TY  - JOUR
A1  - Ujevic, Maximiliano
A1  - Rashti, Alireza
A1  - Gieg, Henrique Leonhard
A1  - Tichy, Wolfgang
A1  - Dietrich, Tim
T1  - High-accuracy high-mass-ratio simulations for binary neutron stars and their comparison to existing waveform models
T2  - Physical review : D, Particles, fields, gravitation, and cosmology
N2  - The subsequent observing runs of the advanced gravitational-wave detector network will likely provide us with various gravitational-wave observations of binary neutron star systems. For an accurate interpretation of these detections, we need reliable gravitational-wave models. To test and to point out how existing models could be improved, we perform a set of high-resolution numerical relativity simulations for four different physical setups with mass ratios q = 1.25, 1.50, 1.75, 2.00, and total gravitational mass M = 2.7 M???. Each configuration is simulated with five different resolutions to allow a proper error assessment. Overall, we find approximately second-order converging results for the dominant (2,2) mode, but also the subdominant (2,1), (3,3), and (4,4) modes, while generally, the convergence order reduces slightly for an increasing mass ratio. Our simulations allow us to validate waveform models, where we find generally good agreement between state-of-the-art models and our data, and to prove that scaling relations for higher modes currently employed for binary black hole waveform modeling also apply for the tidal contribution. Finally, we also test if the current NRTidal model used to describe tidal effects is a valid description for high-mass-ratio systems. We hope that our simulation results can be used to further improve and test waveform models in preparation for the next observing runs.
Y1  - 2022
UR  - https://publishup.uni-potsdam.de/frontdoor/index/index/docId/63720
SN  - 2470-0010
SN  - 2470-0029
VL  - 106
IS  - 2
PB  - American Physical Society
CY  - College Park
ER  -