Relativistic hydrodynamics: gradient expansion

In summary, the gradient expansion of the collision term around local thermal equilibrium is used to derive the Boltzmann transport equation. This equation is applicable to particles in a relativistic context, and requires second order in gradients.
  • #1
klabautermann
34
0
Hi everyone,
I'm interested in relativistic anisotropic hydrodynamics and often a "gradient Expansion" is mentioned in articles, but not how this works exactly. I gathered that this is some kind of expansion of the energy-momentum tensor. Can someone explain to me how this expansion is set up, or better yet point me to some literature or articles?

Thanks a lot!
 
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  • #2
The gradient expansion usually refers to the derivation of the Boltzmann transport equation from off-equilibrium quantum-many-body theory.

Now having the Boltzmann equation to get hydrodynamics you start from an expansion of the collision term around local thermal equilibrium and do another gradient expansion. For the relativistic case you must go to at least the 2nd order in gradients since Navier-Stokes is acausal in the relativistic case. In the most simple version this leads to the Israel-Stewart hydro equation. For a systematic way in terms of moment expansions, see the works by Denicol et al, e.g.,

https://arxiv.org/abs/1004.5013https://arxiv.org/abs/1202.4551https://arxiv.org/abs/1206.1554
Maybe I can give more specific references, if you tell me, which paper(s) you are referring to.
 
  • #3
Good evening,

first of all, thanks for your reply and the references. Actually I need to understand this https://arxiv.org/abs/1712.03282 . Since I had virtually no exposure to hydrodynamics so far, I am trying to get a general picture about the subject, so I am working through this https://arxiv.org/abs/0902.3663 right now. For my purposes, its probably not all that necessary to know, but, I have to say, I am getting more and more intrigued by the subject. So I just wanted know.

At first sight the papers you posted seem to be exactly what I was looking for, thanks again!
 
  • #5
Thanks for the tip, I'm certainly going to look into it!
 

FAQ: Relativistic hydrodynamics: gradient expansion

What is relativistic hydrodynamics?

Relativistic hydrodynamics is a branch of physics that studies the behavior of fluids (such as gases and liquids) at high speeds and in strong gravitational fields, taking into account the effects of special relativity. It is used to describe the dynamics of systems such as astrophysical jets, supernova explosions, and the early universe.

What is the gradient expansion in relativistic hydrodynamics?

The gradient expansion is a mathematical technique used in relativistic hydrodynamics to expand the equations of motion in a series of terms based on the spatial derivatives of the fluid variables. It allows for a systematic treatment of the effects of gradients (or spatial variations) in the fluid, which are important at high speeds and in strong gravitational fields.

What are the assumptions made in the gradient expansion method?

The gradient expansion method assumes that the fluid is in local thermal equilibrium, meaning that the fluid properties (such as temperature and pressure) vary smoothly in space. It also assumes that the fluid is isotropic, meaning that its properties are the same in all directions. Additionally, it assumes that the fluid is described by a perfect fluid model, where there is no viscosity or heat conduction.

What are the limitations of the gradient expansion method?

The gradient expansion method is limited to systems that are close to thermal equilibrium, as it assumes that the fluid properties vary smoothly in space. It also cannot account for non-ideal effects such as viscosity and heat conduction. Additionally, it may not be accurate for systems with large gradients or strong shocks.

How is the gradient expansion method used in practical applications?

The gradient expansion method is used in numerical simulations of relativistic hydrodynamics, where the equations of motion are solved on a grid using finite difference or finite volume methods. It is also used in analytical calculations to study the behavior of fluids in specific scenarios, such as the expansion of the early universe or the formation of astrophysical jets.

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