Thermoelectric Conduction in General Relativity: A Causal, Stable, and Well Posed Theory
arXiv:2509.23845 · doi:10.1103/b2k6-thdy
Abstract
We present a covariantly stable first-order framework for describing charge and heat transport in isotropic rigid media embedded in curved spacetime. Working in the Lorenz gauge, we show that the associated initial value problem is both causal and locally well-posed in the fully nonlinear regime. We then apply such framework to explore a range of gravitothermoelectric effects in metals undergoing relativistic acceleration. These include (1) the separation of charge through acceleration, (2) the non-uniformity of Joule heating across accelerating circuits due to time dilation, and (3) the effect of redshift on magnetic diffusion. As an astrophysical application, we derive a relativistic Thomas-Fermi equation governing the charge distribution inside a compact object, also accounting for Seebeck charge displacements driven by cooling.
6 pages and 5 figures (main text) + 6 pages and 1 figure (supplementary material), published in PRL (see https://journals.aps.org/prl/abstract/10.1103/b2k6-thdy)
References in corpus (16)
- Electrically Charged Strange Quark Stars
- Electromagnetic Field and Cylindrical Compact Objects in Modified Gravity
- When the entropy has no maximum: A new perspective on the instability of the first-order theories of dissipation
- Bounds on transport from hydrodynamic stability
- Study of Charged Compact Stars in Non-minimally Coupled Gravity
- Dissipative relativistic magnetohydrodynamics of a multicomponent mixture and its application to neutron stars
- Charge diffusion in relativistic resistive second-order dissipative magnetohydrodynamics
- Temperature in relativistic fluids
- General Relativistic Thermoelectric Effects in Superconductors
- Stability of multicomponent Israel-Stewart-Maxwell theory for charge diffusion
- Infinite Order Hydrodynamics: An Analytical Example
- Heat propagation in rotating relativistic bodies
- Thermal Conductivity and Thermal Hall Effect in Dense Electron-Ion Plasma
- Stability of electrically charged stars, regular black holes, quasiblack holes, and quasinonblack holes
- Revisiting thermoelectric effects in the crust of neutron stars
- Spontaneous charge separation in accelerating relativistic plasmas