Koji Uryu

Simulation of merging binary neutron stars in full general relativity: Gamma = two case

We perform 3D numerical simulations for the merger of equal mass binary neutron stars in full general relativity. We adopt a

Gravitational waves from the merger of binary neutron stars in a fully general relativistic simulation

\ensuremath{\Gamma}

Merger of binary neutron stars of unequal mass in full general relativity

-law equation of state in the form

Merger of black hole-neutron star binaries: Nonspinning black hole case

P=(\ensuremath{\Gamma}\ensuremath{-}1)\ensuremath{\rho}\ensuremath{\varepsilon}

Merger of black hole-neutron star binaries in full general relativity

where P,

Magnetohydrodynamics in stationary and axisymmetric spacetimes: A fully covariant approach

\ensuremath{\rho},

Comparing the inspiral of irrotational and corotational binary neutron stars

\ensuremath{\varepsilon}

New numerical scheme to compute three-dimensional configurations of quasiequilibrium compact stars in general relativity: Application to synchronously rotating binary star systems

and

Equilibrium solutions of relativistic rotating stars with mixed poloidal and toroidal magnetic fields

\ensuremath{\Gamma}