Showing 1–20 of 24 results
/ Date/ Name
Apr 23, 2014A Hybrid Advection Scheme for Conserving Angular Momentum on a Refined Cartesian MeshFeb 12, 2017A Comparison of Grid-Based and SPH Binary Mass-Transfer and Merger SimulationsApr 5, 2006Unexpected Dynamical Instabilities In Differentially Rotating Neutron StarsJan 22, 2001Populating Stellar Orbits Inside a Rotating, Gaseous BarApr 24, 2014A Numerical Method for Studying Super-Eddington Mass Transfer in Double White Dwarf BinariesFeb 28, 2007Further Evidence for an Elliptical Instability in Rotating Fluid Bars and Ellipsoidal StarsJan 28, 2008Magnetized Neutron Star Mergers and Gravitational Wave SignalsAug 2, 2012Do R Coronae Borealis Stars Form from Double White Dwarf Mergers?Jan 24, 2001Alternative Fourier Expansions for Inverse Square Law ForcesMar 5, 1997The Relative Stability Against Merger of Close, Compact BinariesMar 25, 1995Millisecond Pulsars: Detectable Sources of Continuous Gravitational Waves?Nov 30, 1999Gravitational Waves from Long-Duration Simulations of the Dynamical Bar InstabilityAug 20, 2007Simulating binary neutron stars: dynamics and gravitational wavesNov 28, 2008NuGrid: Toward High Precision Double-Degenerate Merger Simulations with SPH in 3DSep 20, 2001Numerical evolutions of nonlinear r-modes in neutron starsOct 31, 2000Non-Linear Evolution of the r-Modes in Neutron StarsJul 17, 2001Numerical Methods for the Simulation of Dynamical Mass Transfer in BinariesMar 23, 1998A Physical Model of Warped Galaxy DisksOct 18, 2006Population Boundaries for Galactic White Dwarf Binaries in LISA's Amplitude-Frequency DomainAug 14, 2009Constructing Synchronously Rotating Double White Dwarf Binaries