Post-merger gravitational-waveforms from binary neutron stars
First Release : 2014-12-24 ( ver. 1.0 ) Last Update : 2014-12-24 ( ver. 1.0 )
- Kentaro Takami, Luciano Rezzolla and Luca Baiotti,”Constraining the Equation of State of Neutron Stars from Binary Mergers”, Phys. Rev. Lett., 113, 091104, 2014 ( arXiv:1403.5672).
- Kentaro Takami, Luciano Rezzolla and Luca Baiotti,”Spectral properties of the post-merger gravitational-wave signal from binary neutron stars”, Phys. Rev. D, 91, 064001, 2015 ( arXiv:1412.3240).
Description : All of these simulations have been performed in full general relativity using the fourth-order finite-differencing code McLachlan. At the same time, the general-relativistic hydrodynamics equations have been solved using the finite-volume code Whisky, where “hybrid equations of states (EOSs)” combined with an ideal-fluid and a piece-wise polytropes EOS for APR4, ALF2, SLy, H4 or GNH3 have been used. Download