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I think this is a fine project, but we should temper our expectations! I suspect that the current solver isn't even close to the bottleneck in any of our calculations. N-R usually converges in only a couple iterations except in high eccentricity cases, I believe.
Right now the Kepler equation is solved using the Newton-Raphson method.
PINT/src/pint/models/stand_alone_psr_binaries/binary_generic.py
Line 350 in 18c643a
There are faster (and no less accurate) methods for doing this.
For example, Markley (1995) http://adsabs.harvard.edu/abs/1995CeMDA..63..101M
We should implement such a method instead of the Newton-Raphson method.
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