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6. Renormalized Perturbation Theory

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<strong>6.</strong> <strong>Renormalized</strong> <strong>Perturbation</strong> <strong>Theory</strong><br />

<strong>6.</strong>1. <strong>Perturbation</strong> expansion of the Navier-Stokes equation<br />

Kraichnan (1959): direct-interaction approximation<br />

Wyld (1961): partial summation for a simplified scalar model<br />

Lee (1965): partial summation for Navier-Stokes and MHD<br />

<strong>6.</strong>1.1. The zero-order isotropic propagators<br />

What is a plasma ?<br />

Kinetic description<br />

Fluid description<br />

Navier-Stokes turbulence<br />

Closure Theories<br />

<strong>Renormalized</strong> . . .<br />

λ: bookkeeping parameter, D αβ : projector on divergence free part<br />

zero-order Green tensor:<br />

Renormalization Group<br />

Passive Scalar<br />

Dynamic Functional<br />

Magnetic Reconnection<br />

Mean Field . . .<br />

with<br />

Magneto-Rotational . . .<br />

Interstellar Medium (ISM)<br />

so that<br />

Turbulence in Fusion<br />

Literature


zero-order velocity:<br />

What is a plasma ?<br />

Kinetic description<br />

Fluid description<br />

Fourier transform in time:<br />

Navier-Stokes turbulence<br />

Closure Theories<br />

<strong>Renormalized</strong> . . .<br />

=⇒ Navier-Stokes<br />

Renormalization Group<br />

Passive Scalar<br />

Dynamic Functional<br />

Magnetic Reconnection<br />

zero-order propagator is given by<br />

Mean Field . . .<br />

Magneto-Rotational . . .<br />

Interstellar Medium (ISM)<br />

Turbulence in Fusion<br />

Literature


<strong>6.</strong>1.2. The primitive perturbation expansion<br />

Stirring force<br />

What is a plasma ?<br />

after Fourier-trafo<br />

Kinetic description<br />

Fluid description<br />

Navier-Stokes turbulence<br />

zero-order velocity field after in Fourier-space<br />

Closure Theories<br />

<strong>Renormalized</strong> . . .<br />

which is the zero-order term in expansion<br />

Renormalization Group<br />

Passive Scalar<br />

Dynamic Functional<br />

correlation Q αβ (k; ω, ω ′ )<br />

Magnetic Reconnection<br />

Mean Field . . .<br />

Magneto-Rotational . . .<br />

Interstellar Medium (ISM)<br />

Turbulence in Fusion<br />

Literature


homogeneous isotropic turbulence<br />

and<br />

<strong>Perturbation</strong> expansion for Q<br />

What is a plasma ?<br />

Kinetic description<br />

Fluid description<br />

Navier-Stokes turbulence<br />

Closure Theories<br />

<strong>Renormalized</strong> . . .<br />

Renormalization Group<br />

Passive Scalar<br />

Dynamic Functional<br />

Magnetic Reconnection<br />

Mean Field . . .<br />

Take Fourier transformed NS-equation, invert linear part and substitute<br />

forcing by u (0)<br />

Magneto-Rotational . . .<br />

Interstellar Medium (ISM)<br />

Turbulence in Fusion<br />

Literature


Now substitute perturbation expansion for u<br />

What is a plasma ?<br />

Kinetic description<br />

Fluid description<br />

Navier-Stokes turbulence<br />

Closure Theories<br />

<strong>Renormalized</strong> . . .<br />

equating coefficients:<br />

Renormalization Group<br />

Passive Scalar<br />

Dynamic Functional<br />

Magnetic Reconnection<br />

Mean Field . . .<br />

u (2) can be expressed by u (0)<br />

Magneto-Rotational . . .<br />

Interstellar Medium (ISM)<br />

Turbulence in Fusion<br />

Literature


stirring Gaussian =⇒ u (0) Gaussian<br />

=⇒ 〈 u (0) u (0) u (0) u (0)〉 can be factored as in Quasi-Normal approximation<br />

second-order correlation tensor:<br />

What is a plasma ?<br />

Kinetic description<br />

Fluid description<br />

Navier-Stokes turbulence<br />

Closure Theories<br />

<strong>Renormalized</strong> . . .<br />

Renormalization Group<br />

Passive Scalar<br />

Dynamic Functional<br />

Magnetic Reconnection<br />

Mean Field . . .<br />

Magneto-Rotational . . .<br />

Interstellar Medium (ISM)<br />

Turbulence in Fusion<br />

Literature


<strong>6.</strong>1.3. Graphical representation of the perturbation series<br />

