I’m not sure, but this could be the original technical article.
Symmetries play an important role in modern theories of gravity. The strong equivalence
principle (SEP) constitutes a collection of gravitationalsymmetries which are all implemented
by general relativity. Alternative theories, however, are generally expected to violate some
aspects of SEP. We test three aspects of SEP using observed change rates in the orbital period
and eccentricity of binary pulsar J1713+0747: 1. the gravitational constant’s constancy as part
of locational invariance of gravitation; 2. the post-Newtonian parameter α 3 in gravitational
Lorentz invariance; 3. the universality of free fall (UFF) for strongly self-gravitating bodies.
Based on the pulsar timing result of the combined dataset from the North American Nanohertz
Gravitational Observatory (NANOGrav) and the European Pulsar Timing Array (EPTA), we
find GÛ/G = (−0.1±0.9) ×10^−12 yr^−1
, which is somewhat weaker than Solar system limits, but
applies for strongly self-gravitating objects. Furthermore, we obtain the constraints |∆| < 0.002
for the UFF test and −3 × 10^−20 < α 3 < 4 × 10^−20 at 95% confidence. These are the first direct
UFF and α 3 tests based on pulsar binaries, and they overcome various limitations of previous
tests.
Let’s just check that α 3 from wikipedia shall we.
That’s already in there, < 4 × 10^−20 from pulsar spin down tests. Excellent, all that’s missing from wikipedia is a cross reference to the technical paper. And that doesn’t matter.
Just what does that value of α 3 rule out? It rules out three alternatives to GR and puts a tight Occam’s Razor type “fine tuning” constraint on a fourth.