6. renormalized perturbation theory - ruhr-uni-bochum.de
TRANSCRIPT
What is a plasma ?
Kinetic description
Fluid description
Navier-Stokes turbulence
Closure Theories
Renormalized . . .
Renormalization Group
Passive Scalar
Dynamic Functional
Magnetic Reconnection
Mean Field . . .
Magneto-Rotational . . .
Interstellar Medium (ISM)
Turbulence in Fusion
Literature
6. Renormalized Perturbation Theory
6.1. Perturbation expansion of the Navier-Stokes equation
Kraichnan (1959): direct-interaction approximationWyld (1961): partial summation for a simplified scalar modelLee (1965): partial summation for Navier-Stokes and MHD
6.1.1. The zero-order isotropic propagators
λ: bookkeeping parameter, Dαβ: projector on divergence free part
zero-order Green tensor:
with
so that
What is a plasma ?
Kinetic description
Fluid description
Navier-Stokes turbulence
Closure Theories
Renormalized . . .
Renormalization Group
Passive Scalar
Dynamic Functional
Magnetic Reconnection
Mean Field . . .
Magneto-Rotational . . .
Interstellar Medium (ISM)
Turbulence in Fusion
Literature
zero-order velocity:
Fourier transform in time:
=⇒ Navier-Stokes
zero-order propagator is given by
What is a plasma ?
Kinetic description
Fluid description
Navier-Stokes turbulence
Closure Theories
Renormalized . . .
Renormalization Group
Passive Scalar
Dynamic Functional
Magnetic Reconnection
Mean Field . . .
Magneto-Rotational . . .
Interstellar Medium (ISM)
Turbulence in Fusion
Literature
6.1.2. The primitive perturbation expansion
Stirring force
after Fourier-trafo
zero-order velocity field after in Fourier-space
which is the zero-order term in expansion
correlation Qαβ(k;ω, ω′)
What is a plasma ?
Kinetic description
Fluid description
Navier-Stokes turbulence
Closure Theories
Renormalized . . .
Renormalization Group
Passive Scalar
Dynamic Functional
Magnetic Reconnection
Mean Field . . .
Magneto-Rotational . . .
Interstellar Medium (ISM)
Turbulence in Fusion
Literature
homogeneous isotropic turbulence
and
Perturbation expansion for Q
Take Fourier transformed NS-equation, invert linear part and substituteforcing by u(0)
What is a plasma ?
Kinetic description
Fluid description
Navier-Stokes turbulence
Closure Theories
Renormalized . . .
Renormalization Group
Passive Scalar
Dynamic Functional
Magnetic Reconnection
Mean Field . . .
Magneto-Rotational . . .
Interstellar Medium (ISM)
Turbulence in Fusion
Literature
Now substitute perturbation expansion for u
equating coefficients:
u(2) can be expressed by u(0)
What is a plasma ?
Kinetic description
Fluid description
Navier-Stokes turbulence
Closure Theories
Renormalized . . .
Renormalization Group
Passive Scalar
Dynamic Functional
Magnetic Reconnection
Mean Field . . .
Magneto-Rotational . . .
Interstellar Medium (ISM)
Turbulence in Fusion
Literature
stirring Gaussian =⇒ u(0) Gaussian=⇒
⟨u(0)u(0)u(0)u(0)
⟩can be factored as in Quasi-Normal approximation
second-order correlation tensor:
What is a plasma ?
Kinetic description
Fluid description
Navier-Stokes turbulence
Closure Theories
Renormalized . . .
Renormalization Group
Passive Scalar
Dynamic Functional
Magnetic Reconnection
Mean Field . . .
Magneto-Rotational . . .
Interstellar Medium (ISM)
Turbulence in Fusion
Literature
6.1.3. Graphical representation of the perturbation series
all orders can be expressed by zero-order terms, but divergent series
three main constituents: u(0), G0 and M
zero-order:
first-order: wavenumber conservation
What is a plasma ?
Kinetic description
Fluid description
Navier-Stokes turbulence
Closure Theories
Renormalized . . .
Renormalization Group
Passive Scalar
Dynamic Functional
Magnetic Reconnection
Mean Field . . .
Magneto-Rotational . . .
Interstellar Medium (ISM)
Turbulence in Fusion
Literature
second-order: two M factors:
third-order: three M factors:
What is a plasma ?
Kinetic description
Fluid description
Navier-Stokes turbulence
Closure Theories
Renormalized . . .
Renormalization Group
Passive Scalar
Dynamic Functional
Magnetic Reconnection
Mean Field . . .
Magneto-Rotational . . .
Interstellar Medium (ISM)
Turbulence in Fusion
Literature
graphical expansion for correlation tensor
zero-order:
second-order:
this is middle second-order term:
What is a plasma ?
Kinetic description
Fluid description
Navier-Stokes turbulence
Closure Theories
Renormalized . . .
Renormalization Group
Passive Scalar
Dynamic Functional
Magnetic Reconnection
Mean Field . . .
Magneto-Rotational . . .
Interstellar Medium (ISM)
Turbulence in Fusion
Literature
this is the last second-order term:
The third is a mirrow image of this one.
What is a plasma ?
Kinetic description
Fluid description
Navier-Stokes turbulence
Closure Theories
Renormalized . . .
Renormalization Group
Passive Scalar
Dynamic Functional
Magnetic Reconnection
Mean Field . . .
Magneto-Rotational . . .
