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The Imperfect Fluid behind Kinetic Gravity Braiding

We present a standard hydrodynamical description for non-canonical scalar field theories with kinetic gravity braiding. In particular, this picture applies to the simplest galileons and k-essence. The fluid variables not only have a clear physical meaning but also drastically simplify the analysis o...

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Detalles Bibliográficos
Autores principales: Pujolas, Oriol, Sawicki, Ignacy, Vikman, Alexander
Lenguaje:eng
Publicado: 2011
Materias:
Acceso en línea:https://dx.doi.org/10.1007/JHEP11(2011)156
http://cds.cern.ch/record/1340844
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author Pujolas, Oriol
Sawicki, Ignacy
Vikman, Alexander
author_facet Pujolas, Oriol
Sawicki, Ignacy
Vikman, Alexander
author_sort Pujolas, Oriol
collection CERN
description We present a standard hydrodynamical description for non-canonical scalar field theories with kinetic gravity braiding. In particular, this picture applies to the simplest galileons and k-essence. The fluid variables not only have a clear physical meaning but also drastically simplify the analysis of the system. The fluid carries charges corresponding to shifts in field space. This shift-charge current contains a spatial part responsible for diffusion of the charges. Moreover, in the incompressible limit, the equation of motion becomes the standard diffusion equation. The fluid is indeed imperfect because the energy flows neither along the field gradient nor along the shift current. The fluid has zero vorticity and is not dissipative: there is no entropy production, the energy-momentum is exactly conserved, the temperature vanishes and there is no shear viscosity. Still, in an expansion around a perfect fluid one can identify terms which correct the pressure in the manner of bulk viscosity. We close by formulating the non-trivial conditions for the thermodynamic equilibrium of this imperfect fluid.
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spelling cern-13408442023-01-26T07:40:27Zdoi:10.1007/JHEP11(2011)156http://cds.cern.ch/record/1340844engPujolas, OriolSawicki, IgnacyVikman, AlexanderThe Imperfect Fluid behind Kinetic Gravity BraidingParticle Physics - TheoryWe present a standard hydrodynamical description for non-canonical scalar field theories with kinetic gravity braiding. In particular, this picture applies to the simplest galileons and k-essence. The fluid variables not only have a clear physical meaning but also drastically simplify the analysis of the system. The fluid carries charges corresponding to shifts in field space. This shift-charge current contains a spatial part responsible for diffusion of the charges. Moreover, in the incompressible limit, the equation of motion becomes the standard diffusion equation. The fluid is indeed imperfect because the energy flows neither along the field gradient nor along the shift current. The fluid has zero vorticity and is not dissipative: there is no entropy production, the energy-momentum is exactly conserved, the temperature vanishes and there is no shear viscosity. Still, in an expansion around a perfect fluid one can identify terms which correct the pressure in the manner of bulk viscosity. We close by formulating the non-trivial conditions for the thermodynamic equilibrium of this imperfect fluid.We present a standard hydrodynamical description for non-canonical scalar field theories with kinetic gravity braiding. In particular, this picture applies to the simplest galileons and k-essence. The fluid variables not only have a clear physical meaning but also drastically simplify the analysis of the system. The fluid carries charges corresponding to shifts in field space. This shift-charge current contains a spatial part responsible for diffusion of the charges. Moreover, in the incompressible limit, the equation of motion becomes the standard diffusion equation. The fluid is indeed imperfect because the energy flows neither along the field gradient nor along the shift current. The fluid has zero vorticity and is not dissipative: there is no entropy production, the energy-momentum is exactly conserved, the temperature vanishes and there is no shear viscosity. Still, in an expansion around a perfect fluid one can identify terms which correct the pressure in the manner of bulk viscosity. We close by formulating the non-trivial conditions for the thermodynamic equilibrium of this imperfect fluid.arXiv:1103.5360CERN-PH-TH-2010-210CERN-PH-TH-2010-210oai:cds.cern.ch:13408442011-03-29
spellingShingle Particle Physics - Theory
Pujolas, Oriol
Sawicki, Ignacy
Vikman, Alexander
The Imperfect Fluid behind Kinetic Gravity Braiding
title The Imperfect Fluid behind Kinetic Gravity Braiding
title_full The Imperfect Fluid behind Kinetic Gravity Braiding
title_fullStr The Imperfect Fluid behind Kinetic Gravity Braiding
title_full_unstemmed The Imperfect Fluid behind Kinetic Gravity Braiding
title_short The Imperfect Fluid behind Kinetic Gravity Braiding
title_sort imperfect fluid behind kinetic gravity braiding
topic Particle Physics - Theory
url https://dx.doi.org/10.1007/JHEP11(2011)156
http://cds.cern.ch/record/1340844
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