Holography and black holes in asymptotically flat FLRW spacetimes
In this paper, we extend the treatment of asymptotically decelerating spatially flat Friedmann-Lemaître-Robertson-Walker (FLRW) spacetimes initiated in [M. E. Rojo and T. Heckelbacher, Phys. Rev. D 103, 064009 (2021).]. We show that a certain class of those metrics is ruled by the asymptotic algebra...
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description | In this paper, we extend the treatment of asymptotically decelerating spatially flat Friedmann-Lemaître-Robertson-Walker (FLRW) spacetimes initiated in [M. E. Rojo and T. Heckelbacher, Phys. Rev. D 103, 064009 (2021).]. We show that a certain class of those metrics is ruled by the asymptotic algebra bmss, which belongs to a one-parameter family of deformations of b m s . Furthermore, we enlarge our ansatz to include Diff ( S2 ) transformations whose asymptotic algebra g b m s s is a one-parameter deformation of g b m s . Therefore, the holographic algebras bmss and gbmss in FLRW can be related to their flat counterparts through a cosmological holographic flow. Finally, we introduce a logarithmic ansatz in order to account for cosmological black holes, which does not generally satisfy the peeling property but preserves the asymptotic algebra. |
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E. Rojo and T. Heckelbacher, Phys. Rev. D 103, 064009 (2021).]. We show that a certain class of those metrics is ruled by the asymptotic algebra bmss, which belongs to a one-parameter family of deformations of b m s . Furthermore, we enlarge our ansatz to include Diff ( S2 ) transformations whose asymptotic algebra g b m s s is a one-parameter deformation of g b m s . Therefore, the holographic algebras bmss and gbmss in FLRW can be related to their flat counterparts through a cosmological holographic flow. 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Finally, we introduce a logarithmic ansatz in order to account for cosmological black holes, which does not generally satisfy the peeling property but preserves the asymptotic algebra.</description><subject>Algebra</subject><subject>Asymptotic properties</subject><subject>Black holes</subject><subject>Deceleration</subject><subject>Deformation</subject><subject>Holography</subject><subject>Parameters</subject><subject>Spacetime</subject><issn>2470-0010</issn><issn>2470-0029</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><recordid>eNo9kE1LAzEQhoMoWLS_wEvA89bJV5M9lmqtUFCK4jFks4ndmjZrshX237ul6mGY94WHGXgQuiEwIQTY3cumz2v3fT8ZyjAcmDhDI8olFAC0PP_PBC7ROOctDHEKpSRkhGbLGOJHMu2mx2Zf4yoY-4k3MbiMmz02ud-1Xewaa0LosQ-mw4vV-h3n1ljXNTuXr9GFNyG78e--Qm-Lh9f5slg9Pz7NZ6vCUim7YlqBdV6B9MoZqJyncmprKmRJeF0ryU3NlSoZcFMJQp2SMCCEW0oJZd6zK3R7utum-HVwudPbeEj74aWmggmlmBBioNiJsinmnJzXbWp2JvWagD7q0n-69LGcdLEf8ZdeRw</recordid><startdate>20210517</startdate><enddate>20210517</enddate><creator>Rojo, Martín Enríquez</creator><creator>Heckelbacher, Till</creator><general>American Physical Society</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0002-9482-0282</orcidid><orcidid>https://orcid.org/0000-0002-3145-4174</orcidid></search><sort><creationdate>20210517</creationdate><title>Holography and black holes in asymptotically flat FLRW spacetimes</title><author>Rojo, Martín Enríquez ; Heckelbacher, Till</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c277t-6b0cef807f8ea0bef276cd257914dd874ad4889304ab512e870f2714c22123ff3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Algebra</topic><topic>Asymptotic properties</topic><topic>Black holes</topic><topic>Deceleration</topic><topic>Deformation</topic><topic>Holography</topic><topic>Parameters</topic><topic>Spacetime</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Rojo, Martín Enríquez</creatorcontrib><creatorcontrib>Heckelbacher, Till</creatorcontrib><collection>CrossRef</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Physical review. 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Furthermore, we enlarge our ansatz to include Diff ( S2 ) transformations whose asymptotic algebra g b m s s is a one-parameter deformation of g b m s . Therefore, the holographic algebras bmss and gbmss in FLRW can be related to their flat counterparts through a cosmological holographic flow. Finally, we introduce a logarithmic ansatz in order to account for cosmological black holes, which does not generally satisfy the peeling property but preserves the asymptotic algebra.</abstract><cop>College Park</cop><pub>American Physical Society</pub><doi>10.1103/PhysRevD.103.104035</doi><orcidid>https://orcid.org/0000-0002-9482-0282</orcidid><orcidid>https://orcid.org/0000-0002-3145-4174</orcidid></addata></record> |
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title | Holography and black holes in asymptotically flat FLRW spacetimes |
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