Delayed phase transition to quarkgluon plasma in binary neutron star merger

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The simulation shows The density of two neutron stars that merge. After the merger, a phase transition from ordinary hadronic matter (red-yellow) to quark matter (green) takes place. • The simulations were performed in order to find out whether such a quark-gluon plasma inside a merger remnant could be detected via graviational waves. See https://arxiv.org/pdf/1912.09340.pdf for the corresponding publication, which has been accepted to Physical Review Letters. • Link to our homepage: https://relastro.uni-frankfurt.de/ • Link to our gallery: https://relastro.uni-frankfurt.de/gal... • Copyright: Lukas R. Weih Luciano Rezzolla (2019)

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