The Modern Taylor Method Package

Keywords: ODE, Taylor Method, Taylor Solver, Taylor Series, Numeric Integration, High Accuracy Integration, Ultimate Accuracy, Finite Step, Dynamic Graphic, 3D Stereo, 3D Cursor, Trajectories, Interactive environment, Windows, Linux.

The Modern Taylor Method is a descender of its classical counterpart. It is an efficient method for numerical integration of the Initial Value Problems for Ordinary Differential Equations (ODEs). What distinguishes it from all other numerical methods for ODEs is that only the Taylor Method can compute the increments of the solution with principally unlimited order of approximation so that the integration step does not approach zero whatever high accuracy is specified. That is possible because the method performs the automatic differentiation - exact computing of the derivatives up to any desired order N, allowing to obtain the Taylor series of any length for the solution components.

To download the Demo for Windows (95, NT and later), click here, then download and unzip the file ("Save", don't "Open" it in your browser). See for a short guide navigating you through the DEMO. You can also download the full User Manual (in MS Word doc format), or the recent article published in the Proceedings of the 2005 International Conference on Scientific Computing CSC'05.

To make inquires, please contact Alexander Gofen at galex@ski.org .

With the current version of the product you can:

In particular, the Demo includes a fascinating example of the so called Choreography for the Three Body motion, an eight-shaped orbit, discovered just recently by Chenciner and Montgomery (2000) . Click here to learn more about the Choreographies of N-body problem. You can "feed" the equations found there into the Taylor Center, integrate them, draw the curves and play the motion in the real-time mode all in the same place.  

 
   The future versions will include everything above plus the following:

      Here is how the front panel of the Taylor Center looks like:



And here are the trajectories of a slightly disturbed (Lagrange) case of the Three Body Problem with the central symmetry (Demo/Three bodies/Disturbed/2D). All possible pairs of the three bodies couple randomly in turn. You would prefer to watch it as a real time motion in the Demo rather than as a still image.

To view stereo images, you need anaglyphic Red/Blue glasses (Left - Red, Right - Blue). Such glasses may be ordered here: look for a Red/Blue type (not Red/Cyan).

If you have the anaglyphic glasses, click to view 3D stereo images.

You may also display a field of directions for selected pairs of variables, or better a field of curvy segments, for example like that below:

Field of directions