2013
DOI: 10.1007/s00161-013-0291-z
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A frame-indifferent model for a thermo-elastic material beyond the three-dimensional Eulerian and Lagrangian descriptions

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Cited by 17 publications
(4 citation statements)
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“…In his relativistic thermodynamics ( [23,24]), Souriau proposed to generalize the second principle as ∇ α S α ≥ 0 and introduced the friction tensor f αβ = 1 2 (∇ α b β + ∇ β b α ) that merges the temperature gradient and the strain rate tensor, allowing to extend Fourier's conduction law and viscous flow rules to Relativity, as proposed by Vallée [25,26]. By the way, Relativity is a consistent framework for the hypoelastic, hyperelastic and dissipative constitutive laws [27][28][29].…”
Section: Relativistic Dynamics and Thermodynamicsmentioning
confidence: 99%
“…In his relativistic thermodynamics ( [23,24]), Souriau proposed to generalize the second principle as ∇ α S α ≥ 0 and introduced the friction tensor f αβ = 1 2 (∇ α b β + ∇ β b α ) that merges the temperature gradient and the strain rate tensor, allowing to extend Fourier's conduction law and viscous flow rules to Relativity, as proposed by Vallée [25,26]. By the way, Relativity is a consistent framework for the hypoelastic, hyperelastic and dissipative constitutive laws [27][28][29].…”
Section: Relativistic Dynamics and Thermodynamicsmentioning
confidence: 99%
“…The constant C 1 is homogeneous to a stress and has a weight equal to 1 (Panicaud and Rouhaud 2014). This leads to the fact that Lie derivative of C 1 does not vanish in general, but is equal to…”
Section: Incompressible Neo-hookean Hypoelastic Modelmentioning
confidence: 99%
“…Attempts to formulate Relativistic Elasticity in the General Relativity framework go back to 1916 with the pioneering work of Nordström [68], in Dutch. Since then, several authors have first aimed at proposing constitutive equations for Relativistic fluids [87,54,14,60] and, then, at modeling Relativistic continuous media, most often at the astrophysics scale [80,86,19,74,82,5,70,50,43,44,4,27,90,36,10], for instance for the modeling of the solid crust of neutron stars, but also at a local scale [57,58,59,72,72,73,63], for mechanical engineering applications.…”
Section: Introductionmentioning
confidence: 99%