IMR consistency tests with higher modes on gravitational signals from the second observing run of LIGO and Virgo
- 1. Dipartimento di Fisica 'Enrico Fermi', Università di Pisa, Pisa I-56127 (Italy)
- 2. Center for Computational Relativity and Gravitation, Rochester Institute of Technology, Rochester, NY 14623 (United States)
Description
Current tests of general relativity are performed using approximations which neglect a key feature of complete solution of Einstein's theory: higher-order modes. Our analysis will reassess these tests, including these higher-order mode effects. We have chosen to perform inspiral-merger-ringdown consistency tests on the gravitational transients detected by LIGO and Virgo during the observing run O2. We use an approximant which includes all higher modes with (NRSur7dq2) and then, for three selected cases, we repeat the tests involving fits on numerical relativity simulations. The results are consist with the predictions of general relativity and the combined posterior distribution for the analyzed events does not show deviations from GR above the 39.3% confidence level. (paper)
Availability note (English)
Available from http://dx.doi.org/10.1088/1361-6382/ab5629Additional details
Identifiers
Publishing Information
- Journal Title
- Classical and Quantum Gravity
- Journal Volume
- 36
- Journal Issue
- 24
- Journal Page Range
- [21 p.]
- ISSN
- 0264-9381
- CODEN
- CQGRDG
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 52029351
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- APPROXIMATIONS; EINSTEIN FIELD EQUATIONS; GENERAL RELATIVITY THEORY; GRAVITATIONAL WAVE DETECTORS; SIGNALS; SIMULATION
- Descriptors DEC
- CALCULATION METHODS; EQUATIONS; FIELD EQUATIONS; FIELD THEORIES; MEASURING INSTRUMENTS; RADIATION DETECTORS; RELATIVITY THEORY