes, whose isoperimetric ratio becomes unbounded in a certain region of parameter space. |
doi_str_mv | 10.1088/1361-6382/ab129f |
format | article |
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When compared to the charged AdS black hole without acceleration, a remarkable new feature of 'snapping swallowtails' appears. Namely, for any black hole with charge Q and any string tension causing the acceleration of the black hole, there exists a transition pressure at which the standard swallowtail 'snaps', causing the branch of low temperature black holes to completely disappear, leading to a pressure induced zeroth order phase transition between small and large black holes. For intermediate values of the string tension, we also observe a reentrant phase transition, as the small black hole changes to a large one and then back to small, as the pressure decreases, crossing the coexistence line of the two phases several times. 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For intermediate values of the string tension, we also observe a reentrant phase transition, as the small black hole changes to a large one and then back to small, as the pressure decreases, crossing the coexistence line of the two phases several times. We also find a new class of 'mini-entropic' black holes, whose isoperimetric ratio becomes unbounded in a certain region of parameter space.</abstract><pub>IOP Publishing</pub><doi>10.1088/1361-6382/ab129f</doi><tpages>17</tpages><orcidid>https://orcid.org/0000-0002-4883-0834</orcidid><orcidid>https://orcid.org/0000-0002-5859-2227</orcidid></addata></record> |
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subjects | black holes holography PV criticality thermodynamics |
title | Snapping swallowtails in accelerating black hole thermodynamics |
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