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Riemann invariant

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Riemann invariants are mathematical transformations made on a system of conservation equations to make them more easily solvable. Riemann invariants are constant along the characteristic curves of the partial differential equations where they obtain the name invariant. They were first obtained by Bernhard Riemann in his work on plane waves in gas dynamics.

Contents

Mathematical theory

Consider the set of conservation equations:

l i ( A i j u j t + a i j u j x ) + l j b j = 0

where A i j and a i j are the elements of the matrices A and a where l i and b i are elements of vectors. It will be asked if it is possible to rewrite this equation to

m j ( β u j t + α u j x ) + l j b j = 0

To do this curves will be introduced in the ( x , t ) plane defined by the vector field ( α , β ) . The term in the brackets will be rewritten in terms of a total derivative where x , t are parametrized as x = X ( η ) , t = T ( η )

d u j d η = T u j t + X u j x

comparing the last two equations we find

α = X ( η ) , β = T ( η )

which can be now written in characteristic form

m j d u j d η + l j b j = 0

where we must have the conditions

l i A i j = m j T l i a i j = m j X

where m j can be eliminated to give the necessary condition

l i ( A i j X a i j T ) = 0

so for a nontrival solution is the determinant

| A i j X a i j T | = 0

For Riemann invariants we are concerned with the case when the matrix A is an identity matrix to form

u i t + a i j u j x = 0

notice this is homogeneous due to the vector n being zero. In characteristic form the system is

l i d u i d t = 0 with d x d t = λ

Where l is the left eigenvector of the matrix A and λ s is the characteristic speeds of the eigenvalues of the matrix A which satisfy

| A λ δ i j | = 0

To simplify these characteristic equations we can make the transformations such that d r d t = l i d u i d t

which form

μ l i d u i = d r

An integrating factor μ can be multiplied in to help integrate this. So the system now has the characteristic form

d r d t = 0 on d x d t = λ i

which is equivalent to the diagonal system

r t k + λ k r x k = 0 , k = 1 , . . . , N .

The solution of this system can be given by the generalized hodograph method.

Example

Consider the shallow water equations

ρ t + ρ u x + u ρ x = 0 u t + u u x + ( c 2 / ρ ) ρ x = 0

write this system in matrix form

( ρ u ) t + ( u ρ c 2 ρ u ) ( ρ u ) x = ( 0 0 )

where the matrix a from the analysis above the eigenvalues and eigenvectors need to be found.The eigenvalues are found to satisfy

λ 2 2 u λ + u 2 c 2 = 0

to give

λ = u ± c

and the eigenvectors are found to be

( 1 c ρ ) , ( 1 c ρ )

where the Riemann invariants are

r 1 = u + c ρ d ρ , r 2 = u c ρ d ρ ,

In shallow water equations there is the relation c = ρ to give the Riemann invariants

r 1 = u + 2 ρ , r 2 = u 2 ρ ,

to give the equations

r 1 t + ( u + ρ ) r 1 x = 0 r 2 t + ( u ρ ) r 2 x = 0

Which can be solved by the hodograph transformation. If the matrix form of the system of pde's is in the form

A v t + B v x = 0

Then it may be possible to multiply across by the inverse matrix A 1 so long as the matrix determinant of A is not zero.

References

Riemann invariant Wikipedia