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CactusEinstein Overview

NOTE: THIS FILE IS SOMEWHAT OUT OF DATE. I WILL UPDATE IT WHEN I HAVE MORE TIME.
Cactus Einstein
Thorns for solving the Einstein equations of general relativity.
ADM
This thorn evolves the standard 3+1 variables using the ADM Evolution equations.
ADMAnalysis
This thorn does basic analysis of the metric and extrinsic curvature tensors.
ADMBase
This thorn provides the basic variables used to communicate between thorns doing General Relativity in the $3+1$ formalism.
ADMConstraints
This analysis thorn calculates the violation in the ADM constraints using the standard Einstein variables.
ADMCoupling
The "friend of a friend" thorn to help matter/spacetime coupling. Does nothing itself.
ADMMacros
This thorn provides nothing but a load of macros for other thorns to use.
AHFinder
This thorn looks for apparent horizons (AH) in 3D. An AH is defined as a surface where the expansion of outgoing null geodesics is zero.
CoordGauge
Base thorn to provide the infrastructure for dynamic gauge selection.
EvolSimple
Simplistic evolver for the ADM equations, demonstrating the use of the CactusEinstein arrangement.
This evolver evolves the physical metric, and does not contain the shift.
Extract
Calculate gauge invariant waveforms, using the Moncrief formalism, for cases when the spacetime approximates spherical symmetry.
Calculate other quantities on a surface, such as ADM mass, momenta, and spins.
IDAnalyticBH
This thorn calculates analytic initial data for the Einstein grid functions (lapse, shift, metric, curv) for various black hole spacetimes:
  • Schwarzschild black hole
  • 2 Misner black holes placed on the z-axis
  • n Misner black holes placed in a circle in the x-y plane
  • Brill-Lindquist data
IDAxiBrillBH
This thorn calculates initial data for a black hole distorted by an even parity perturbation.
IDBrillData
Initializes Brill wave data.
IDLinearWaves
Provides analytic data for linear gravitational waves.
IDLinearWaves
Provides analytic data for linear gravitational waves.
IDSimple
Simple initial data sets for 3-metric and extrinsic curvature.
Currently Minkowski in Cartesian coordinates optionally with a conformal factor.
Maximal
This thorn setus up the maximal slicing equation (dtrK/dt=0)
PsiKadelia
This thorn provides a somewhat invariant means of measuring "waves" and other geometrical content in a numerically generated spacetime.
Specifically, the thorn calculates the complex scalars psi0, psi1, psi2, psi3 and psi4 with respect to a specified tetrad, and the invariants I and J.
SpaceMask
Provides utilities for assigning states to individual grid points using a mask grid function.
StaticConformal
This thorn provides the variables defining a static conformal factor which is used to transform the physical metric. If this thorn is active and the ADMBase::metric_type parameter is set to `static conformal' then the ADMBase::g... variables are the conformal values as opposed to the physical values.
timegeodesic
This thorn integrates timelike geodesics. The integration is done `on the fly', that is, at the same time as the evolution of the spacetime is being calculated. The thorn can calculate geodesics either on the numerical spacetime, or on an exact spacetime (given by thorn Exact).
Created by swhite
Last modified 2005-08-04 07:05 PM
 

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