Signatures of chaos and non-integrability in two-dimensional gravity with dynamical boundary

We propose a model of two-dimensional dilaton gravity with a boundary. In the bulk our model coincides with the classically integrable CGHS model; the dynamical boundary cuts of the CGHS strong-coupling region. As a result, classical dynamics in our model reminds that in the spherically-symmetric gr...

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Main Author: Fitkevich Maxim
Format: Article
Language:English
Published: EDP Sciences 2016-01-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/201612505004
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author Fitkevich Maxim
author_facet Fitkevich Maxim
author_sort Fitkevich Maxim
collection DOAJ
description We propose a model of two-dimensional dilaton gravity with a boundary. In the bulk our model coincides with the classically integrable CGHS model; the dynamical boundary cuts of the CGHS strong-coupling region. As a result, classical dynamics in our model reminds that in the spherically-symmetric gravity: wave packets of matter fields either reflect from the boundary or form black holes. We find large integrable sector of multisoliton solutions in this model. At the same time, we argue that the model is globally non-integrable because solutions at the verge of black hole formation display chaotic properties.
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spelling doaj.art-266e4de7fc1f4d06940579b370876a772022-12-21T22:25:06ZengEDP SciencesEPJ Web of Conferences2100-014X2016-01-011250500410.1051/epjconf/201612505004epjconf_quark2016_05004Signatures of chaos and non-integrability in two-dimensional gravity with dynamical boundaryFitkevich Maxim0Institute for Nuclear Research of the Russian Academy of SciencesWe propose a model of two-dimensional dilaton gravity with a boundary. In the bulk our model coincides with the classically integrable CGHS model; the dynamical boundary cuts of the CGHS strong-coupling region. As a result, classical dynamics in our model reminds that in the spherically-symmetric gravity: wave packets of matter fields either reflect from the boundary or form black holes. We find large integrable sector of multisoliton solutions in this model. At the same time, we argue that the model is globally non-integrable because solutions at the verge of black hole formation display chaotic properties.http://dx.doi.org/10.1051/epjconf/201612505004
spellingShingle Fitkevich Maxim
Signatures of chaos and non-integrability in two-dimensional gravity with dynamical boundary
EPJ Web of Conferences
title Signatures of chaos and non-integrability in two-dimensional gravity with dynamical boundary
title_full Signatures of chaos and non-integrability in two-dimensional gravity with dynamical boundary
title_fullStr Signatures of chaos and non-integrability in two-dimensional gravity with dynamical boundary
title_full_unstemmed Signatures of chaos and non-integrability in two-dimensional gravity with dynamical boundary
title_short Signatures of chaos and non-integrability in two-dimensional gravity with dynamical boundary
title_sort signatures of chaos and non integrability in two dimensional gravity with dynamical boundary
url http://dx.doi.org/10.1051/epjconf/201612505004
work_keys_str_mv AT fitkevichmaxim signaturesofchaosandnonintegrabilityintwodimensionalgravitywithdynamicalboundary