Physics:Relativistic heat conduction

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Short description: Model compatible with special relativity

Relativistic heat conduction refers to the modelling of heat conduction (and similar diffusion processes) in a way compatible with special relativity. In special (and general) relativity, the usual heat equation for non-relativistic heat conduction must be modified, as it leads to faster-than-light signal propagation.[1][2] Relativistic heat conduction, therefore, encompasses a set of models for heat propagation in continuous media (solids, fluids, gases) that are consistent with relativistic causality, namely the principle that an effect must be within the light-cone associated to its cause. Any reasonable relativistic model for heat conduction must also be stable, in the sense that differences in temperature propagate both slower than light and are damped over time (this stability property is intimately intertwined with relativistic causality[3]).

Parabolic model (non-relativistic)

Heat conduction in a Newtonian context is modelled by the Fourier equation,[4] namely a parabolic partial differential equation of the kind:

[math]\displaystyle{ \frac{\partial\theta}{\partial t}~=~\alpha~\nabla^2\theta , }[/math]

where θ is temperature,[5] t is time, α = k/(ρ c) is thermal diffusivity, k is thermal conductivity, ρ is density, and c is specific heat capacity. The Laplace operator,[math]\displaystyle{ \scriptstyle\nabla^2 }[/math], is defined in Cartesian coordinates as

[math]\displaystyle{ \nabla^2~=~\frac{\partial^2}{\partial x^2}~+~\frac{\partial^2}{\partial y^2}~+~\frac{\partial^2}{\partial z^2} . }[/math]

This Fourier equation can be derived by substituting Fourier’s linear approximation of the heat flux vector, q, as a function of temperature gradient,

[math]\displaystyle{ \mathbf{q}~=~-k~\nabla\theta , }[/math]

into the first law of thermodynamics

[math]\displaystyle{ \rho~c~\frac{\partial \theta}{\partial t}~+ ~\nabla \cdot \mathbf{q}~=~ 0 , }[/math]

where the del operator, ∇, is defined in 3D as

[math]\displaystyle{ \nabla ~=~\frac{\partial}{\partial x}~\mathbf{i}~+~\frac{\partial}{\partial y}~\mathbf{j}~+~\frac{\partial}{\partial z}~\mathbf{k} . }[/math]

It can be shown that this definition of the heat flux vector also satisfies the second law of thermodynamics,[6]

[math]\displaystyle{ \nabla\cdot\left(\frac{\mathbf{q}}{\theta}\right)~+~\rho~\frac{\partial s}{\partial t}~=~\sigma, }[/math]

where s is specific entropy and σ is entropy production. This mathematical model is inconsistent with special relativity: the Green function associated to the heat equation (also known as heat kernel) has support that extends outside the light-cone, leading to faster-than-light propagation of information. For example, consider a pulse of heat at the origin; then according to Fourier equation, it is felt (i.e. temperature changes) at any distant point, instantaneously. The speed of propagation of heat is faster than the speed of light in vacuum, which is inadmissible within the framework of relativity.

Hyperbolic model (relativistic)

The parabolic model for heat conduction discussed above shows that the Fourier equation (and the more general Fick's law of diffusion) is incompatible with the theory of relativity[7] for at least one reason: it admits infinite speed of propagation of the continuum field (in this case: heat, or temperature gradients). To overcome this contradiction, workers such as Carlo Cattaneo,[2] Vernotte,[8] Chester,[9] and others[10] proposed that Fourier equation should be upgraded from the parabolic to a hyperbolic form, where the n, the temperature field [math]\displaystyle{ \theta }[/math] is governed by:

[math]\displaystyle{ \frac{1}{C^2}~\frac{\partial^2\theta}{\partial t^2}~+~\frac{1}{\alpha}~\frac{\partial\theta}{\partial t}~=~\nabla^2\theta }[/math].

In this equation, C is called the speed of second sound (that is related to excitations and quasiparticles, like phonons). The equation is known as the "hyperbolic heat conduction" (HHC) equation.[11] Mathematically, the above equation is called "telegraph equation", as it is formally equivalent to the telegrapher's equations, which can be derived from Maxwell’s equations of electrodynamics.

