A fast method for solving the heat equation by layer potentials

نویسنده

  • Johannes Tausch
چکیده

Boundary integral formulations of the heat equation involve time convolutions in addition to surface potentials. If M is the number of time steps and N is the number of degrees of freedom of the spatial discretization then the direct computation of a heat potential involves order N M operations. This article describes a fast method to compute three dimensional heat potentials which is based on Chebyshev interpolation of the heat kernel in both space and time. The computational complexity is order pqNM operations, where p and q are the orders of the polynomial approximation in space and time.

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عنوان ژورنال:
  • J. Comput. Physics

دوره 224  شماره 

صفحات  -

تاریخ انتشار 2007