Small & large argument expansion of plasma dispersion function

In summary, plasma dispersion function can be approximated using either power series expansion or asymptotic expression, depending on the argument. When you add a zeroth order magnetic field, the dispersion relation becomes more complicated.
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sreerajt
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In plasma physics we have what is known as plasma dispersion function. There are two approximation under which this function can be expanded: when the argument is less than 1, we can use power series expansion and when the argument is greater than 1 we can have asymptotic expression.

My question is, given any plasma system, how do we know that under which approximation we have to expand the plasma dispersion function? How does this change when one introduces magnetic fields into it?
 
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There is no easy answer to this. If the phenomenon you are studying can be (at least partially) described with fluid theory, it is often helpful to do the fluid theory calculation to gain physical insight to help determine what approximations might make sense in the kinetic theory calculation. Sometimes you just have to make a choice and see where the calculation leads you, then investigate the answer you get to see if it is of interest. If it isn't, then try the other approximation. But in general, if you are trying to understand a particular phenomenon or situation there is no guarantee that either of these expansions will be particularly useful and you may need to resort to numerically solving the actual dispersion relation.

When you add a zeroth order magnetic field then things get more complicated. You end up with a dielectric tensor, where each element contains an infinite series of plasma dispersion functions and modified Bessel functions (at least if you have a Gaussian zeroth-order distribution function). This tensor is then part of the dispersion relation. There are some analytical approximations that can be useful to gain insight into some important phenomena (see any textbook that covers plasma kinetic theory), but in general you numerically solve the dispersion relation. 20+ years ago there was open source code called WHAMP (Waves in Homogeneous Anisotropic Magnetized Plasmas) that you could get to do the numerics for you; I believe it came out of one of the Scandinavian groups, but I have been out of this field for a long time so cannot remember much. However, if I recall correctly WHAMP did require the user to provide a starting "guess", which you would need to get either from one of the large/small argument expansions, or (if appropriate) from a fluid theory calculation. I certainly remember doing a lot of analysis to even get WHAMP started on the dispersion surface I was interested in. Once it found part of the surface, you can then have it follow the surface into the regimes where the analytical approximations do not hold.

Please don't get discouraged if you struggle with this - kinetic theory is complicated and the messy mathematics can obscure the physics - so it is not easy to do this stuff. Even after a graduate course in kinetic theory of plasmas and a subsequent course on plasma waves (that included waves requiring kinetic theory to understand) I didn't find it easy when needing to use it during my research. In grad school it was comforting to hear well-established faculty and research scientists arguing at the blackboard about just this sort of stuff when working on research problems.Jason
 
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jasonRF said:
There is no easy answer to this.
...
In grad school it was comforting to hear well-established faculty and research scientists arguing at the blackboard about just this sort of stuff when working on research problems.Jason

Thanks you for the reply. Seems like I am not the only one who has this doubt :smile: ...
 

What is the "Small & large argument expansion" of plasma dispersion function?

The small and large argument expansions of plasma dispersion function are mathematical methods used to approximate the values of the plasma dispersion function for small and large values of the argument. This function is used in the study of plasma physics and is defined as the integral of the Maxwellian distribution function multiplied by the electric susceptibility.

Why is it important to have small and large argument expansions for the plasma dispersion function?

Having small and large argument expansions for the plasma dispersion function allows for easier and more accurate calculations in the study of plasma physics. This function is used to describe the behavior of electromagnetic waves in a plasma, and having efficient methods for approximating its values is crucial for understanding and predicting plasma behavior.

What are the limitations of the small and large argument expansions for the plasma dispersion function?

The small and large argument expansions are only accurate for specific ranges of the argument. For small arguments, the expansion is only accurate for values less than 0.1, and for large arguments, the expansion is only accurate for values greater than 10. Beyond these ranges, the approximations may become increasingly inaccurate.

How are the small and large argument expansions derived?

The small and large argument expansions are derived using asymptotic analysis, which involves finding the limiting behavior of a function as the argument approaches either 0 or infinity. This involves using mathematical techniques such as series expansions and asymptotic expansions to approximate the values of the plasma dispersion function for small and large arguments.

What are some applications of the small and large argument expansions for the plasma dispersion function?

The small and large argument expansions are used in various fields of plasma physics, such as in the study of plasma waves and instabilities, as well as in the design of plasma-based technologies such as fusion reactors and plasma thrusters. They are also used in the analysis of astrophysical plasmas, such as those found in stars and other celestial bodies.

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