2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/211387Some years ago, a new powerful technique, known as the Classical Effective Field Theory, was proposed to describe classical phenomena in gravitational systems. Here we show how this approach can be useful to investigate theoretically important issues, such as gravitational radiation in any spacetime dimension. In particular, we derive for the first time the Einstein-Infeld-Hoffman Lagrangian and we compute Einstein's quadrupole formula for any number of flat spacetime dimensions.32 pages, 10 figures. v2: Factor in eq. (3.11) fixed. References addedHigh Energy Physics - TheoryAstrophysicsGeneral Relativity and Quantum CosmologyGravitational radiation in d>4 from effective field theorytext