A new code for equilibriums and quasiequilibrium initial data of compact objects
arXiv:1108.3065 · doi:10.1103/PhysRevD.85.064014
Abstract
We present a new code, named COCAL - Compact Object CALculator, for the computation of equilibriums and quasiequilibrium initial data sets of single or binary compact objects of all kinds. In the cocal code, those solutions are calculated on one or multiple spherical coordinate patches covering the initial hypersurface up to the asymptotic region. The numerical method used to solve field equations written in elliptic form is an adaptation of self-consistent field iterations in which Green's integral formula is computed using multipole expansions and standard finite difference schemes. We extended the method so that it can be used on a computational domain with excised regions for a black hole and a binary companion. Green's functions are constructed for various types of boundary conditions imposed at the surface of the excised regions for black holes. The numerical methods used in cocal are chosen to make the code simpler than any other recent initial data codes, accepting the second order accuracy for the finite difference schemes. We perform convergence tests for time symmetric single black hole data on a single coordinate patch, and binary black hole data on multiple patches. Then, we apply the code to obtain spatially conformally flat binary black hole initial data using boundary conditions including the one based on the existence of equilibrium apparent horizons.
Revised version with a new title, 29 pages
References in corpus (26)
- Total recoil: the maximum kick from nonspinning black-hole binary inspiral
- Inspiral, merger and ringdown of unequal mass black hole binaries: a multipolar analysis
- Supermassive recoil velocities for binary black-hole mergers with antialigned spins
- Binary Neutron Star Mergers: Dependence on the Nuclear Equation of State
- Magnetized Neutron Star Mergers and Gravitational Wave Signals
- Accurate evolutions of inspiralling and magnetized neutron-stars: equal-mass binaries
- Exploring black hole superkicks
- General relativistic simulations of magnetized binary neutron star mergers
- Binary-black-hole initial data with nearly-extremal spins
- Gravitational waves from spinning black hole-neutron star binaries: dependence on black hole spins and on neutron star equations of state
- Circular orbits and spin in black-hole initial data
- Waveless Approximation Theories of Gravity
- Initial data for black hole-neutron star binaries: a flexible, high-accuracy spectral method
- Mergers of Magnetized Neutron Stars with Spinning Black Holes: Disruption, Accretion and Fallback
- Exploring binary-neutron-star-merger scenario of short-gamma-ray bursts by gravitational-wave observation
- Quasiequilibrium black hole-neutron star binaries in general relativity
- Relativistic black hole-neutron star binaries in quasiequilibrium: effects of the black hole excision boundary condition
- Is super-Planckian physics visible? -- Scattering of black holes in 5 dimensions
- Black hole puncture initial data with realistic gravitational wave content
- Stellar core collapse in full general relativity with microphysics - Formulation and Spherical collapse test -
- Quasiequilibrium sequences of black-hole--neutron-star binaries in general relativity
- Magnetohydrodynamics in stationary and axisymmetric spacetimes: a fully covariant approach
- Numerical method for binary black hole/neutron star initial data: Code test
- Models of helically symmetric binary systems
- Quasi-equilibrium models for triaxially deformed rotating compact stars
- Thermodynamics of magnetized binary compact objects
Cited by in corpus (32)
- Binary neutron-star mergers: a review of Einstein's richest laboratory
- Rotating Stars in Relativity
- The Science of the Einstein Telescope
- Realistic Finite-Temperature Effects in Neutron Star Merger Simulations
- Modeling differential rotations of compact stars in equilibriums
- The initial value problem as it relates to numerical relativity
- Equilibrium solutions of relativistic rotating stars with mixed poloidal and toroidal magnetic fields
- New code for equilibriums and quasiequilibrium initial data of compact objects. IV. Rotating relativistic stars with mixed poloidal and toroidal magnetic fields
- Effect of spin on the inspiral of binary neutron stars
- Quasi-equilibrium configurations of binary systems of dark matter admixed neutron stars
- Great Impostors: Extremely Compact, Merging Binary Neutron Stars in the Mass Gap Posing as Binary Black Holes
- Horizon Surface Gravity in Corotating Black Hole Binaries
- Uniformly rotating, axisymmetric and triaxial quark stars in general relativity
- Constant circulation sequences of binary neutron stars and their spin characterization
- Initial-data contribution to the error budget of gravitational waves from neutron-star binaries
- New code for equilibriums and quasiequilibrium initial data of compact objects. II. Convergence tests and comparisons of binary black hole initial data
- Elliptica: a new pseudo-spectral code for the construction of initial data
- Evolution of equal mass binary bare quark stars in full general relativity: could a supramassive merger remnant experience prompt collapse?
- Binary black hole circular orbits computed with COCAL
- Evolution of bare quark stars in full general relativity: Single star case
- Complete initial value spacetimes containing black holes in general relativity: Application to black hole-disk systems
- Do triaxial supramassive compact stars exist?
- NRPyElliptic: A Fast Hyperbolic Relaxation Elliptic Solver for Numerical Relativity, I: Conformally Flat, Binary Puncture Initial Data
- Non-axisymmetric oscillations of rapidly rotating relativistic stars by conformal flatness approximation
- Gravitational wave content and stability of uniformly, rotating, triaxial neutron stars in general relativity
- Initial data for high-compactness black hole-neutron star binaries
- Equilibriums of extremely magnetized compact stars with force-free magnetotunnels
- Methods for relativistic self-gravitating fluids: From binary neutron stars to black hole-disks and magnetized rotating neutron stars
- Stationary massive disks around black holes: realistic equation of state and bifurcation
- Gravitational systems in asymptotically anti-de Sitter space-times
- Source term method for binary neutron stars initial data
- The Parallel Compact Object CALculator: An Efficient General Relativistic Initial Data Solver for Compact Objects