| Texto completo | |
| Autor(es): |
Foffa, Stefano
;
Porto, Rafael A.
;
Rothstein, Ira
;
Sturani, Riccardo
Número total de Autores: 4
|
| Tipo de documento: | Artigo Científico |
| Fonte: | PHYSICAL REVIEW D; v. 100, n. 2, p. 25-pg., 2019-07-24. |
| Resumo | |
We complete the derivation of the conservative dynamics of binary systems to fourth Post-Newtonian (4PN) order in the effective field theory (EFT) approach. We present a self-contained (ambiguity-free) computation of the renormalized Lagrangian, entirely within the confines of the PN expansion. While we confirm the final results reported in the literature, we clarify several issues regarding intermediate infrared (IR) and ultraviolet (UV) divergences, as well as the renormalization procedure. First, we properly identify the IR and UV singularities using (only) dimensional regularization and the method of regions, which are the pillars of the EFT formalism. This requires a careful study of scaleless integrals in the potential region, as well as conservative contributions from radiation modes due to tail effects. As expected by consistency, the UV divergences in the near region (due to the point-particle limit) can be absorbed into two counterterms in the worldline effective theory. The counterterms can then be removed by field redefinitions, such that the renormalization scheme dependence has no physical effect to 4PN order. The remaining IR poles, which are spurious in nature, are unambiguously removed by implementing the zero-bin subtraction in the EFT approach. The procedure transforms the IR singularities into UV counterparts. As anticipated, the leftover UV poles explicitly cancel out against UV divergences in conservative terms from radiation reaction, uniquely determining the gravitational potential. Similar artificial IR/UV poles, which are intimately linked to the split into regions, are manifest at lower orders. Starting at 4PN order, both local- and nonlocal-in-time contributions from the radiation region enter in the conservative dynamics. Neither additional regulators nor ambiguity parameters are introduced at any stage of the computations. (AU) | |
| Processo FAPESP: | 12/14132-3 - Análise das ondas gravitacionais |
| Beneficiário: | Riccardo Sturani |
| Modalidade de apoio: | Auxílio à Pesquisa - Jovens Pesquisadores |