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Maybe also add a notebook to compute the Detweiler redshift invariant from the values on the worldline. This will need the first-order tensor-mode punctures so may be best done in conjunction with a package that can load those.
The text was updated successfully, but these errors were encountered:
Add an example in the notebook that creates h_ab.
Maybe also add a notebook to compute the Detweiler redshift invariant from the values on the worldline. This will need the first-order tensor-mode punctures so may be best done in conjunction with a package that can load those.
The text was updated successfully, but these errors were encountered: