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New results at 3PN via an effective field theory of gravity

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arxiv gr-qc/0701106 v1 pith:3OB7CKHC submitted 2007-01-18 gr-qc astro-phhep-phhep-th

classification gr-qcastro-phhep-phhep-th
keywords effectivefieldgravityorderpost-newtonianresultstheoryapproach
verification ladder T0 review T1 audit T2 compute T3 formal
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NRGR, an Effective Field Theory approach to gravity, has emerged as a powerful tool to systematically compute higher order corrections in the Post-Newtonian expansion. Here we discuss in somehow more detail the recently reported new results for the spin-spin gravitational potential at third Post-Newtonian order.

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  1. Worldline effective field theory of inspiralling black hole binaries in presence of dark photon and axionic dark matter

    hep-th 2023-05 unverdicted novelty 6.0 of 10

    Computes 1PN conservative dynamics for gravitational/EM/Proca fields and 2PN for scalar, plus radiation effects from axion-photon coupling at high PN orders in binary black hole systems with dark matter.

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