For the HHC equation to remain compatible with the first law of thermodynamics, it is necessary to modify the definition of heat flux vector, q, to

[math]\displaystyle{ \tau_{_0}~\frac{\partial\mathbf{q}}{\partial t}~+~\mathbf{q}~=~-k~\nabla\theta, }[/math]

where [math]\displaystyle{ \scriptstyle\tau_{_0} }[/math] is a relaxation time, such that [math]\displaystyle{ \scriptstyle C^2~=~ \alpha/ \tau_{_0} . }[/math] This equation for the heat flux is often referred to as "Maxwell-Cattaneo equation". The most important implication of the hyperbolic equation is that by switching from a parabolic (dissipative) to a hyperbolic (includes a conservative term) partial differential equation, there is the possibility of phenomena such as thermal resonance[12][13][14] and thermal shock waves.[15]

Notes

  1. ↑ van Kampen, N. G. (1970-03-02). "A model for relativistic heat transport" (in en). Physica 46 (2): 315–332. doi:10.1016/0031-8914(70)90231-4. ISSN 0031-8914. Bibcode: 1970Phy....46..315V. https://dx.doi.org/10.1016/0031-8914%2870%2990231-4. 
  2. ↑ 2.0 2.1 Cattaneo, C. R. (1958). "Sur une forme de l'équation de la chaleur éliminant le paradoxe d'une propagation instantanée". Comptes Rendus 247 (4): 431. 
  3. ↑ Gavassino, L.; Antonelli, M.; Haskell, B. (2022-01-06). "Thermodynamic Stability Implies Causality". Physical Review Letters 128 (1): 010606. doi:10.1103/PhysRevLett.128.010606. PMID 35061457. Bibcode: 2022PhRvL.128a0606G. https://link.aps.org/doi/10.1103/PhysRevLett.128.010606. 
  4. ↑ Carslaw, H. S.; Jaeger, J. C. (1959). Conduction of Heat in Solids (Second ed.). Oxford: University Press. 
  5. ↑ Some authors also use T, φ,...
  6. ↑ Barletta, A.; Zanchini, E. (1997). "Hyperbolic heat conduction and local equilibrium: a second law analysis". International Journal of Heat and Mass Transfer 40 (5): 1007–1016. doi:10.1016/0017-9310(96)00211-6. 
  7. ↑ Eckert, E. R. G.; Drake, R. M. (1972). Analysis of Heat and Mass Transfer. Tokyo: McGraw-Hill, Kogakusha. 
  8. ↑ Vernotte, P. (1958). "Les paradoxes de la theorie continue de l'équation de la chaleur". Comptes Rendus 246 (22): 3154. 
  9. ↑ Chester, M. (1963). "Second sound in solids". Physical Review 131 (15): 2013–2015. doi:10.1103/PhysRev.131.2013. Bibcode: 1963PhRv..131.2013C. 
  10. ↑ Morse, P. M.; Feshbach, H. (1953). Methods of Theoretical Physics. New York: McGraw-Hill. 
  11. ↑ Joseph, D. D.; Preziosi, L. (1989). "Heat waves". Reviews of Modern Physics 61 (1): 47–71. doi:10.1103/RevModPhys.61.41. Bibcode: 1989RvMP...61...41J. 
  12. ↑ Mandrusiak, G. D. (1997). "Analysis of non-Fourier conduction waves from a reciprocating heat source". Journal of Thermophysics and Heat Transfer 11 (1): 82–89. doi:10.2514/2.6204. 
  13. ↑ Xu, M.; Wang, L. (2002). "Thermal oscillation and resonance in dual-phase-lagging heat conduction". International Journal of Heat and Mass Transfer 45 (5): 1055–1061. doi:10.1016/S0017-9310(01)00199-5. 
  14. ↑ Barletta, A.; Zanchini, E. (1996). "Hyperbolic heat conduction and thermal resonances in a cylindrical solid carrying a steady periodic electric field". International Journal of Heat and Mass Transfer 39 (6): 1307–1315. doi:10.1016/0017-9310(95)00202-2. 
  15. ↑ Tzou, D. Y. (1989). "Shock wave formation around a moving heat source in a solid with finite speed of heat propagation". International Journal of Heat and Mass Transfer 32 (10): 1979–1987. doi:10.1016/0017-9310(89)90166-X. 



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