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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...
Autores principales: | , , |
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Lenguaje: | eng |
Publicado: |
2011
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Acceso en línea: | https://dx.doi.org/10.1007/JHEP11(2011)156 http://cds.cern.ch/record/1340844 |
_version_ | 1780922121773383680 |
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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. |
id | cern-1340844 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2011 |
record_format | invenio |
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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