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Mergers with microphysics
Merger simulations with microphysics.
Merger simulations on large eccentric orbits.
Simulations dedicated to follow up on GW170817; the first combined detection of gravitational waves, a gamma ray burst, and a kilonova.
Simulation of the double pulsar system PSR J0737-3039, anticipating the emitted gravitational wave signal in more than 50 million years when the two stars will finally merge.
High mass ratio mergers
Simulation of a merger of two neutron stars with a mass ratio of q=1.5.
Merger with a deconfined quark phase
A merger of two neutron stars with mass configuration corresponding to PSR J1829+2456 with the production of deconfined quarks shown in red.