Comment on `On the next-to-leading order gravitational spin(1)-spin(2) dynamics' by J. Steinhoff et al

dc.creatorPorto, Rafael A.
dc.creatorRothstein, Ira Z.
dc.date2007-12-12
dc.date.accessioned2026-07-07T08:48:54Z
dc.date.available2026-07-07T08:48:54Z
dc.descriptionIn this comment we explain the discrepancy found between the results in arXiv:0712.1716v1 for the 3PN spin-spin potential and those previously derived in gr-qc/0604099. We point out that to compare one must include sub-leading lower order spin-orbit effects which contribute to the spin-spin potential once one transforms to the PN frame. When these effects are included the results in arXiv:0712.1716v1 do indeed reproduce those found in gr-qc/0604099.
dc.identifierhttps://arxiv.org/abs/0712.2032
dc.identifierhttp://arxiv.org/abs/0712.2032
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/144112
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleComment on `On the next-to-leading order gravitational spin(1)-spin(2) dynamics' by J. Steinhoff et al
dc.typetext

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