Annual Reviews Extra | The Dynamics of Binary Neutron Star Mergers and GW170817: Supplemental Video 2 @annualreviewsextra | Uploaded June 2020 | Updated October 2024, 1 hour ago.
A supplemental video from the 2020 review by David Radice, Sebastiano Bernuzzi, and Albino Perego, "The Dynamics of Binary Neutron Star Mergers and GW170817," from the Annual Review of Nuclear and Particle Science: annualreviews.org/doi/10.1146/annurev-nucl-013120-114541?utm_source=youtube&utm_medium=ns.radice&utm_campaign=suppvideo
The top panels show rest mass density (top left) and temperature (top right) on the orbital plane for a binary neutron star system with MA = MB = 1.35M⊙ simulated with the SFHo equation of state (Steiner et al. 2012). The bottom panels show histograms of log temperature versus log density and entropy versus log density. From this figure it is possible to better appreciate the thermodynamic conditions in the low-density disk and in the ejecta. Reference: Steiner AW, et al. Astrophys J. 774:17 (2013)
A supplemental video from the 2020 review by David Radice, Sebastiano Bernuzzi, and Albino Perego, "The Dynamics of Binary Neutron Star Mergers and GW170817," from the Annual Review of Nuclear and Particle Science: annualreviews.org/doi/10.1146/annurev-nucl-013120-114541?utm_source=youtube&utm_medium=ns.radice&utm_campaign=suppvideo
The top panels show rest mass density (top left) and temperature (top right) on the orbital plane for a binary neutron star system with MA = MB = 1.35M⊙ simulated with the SFHo equation of state (Steiner et al. 2012). The bottom panels show histograms of log temperature versus log density and entropy versus log density. From this figure it is possible to better appreciate the thermodynamic conditions in the low-density disk and in the ejecta. Reference: Steiner AW, et al. Astrophys J. 774:17 (2013)
