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Published in Phys.Rev.D 105 (2022) 8, 084018, 2021
We compute the third post-Newtonian (3PN) accurate instantaneous contributions to the radiated gravitational wave energy and angular momentum arising from the hyperbolic passages of nonspinning compact objects. The present computations employ 3PN-accurate instantaneous contributions to the far-zone energy and angular momentum fluxes and the 3PN-accurate Keplerian type parametric solution for compact binaries in hyperbolic orbits.
Recommended citation: Cho et al. (2021); "Third order post-Newtonian gravitational radiation from two-body scattering: Instantaneous energy and angular momentum radiation." Phys.Rev.D. 105, 8, 084018. https://doi.org/10.1103/PhysRevD.105.084018
Published in arXiv eprints, 2022
The first data release of the Indian Pulsar Timing Array experiment including times of arrival (TOAs) and dispersion measure (DM) time series for 14 millisecond pulsars spanning 3.5 years.
Recommended citation: Tarafdar, P et al. (2022); "The Indian Pulsar Timing Array: First data release." arXiv eprints; 2206.09289.
Published in Physical Review D, 2023
Gravitational waveform and pulsar timing array signal models for relativistic encounters of stellar-mass and supermassive black holes along hyperbolic trajectories.
Recommended citation: Dandapat S, et al. (2023); "Gravitational waves from black-hole encounters: Prospects for ground and galaxy-based observatories." PRD 108 024013. https://doi.org/10.1103/PhysRevD.108.024013
Published in Physical Review D, 2024
Searching for linear gravitational wave memory induced by hyperbolic encounters in the NANOGrav 12.5-year dataset.
Recommended citation: Dandapat S, et al. (2024); "Efficient prescription to search for linear gravitational wave memory from hyperbolic black hole encounters and its application to the NANOGrav 12.5-year dataset." PRD 109 103018 . https://doi.org/10.1103/PhysRevD.109.103018
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