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Quark Matter in Neutron Star Mergers

R. Oechslin·G. Poghosyan·K. Uryu
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Abstract

Binary neutron star mergers are expected to be one of the most promising source of gravitational waves (GW) for the network of laser interferometric and bar detectors becoming operational in the next few years. The merger wave signal is expected to be sensitive to the interior structure of the neutron star (NS). The structure of high density phases of matter is under current experimental investigation in heavy-ion collisions. We investigate the dependence of the merger process and its GW signal on the presence of quarks in these phases by performing numerical simulations, where the smoothed particle hydrodynamics (SPH) method and the conformally flat approximation for the 3-geometry in general relativistic gravity are implemented.

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R. Oechslin, G. Poghosyan, K. Uryu. 2002-10-30. Quark Matter in Neutron Star Mergers. https://doi.org/10.1016/s0375-9474(03)00895-9

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