Degasperis–Procesi equation

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Template:Short description In mathematical physics, the Degasperis–Procesi equation

utuxxt+2κux+4uux=3uxuxx+uuxxx

is one of only two exactly solvable equations in the following family of third-order, non-linear, dispersive PDEs:

utuxxt+2κux+(b+1)uux=buxuxx+uuxxx,

where κ and b are real parameters (b=3 for the Degasperis–Procesi equation). It was discovered by Antonio Degasperis and Michela Procesi in a search for integrable equations similar in form to the Camassa–Holm equation, which is the other integrable equation in this family (corresponding to b=2); that those two equations are the only integrable cases has been verified using a variety of different integrability tests.Template:Sfnm Although discovered solely because of its mathematical properties, the Degasperis–Procesi equation (with κ>0) has later been found to play a similar role in water wave theory as the Camassa–Holm equation.Template:Sfnm

Soliton solutions

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Among the solutions of the Degasperis–Procesi equation (in the special case κ=0) are the so-called multipeakon solutions, which are functions of the form

u(x,t)=i=1nmi(t)e|xxi(t)|

where the functions mi and xi satisfyTemplate:Sfn

x˙i=j=1nmje|xixj|,m˙i=2mij=1nmjsgn(xixj)e|xixj|.

These ODEs can be solved explicitly in terms of elementary functions, using inverse spectral methods.Template:Sfnm

When κ>0 the soliton solutions of the Degasperis–Procesi equation are smooth; they converge to peakons in the limit as κ tends to zero.Template:Sfnm

Discontinuous solutions

The Degasperis–Procesi equation (with κ=0) is formally equivalent to the (nonlocal) hyperbolic conservation law

tu+x[u22+G2*3u22]=0,

where G(x)=exp(|x|), and where the star denotes convolution with respect to x. In this formulation, it admits weak solutions with a very low degree of regularity, even discontinuous ones (shock waves).Template:Sfnm In contrast, the corresponding formulation of the Camassa–Holm equation contains a convolution involving both u2 and ux2, which only makes sense if u lies in the Sobolev space H1=W1,2 with respect to x. By the Sobolev embedding theorem, this means in particular that the weak solutions of the Camassa–Holm equation must be continuous with respect to x.

Notes

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References

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Further reading

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