Hem > Black holes in an Effective Field Theory extension of GR |
Article | |
Report number | arXiv:1808.08962 |
Title | Black holes in an Effective Field Theory extension of GR |
Related title | Erratum: Black Holes in an Effective Field Theory Extension of General Relativity [Phys. Rev. Lett. 121, 251105 (2018)] |
Author(s) | Cardoso, Vitor (Lisbon, CENTRA ; Lisbon, CFTP ; CERN) ; Kimura, Masashi (Lisbon, CENTRA ; Lisbon, CFTP) ; Maselli, Andrea (Lisbon, CENTRA ; Lisbon, CFTP) ; Senatore, Leonardo (KIPAC, Menlo Park ; SLAC ; Stanford U., Phys. Dept.) |
Publication | 2018-12-21 |
Imprint | 2018-08-27 |
Number of pages | 6 |
Note | 8 pages, RevTex4. v2: Minor edits. Accepted for publication in Physical Review Letters |
In: | Phys. Rev. Lett. |
DOI | 10.1103/PhysRevLett.121.251105 10.1103/PhysRevLett.131.109903 (erratum) |
Subject category | hep-th ; Particle Physics - Theory ; hep-ph ; Particle Physics - Phenomenology ; astro-ph.HE ; Astrophysics and Astronomy ; gr-qc ; General Relativity and Cosmology |
Abstract | Effective field theory methods suggest that some rather-general extensions of General Relativity include, or are mimicked by, certain higher-order curvature corrections, with coupling constants expected to be small but otherwise arbitrary. Thus, the tantalizing prospect to test the fundamental nature of gravity with gravitational-wave observations, in a systematic way, emerges naturally. Here, we build black hole solutions in such a framework and study their main properties. Once rotation is included, we find the first purely gravitational example of geometries without $\mathbb{Z}_2$-symmetry. Despite the higher-order operators of the theory, we show that linearized fluctuations of such geometries obey second-order differential equations. We find nonzero tidal Love numbers. We study and compute the quasinormal modes of such geometries. These results are of interest to gravitational-wave science but also potentially relevant for electromagnetic observations of the galactic center or $X$-ray binaries. |
Copyright/License | preprint: (License: arXiv nonexclusive-distrib 1.0) publication: © 2018-2024 authors (License: CC-BY-4.0) |