all orders can be expressed by zero-order terms, but divergent series<br />

three main constituents: u (0) , G 0 and M<br />

What is a plasma ?<br />

Kinetic description<br />

Fluid description<br />

Navier-Stokes turbulence<br />

Closure Theories<br />

zero-order:<br />

<strong>Renormalized</strong> . . .<br />

Renormalization Group<br />

Passive Scalar<br />

first-order: wavenumber conservation<br />

Dynamic Functional<br />

Magnetic Reconnection<br />

Mean Field . . .<br />

Magneto-Rotational . . .<br />

Interstellar Medium (ISM)<br />

Turbulence in Fusion<br />

Literature


second-order: two M factors:<br />

What is a plasma ?<br />

Kinetic description<br />

Fluid description<br />

Navier-Stokes turbulence<br />

Closure Theories<br />

<strong>Renormalized</strong> . . .<br />

Renormalization Group<br />

third-order: three M factors:<br />

Passive Scalar<br />

Dynamic Functional<br />

Magnetic Reconnection<br />

Mean Field . . .<br />

Magneto-Rotational . . .<br />

Interstellar Medium (ISM)<br />

Turbulence in Fusion<br />

Literature


graphical expansion for correlation tensor<br />

zero-order:<br />

What is a plasma ?<br />

Kinetic description<br />

second-order:<br />

Fluid description<br />

Navier-Stokes turbulence<br />

Closure Theories<br />

<strong>Renormalized</strong> . . .<br />

Renormalization Group<br />

Passive Scalar<br />

Dynamic Functional<br />

Magnetic Reconnection<br />

this is middle second-order term:<br />

Mean Field . . .<br />

Magneto-Rotational . . .<br />

Interstellar Medium (ISM)<br />

Turbulence in Fusion<br />

Literature


What is a plasma ?<br />

Kinetic description<br />

Fluid description<br />

this is the last second-order term:<br />

Navier-Stokes turbulence<br />

Closure Theories<br />

<strong>Renormalized</strong> . . .<br />

Renormalization Group<br />

Passive Scalar<br />

Dynamic Functional<br />

Magnetic Reconnection<br />

Mean Field . . .<br />

The third is a mirrow image of this one.<br />

Magneto-Rotational . . .<br />

Interstellar Medium (ISM)<br />

Turbulence in Fusion<br />

Literature


fourth-order showing four of the 29 fourth-order diagrams:<br />

What is a plasma ?<br />

Kinetic description<br />

Fluid description<br />

Navier-Stokes turbulence<br />

Closure Theories<br />

<strong>Renormalized</strong> . . .<br />

Renormalization Group<br />

Now resummation (renormalisation): new diagram elements<br />

Passive Scalar<br />

Dynamic Functional<br />

Magnetic Reconnection<br />

Mean Field . . .<br />

Magneto-Rotational . . .<br />

Write correlation tensor as:<br />

Interstellar Medium (ISM)<br />

Turbulence in Fusion<br />

Literature


<strong>6.</strong>1.4. Class A diagram: the renormalized propagator<br />

Wyld (1961):<br />

Class A diagrams are those diagrams which can be split into<br />

two pieces by cutting a single Q 0 line.<br />

zero-order: Q 0 can be expressed in terms of two zero-order propagators<br />

acting on the spectrum of the stirring forces w(k; ω, ω ′ )<br />

This looks graphically like<br />

What is a plasma ?<br />

Kinetic description<br />

Fluid description<br />

Navier-Stokes turbulence<br />

Closure Theories<br />

<strong>Renormalized</strong> . . .<br />

Now second-order:<br />

Renormalization Group<br />

Passive Scalar<br />

Dynamic Functional<br />

Magnetic Reconnection<br />

Mean Field . . .<br />

Magneto-Rotational . . .<br />

Let’s summarize: at zero order, we have w with a G 0 on each side. At<br />

second order, w has a G 0 on one side and a diagram which connects like a<br />

G 0 on the other. This holds for all orders. Thus we have a generalization<br />

Interstellar Medium (ISM)<br />

Turbulence in Fusion<br />

Literature


of<br />

which reads<br />

where G(k, ω) is the renormalized propagator.<br />

Graphically, this corresponds to<br />

What is a plasma ?<br />

Kinetic description<br />

Fluid description<br />

Navier-Stokes turbulence<br />

Closure Theories<br />

<strong>Renormalized</strong> . . .<br />

Renormalization Group<br />

Passive Scalar<br />

Dynamic Functional<br />

Magnetic Reconnection<br />

Mean Field . . .<br />

Magneto-Rotational . . .<br />

Interstellar Medium (ISM)<br />

Turbulence in Fusion<br />

Literature


<strong>6.</strong>1.5. Class B diagrams: renormalized perturbation series<br />

Class B diagrams can’t be split into two by cutting a single Q 0 line.<br />

In the class A diagrams, certain diagram parts were propagator like, that is,<br />

