Multifluid Modelling of Relativistic Radiation Hydrodynamics
arXiv:2007.09481 · doi:10.3390/sym12091543
Abstract
The formulation of a universal theory for bulk viscosity and heat conduction represents a theoretical challenge for our understanding of relativistic fluid dynamics. Recently, it has been shown that the multifluid variational approach championed by Carter and collaborators has the potential to be a general and natural framework to derive (hyperbolic) hydrodynamic equations for relativistic dissipative systems. Furthermore, it also allows to keep direct contact with non-equilibrium thermodynamics, providing a clear microscopic interpretation of the elements of the theory. To provide an example of its universal applicability, in this paper we derive the fundamental equations of the radiation hydrodynamics directly in the context of Carter's multifluid theory. This operation unveils a novel set of thermodynamic constraints that must be respected by any microscopic model. Then, we prove that the radiation hydrodynamics becomes a multifluid model for bulk viscosity or heat conduction in some appropriate physical limits.
arXiv comment19 pages, 0 figures, published on Symmetry
References in corpus (28)
- Relativistic Fluid Dynamics: Physics for Many Different Scales
- Semi-implicit scheme for treating radiation under M1 closure in general relativistic conservative fluid dynamics codes
- Differential rotation of relativistic superfluid in neutron stars
- Relativistic Radiation Magnetohydrodynamics in Dynamical Spacetimes: Numerical Methods and Tests
- On the Causality and Stability of the Relativistic Diffusion Equation
- Slowly Rotating General Relativistic Superfluid Neutron Stars
- The Equation of State for Cool Relativistic Two-Constituent Superfluid Dynamics
- Numerical Simulations of Optically Thick Accretion onto a Black Hole - II. Rotating Flow
- Thermal Dynamics in General Relativity
- When the entropy has no maximum: A new perspective on the instability of the first-order theories of dissipation
- Photon-conserving Comptonization in simulations of accretion disks around black holes
- Relativistic numerical models for stationary superfluid Neutron Stars
- Bulk viscosity in relativistic fluids: from thermodynamics to hydrodynamics
- Global numerical simulations of the rise of vortex-mediated pulsar glitches in full general relativity
- Thermodynamics of uncharged relativistic multifluids
- A covariant action principle for dissipative fluid dynamics: From formalism to fundamental physics
- The zeroth law of thermodynamics in special relativity
- A consistent first-order model for relativistic heat flow
- A universal formula for the relativistic correction to the mutual friction coupling time-scale in neutron stars
- Covariant Vortex In Superconducting-Superfluid-Normal Fluid Mixtures with Stiff Equation of State
- The dynamics of neutron star crusts: Lagrangian perturbation theory for a relativistic superfluid-elastic system
- Effects of general relativity on glitch amplitudes and pulsar mass upper bounds
- Relativistic formulation of the Hall-Vinen-Bekarevich-Khalatnikov superfluid hydrodynamics
- Numerical models for stationary superfluid neutron stars in general relativity with realistic equations of state
- Relativistic Kinetics of Phonon Gas in Superfluids
- The regular conducting fluid model for relativistic thermodynamics
- A transient phase in cosmological evolution : A multi-fluid approximation for a quasi-thermodynamics equilibrium
- Multi-fluid Theory and Cosmology: A Convective Variational Approach to Interacting Dark-Sector
Cited by in corpus (22)
- Can we make sense of dissipation without causality?
- Bulk viscosity in relativistic fluids: from thermodynamics to hydrodynamics
- Unified Extended Irreversible Thermodynamics and the stability of relativistic theories for dissipation
- Stability and causality of Carter's multifluid theory
- Symmetric-hyperbolic quasi-hydrodynamics
- Simulating bulk viscosity in neutron stars. II. Evolution in spherical symmetry
- Relativistic Liquids: GENERIC or EIT?
- Is Relativistic Hydrodynamics always Symmetric-Hyperbolic in the Linear Regime?
- Universality Classes of Relativistic Fluid Dynamics: Foundations
- Superfluid dynamics in neutron star crusts: the Iordanskii force and chemical gauge covariance
- Global high-order numerical schemes for the time evolution of the general relativistic radiation magneto-hydrodynamics equations
- Universality Classes of Relativistic Fluid Dynamics: Applications
- Infinite Order Hydrodynamics: An Analytical Example
- Mapping GENERIC hydrodynamics into Carter's multifluid theory
- Dispersion relations of relativistic radiation hydrodynamics
- Relativistic heat conduction in the large-flux regime
- Simulating bulk viscosity in neutron stars. I. Formalism
- Thermodynamic stability implies causality
- How Lorentz boosts reshape relaxation spectra
- Non-Newtonian corrections to radiative viscosity: Israel-Stewart theory as a viscosity limiter
- A multifluid perspective on multimessenger modelling
- Extending Israel and Stewart hydrodynamics to relativistic superfluids via Carter's multifluid approach