Interstellar Medium (ISM)
Turbulence in Fusion
Literature
fourth-order showing four of the 29 fourth-order diagrams:
Now resummation (renormalisation): new diagram elements
Write correlation tensor as:
What is a plasma ?
Kinetic description
Fluid description
Navier-Stokes turbulence
Closure Theories
Renormalized . . .
Renormalization Group
Passive Scalar
Dynamic Functional
Magnetic Reconnection
Mean Field . . .
Magneto-Rotational . . .
Interstellar Medium (ISM)
Turbulence in Fusion
Literature
6.1.4. Class A diagram: the renormalized propagator
Wyld (1961): Class A diagrams are those diagrams which can be split intotwo pieces by cutting a single Q0 line.
zero-order: Q0 can be expressed in terms of two zero-order propagatorsacting on the spectrum of the stirring forces w(k;ω, ω′)
This looks graphically like
Now second-order:
Let’s summarize: at zero order, we have w with a G0 on each side. Atsecond order, w has a G0 on one side and a diagram which connects like aG0 on the other. This holds for all orders. Thus we have a generalization
What is a plasma ?
Kinetic description
Fluid description
Navier-Stokes turbulence
Closure Theories
Renormalized . . .
Renormalization Group
Passive Scalar
Dynamic Functional
Magnetic Reconnection
Mean Field . . .
Magneto-Rotational . . .
Interstellar Medium (ISM)
Turbulence in Fusion
Literature
of
which reads
where G(k, ω) is the renormalized propagator.
Graphically, this corresponds to
What is a plasma ?
Kinetic description
Fluid description
Navier-Stokes turbulence
Closure Theories
Renormalized . . .
Renormalization Group
Passive Scalar
Dynamic Functional
Magnetic Reconnection
Mean Field . . .
Magneto-Rotational . . .
Interstellar Medium (ISM)
Turbulence in Fusion
Literature
6.1.5. Class B diagrams: renormalized perturbation series
Class B diagrams can’t be split into two by cutting a single Q0 line.
In the class A diagrams, certain diagram parts were propagator like, that is,they connected like G0: renormalize G0 by adding up all diagrams whichconnect like G0.
Renormalize vertex: add up all diagrams which connect like a vertex
Example: consider fourth-order diagram
The part
connects like a point vertex =⇒ renormalized vertex
What is a plasma ?
Kinetic description
Fluid description
Navier-Stokes turbulence
Closure Theories
Renormalized . . .
Renormalization Group
Passive Scalar
Dynamic Functional
Magnetic Reconnection
Mean Field . . .
Magneto-Rotational . . .
Interstellar Medium (ISM)
Turbulence in Fusion
Literature
replace vertex by renormalized vertex:
Therefore the key to the class B diagrams is as follows:
1. Find those diagrams which cannot be reduced to a lower order byreplacing diagram parts.
2. Call these the irreducible diagrams.
3. Replace all elements in the irreducible diagrams by their renormalizedforms.
4. Write down all these modified diagrams in order, thus generating arenormalized perturbation expansion.
What is a plasma ?
Kinetic description
Fluid description
Navier-Stokes turbulence
Closure Theories
Renormalized . . .
Renormalization Group
Passive Scalar
Dynamic Functional
Magnetic Reconnection
Mean Field . . .
Magneto-Rotational . . .
Interstellar Medium (ISM)
Turbulence in Fusion
Literature
Result for Q(k;ω, ω′)
This is an integral equation for Q(k;ω, ω)
Combine vertex and propagator expansions:
Integral equation for the renormalized vertex
What is a plasma ?
Kinetic description
Fluid description
Navier-Stokes turbulence
Closure Theories
Renormalized . . .
Renormalization Group
Passive Scalar
Dynamic Functional
Magnetic Reconnection
Mean Field . . .
Magneto-Rotational . . .
Interstellar Medium (ISM)
Turbulence in Fusion
Literature
Integral equation for the renormalized propagator G(k, ω)
Pecularity of this diagram:
unrenormalized propagator emerging from the left !!!
Reason for this: symbolic form of Navier-Stokes
L0u(k) = λM(k)u(j)u(k − j) , L0 = ∂t + νk2
and renormalize r.h.s., then invert L0 which results in G0
What is a plasma ?
Kinetic description
Fluid description
Navier-Stokes turbulence
Closure Theories
Renormalized . . .
Renormalization Group
Passive Scalar
Dynamic Functional
Magnetic Reconnection
Mean Field . . .
Magneto-Rotational . . .
Interstellar Medium (ISM)
Turbulence in Fusion
Literature
6.1.6. Second-order closures
What have we done:
We replaced a wildly divergent series with one of unknown properties !
We have hope that it might be assymptotic, but we simple don’t know !
Well known examples recovered from this Wyld (1961) formulation:
Example 1:
correlation tensor: truncate at second order (in number vertices)vertex: truncate at first order (unrenormalized vertex)propagator: truncate at zero order (unrenormalized propagator)
This is Chandrasekhar’s theory (1955) which is the two-time analog ofquasi-normality.
What is a plasma ?
Kinetic description
Fluid description
Navier-Stokes turbulence
Closure Theories
Renormalized . . .
Renormalization Group
Passive Scalar
Dynamic Functional
Magnetic Reconnection
Mean Field . . .
Magneto-Rotational . . .
Interstellar Medium (ISM)
Turbulence in Fusion
Literature
Example 2:
correlation tensor: truncate at second ordervertex: truncate at first orderpropagator: truncate at second order
This is the pioneering direct-interaction approximation (DIA) by Kraichnan(1959): second-order closure with line and with no vertex renormalization.