Gravitational Waves, relativistic celestial mechanics and black hole physics
Workshop on Astropysics and General Relativity: Astro-GR 2015
Modelling the Quasi-Periodic Oscillations and Their Respective Time Lags in Neutro...
Full text | |
Author(s): |
Lins, Aline Nascimento
;
Sturani, Riccardo
Total Authors: 2
|
Document type: | Journal article |
Source: | PHYSICAL REVIEW D; v. 103, n. 8, p. 23-pg., 2021-04-19. |
Abstract | |
We investigate the possibility of testing short-distance modifications to general relativity via higher-curvature terms in the fundamental gravity Lagrangian by analyzing their impact on observations of spinning astronomical binary systems. By using effective field theory methods applied to the two-body problem, generic lower bounds on the short-distance scale accompanying high-curvature terms can be set. In particular, we extend known results by deriving spin-dependent effects in binding energy, radiation emission process, and spin precession equations in binary systems, which are the fundamental ingredients to observe spin-dependent effects in gravitational wave detections from compact binary coalescences and spin precession in double binary pulsars. (AU) | |
FAPESP's process: | 16/01343-7 - ICTP South American Institute for Fundamental Research: a regional center for theoretical physics |
Grantee: | Nathan Jacob Berkovits |
Support Opportunities: | Special Projects |