they connected like G 0 : renormalize G 0 by adding up all diagrams which<br />

connect like G 0 .<br />

Renormalize vertex: add up all diagrams which connect like a vertex<br />

Example: consider fourth-order diagram<br />

What is a plasma ?<br />

Kinetic description<br />

Fluid description<br />

Navier-Stokes turbulence<br />

Closure Theories<br />

<strong>Renormalized</strong> . . .<br />

Renormalization Group<br />

Passive Scalar<br />

The part<br />

Dynamic Functional<br />

Magnetic Reconnection<br />

Mean Field . . .<br />

Magneto-Rotational . . .<br />

connects like a point vertex =⇒ renormalized vertex<br />

Interstellar Medium (ISM)<br />

Turbulence in Fusion<br />

Literature


eplace vertex by renormalized vertex:<br />

What is a plasma ?<br />

Kinetic description<br />

Fluid description<br />

Navier-Stokes turbulence<br />

Closure Theories<br />

Therefore the key to the class B diagrams is as follows:<br />

1. Find those diagrams which cannot be reduced to a lower order by<br />

replacing diagram parts.<br />

2. Call these the irreducible diagrams.<br />

3. Replace all elements in the irreducible diagrams by their renormalized<br />

forms.<br />

4. Write down all these modified diagrams in order, thus generating a<br />

renormalized perturbation expansion.<br />

<strong>Renormalized</strong> . . .<br />

Renormalization Group<br />

Passive Scalar<br />

Dynamic Functional<br />

Magnetic Reconnection<br />

Mean Field . . .<br />

Magneto-Rotational . . .<br />

Interstellar Medium (ISM)<br />

Turbulence in Fusion<br />

Literature


Result for Q(k; ω, ω ′ )<br />

What is a plasma ?<br />

Kinetic description<br />

Fluid description<br />

Navier-Stokes turbulence<br />

Closure Theories<br />

<strong>Renormalized</strong> . . .<br />

Renormalization Group<br />

This is an integral equation for Q(k; ω, ω)<br />

Passive Scalar<br />

Dynamic Functional<br />

Combine vertex and propagator expansions:<br />

Integral equation for the renormalized vertex<br />

Magnetic Reconnection<br />

Mean Field . . .<br />

Magneto-Rotational . . .<br />

Interstellar Medium (ISM)<br />

Turbulence in Fusion<br />

Literature


Integral equation for the renormalized propagator G(k, ω)<br />

What is a plasma ?<br />

Kinetic description<br />

Fluid description<br />

Navier-Stokes turbulence<br />

Closure Theories<br />

<strong>Renormalized</strong> . . .<br />

Pecularity of this diagram:<br />

unrenormalized propagator emerging from the left !!!<br />

Reason for this: symbolic form of Navier-Stokes<br />

L 0 u(k) = λM(k)u(j)u(k − j) , L 0 = ∂ t + νk 2<br />

and renormalize r.h.s., then invert L 0 which results in G 0<br />

Renormalization Group<br />

Passive Scalar<br />

Dynamic Functional<br />

Magnetic Reconnection<br />

Mean Field . . .<br />

Magneto-Rotational . . .<br />

Interstellar Medium (ISM)<br />

Turbulence in Fusion<br />

Literature


<strong>6.</strong>1.<strong>6.</strong> Second-order closures<br />

What have we done:<br />

We replaced a wildly divergent series with one of unknown properties !<br />

We have hope that it might be assymptotic, but we simple don’t know !<br />

Well known examples recovered from this Wyld (1961) formulation:<br />

Example 1:<br />

correlation tensor: truncate at second order (in number vertices)<br />

vertex: truncate at first order (unrenormalized vertex)<br />

propagator: truncate at zero order (unrenormalized propagator)<br />

This is Chandrasekhar’s theory (1955) which is the two-time analog of<br />

quasi-normality.<br />

What is a plasma ?<br />

Kinetic description<br />

Fluid description<br />

Navier-Stokes turbulence<br />

Closure Theories<br />

<strong>Renormalized</strong> . . .<br />

Renormalization Group<br />

Passive Scalar<br />

Dynamic Functional<br />

Magnetic Reconnection<br />

Mean Field . . .<br />

Magneto-Rotational . . .<br />

Interstellar Medium (ISM)<br />

Turbulence in Fusion<br />

Literature


Example 2:<br />

correlation tensor:<br />

vertex:<br />

propagator:<br />

truncate at second order<br />

truncate at first order<br />

truncate at second order<br />

This is the pioneering direct-interaction approximation (DIA) by Kraichnan<br />

(1959): second-order closure with line and with no vertex renormalization.<br />

What is a plasma ?<br />

Kinetic description<br />

Fluid description<br />

Navier-Stokes turbulence<br />

Closure Theories<br />

<strong>Renormalized</strong> . . .<br />

Renormalization Group<br />

Passive Scalar<br />

Dynamic Functional<br />

Magnetic Reconnection<br />

Mean Field . . .<br />

Magneto-Rotational . . .<br />

Interstellar Medium (ISM)<br />

Turbulence in Fusion<br />

Literature

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