Conformally flat, quasi-circular numerical simulations of the gravitational wave chirp from binary neutron star merger GW170817

arXiv:2103.05082 · gr-qc, astro-ph.HE, astro-ph.SR · Submitted 2021-03-08 · Read on arXiv

gr-qc, astro-ph.HE, astro-ph.SR

Submitted: 2021-03-08

Updated: 2021-03-08

Comments: 5 pages, 1 figure

Journal ref: J. Phys. Astron. 9, 204 (2021)

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Calibration — 4× in this paper · explained in 7 episodes
• Gravitational Wave Emission — 2× in this paper · explained in 2 episodes
• Equation of State (EoS) — 1× in this paper · explained in 4 episodes
• Trace — 1× in this paper · explained in 2 episodes

Sources

• Review of Conformally Flat Approximation for Binary Neutron Star Initial Conditions

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