Black holes, gravitational waves and fundamental physics: a roadmap
L Barack, V Cardoso, S Nissanke… - … and quantum gravity, 2019 - iopscience.iop.org
70 AIM, UMR 7158, CEA/DRF, CNRS, Université Paris Diderot, Irfu/Service d'Astrophysique,
Centre de Saclay, FR-91191 Gif-sur-Yvette, France
Centre de Saclay, FR-91191 Gif-sur-Yvette, France
[HTML][HTML] Gravitational-wave tests of general relativity with ground-based detectors and pulsar-timing arrays
This review is focused on tests of Einstein's theory of general relativity with gravitational
waves that are detectable by ground-based interferometers and pulsar-timing experiments …
waves that are detectable by ground-based interferometers and pulsar-timing experiments …
Black hole based tests of general relativity
General relativity has passed all solar system experiments and neutron star based tests,
such as binary pulsar observations, with flying colors. A more exotic arena for testing …
such as binary pulsar observations, with flying colors. A more exotic arena for testing …
Chern–Simons modified general relativity
S Alexander, N Yunes - Physics Reports, 2009 - Elsevier
Chern–Simons modified gravity is an effective extension of general relativity that captures
leading-order, gravitational parity violation. Such an effective theory is motivated by anomaly …
leading-order, gravitational parity violation. Such an effective theory is motivated by anomaly …
Fundamental theoretical bias in gravitational wave astrophysics<? format?> and the parametrized post-Einsteinian framework
N Yunes, F Pretorius - Physical Review D—Particles, Fields, Gravitation, and …, 2009 - APS
We consider the concept of fundamental bias in gravitational wave astrophysics as the
assumption that general relativity is the correct theory of gravity during the entire wave …
assumption that general relativity is the correct theory of gravity during the entire wave …
Perturbations of spinning black holes beyond General Relativity: Modified Teukolsky equation
The detection of gravitational waves from compact binary mergers by the LIGO/Virgo
Collaboration has, for the first time, allowed for tests of relativistic gravity in the strong …
Collaboration has, for the first time, allowed for tests of relativistic gravity in the strong …
Low-frequency gravitational-wave science with eLISA/NGO
We review the expected science performance of the New Gravitational-Wave Observatory
(NGO, aka eLISA), a mission under study by the European Space Agency for launch in the …
(NGO, aka eLISA), a mission under study by the European Space Agency for launch in the …
Testing general relativity with low-frequency, space-based gravitational-wave detectors
JR Gair, M Vallisneri, SL Larson, JG Baker - Living Reviews in Relativity, 2013 - Springer
We review the tests of general relativity that will become possible with space-based
gravitational-wave detectors operating in the∼ 10− 5− 1 Hz low-frequency band. The …
gravitational-wave detectors operating in the∼ 10− 5− 1 Hz low-frequency band. The …
The next generation global gravitational wave observatory: the science book
V Kalogera, BS Sathyaprakash, M Bailes… - arXiv preprint arXiv …, 2021 - arxiv.org
The next generation of ground-based gravitational-wave detectors will observe
coalescences of black holes and neutron stars throughout the cosmos, thousands of them …
coalescences of black holes and neutron stars throughout the cosmos, thousands of them …
Metric for rapidly spinning black holes suitable for strong-field tests of the no-hair theorem
T Johannsen, D Psaltis - Physical Review D—Particles, Fields, Gravitation, and …, 2011 - APS
According to the no-hair theorem, astrophysical black holes are uniquely characterized by
their masses and spins and are described by the Kerr metric. Several parametric deviations …
their masses and spins and are described by the Kerr metric. Several parametric deviations …