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The Moment of Inertia of the Binary Pulsar J0737-3039A: Constraining the Nuclear Equation of State
I. A. Morrison, T. W. Baumgarte, S. L. Shapiro +1
We construct numerical models of the newly discovered binary pulsar J0737-3039A, both with a fully relativistic, uniformly rotating, equilibrium code that handles arbitrary spins a…
Quasi-equilibrium Binary Black Hole Initial Data for Dynamical Evolutions
Hwei-Jang Yo, James N. Cook, Stuart L. Shapiro +1
We present a formalism for constructing quasi-equilibrium binary black hole initial data suitable for numerical evolution. We construct quasi-equilibrium models by imposing an appr…
Black Hole-Neutron Star Binaries in General Relativity: Quasiequilibrium Formulation
Thomas W. Baumgarte, Monica L. Skoge, Stuart L. Shapiro
We present a new numerical method for the construction of quasiequilibrium models of black hole-neutron star binaries. We solve the constraint equations of general relativity, deco…
Effect of Differential Rotation on the Maximum Mass of Neutron Stars: Realistic Nuclear Equations of State
Ian A. Morrison, Thomas W. Baumgarte, Stuart L. Shapiro
The merger of binary neutron stars is likely to lead to differentially rotating remnants. In this paper, we survey several cold nuclear equations of state (EOSs) and numerically co…