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% If you are using CVS use this line to give version information
% $Header$

\documentclass{article}

% Use the Cactus ThornGuide style file
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\begin{document}

% The author of the documentation
\author{Frank Löffler}

% The title of the document (not necessarily the name of the Thorn)
\title{ADMMass}

% the date your document was last changed, if your document is in CVS,
% please use:
%    \date{$ $Date: 2004-01-07 14:12:39 -0600 (Wed, 07 Jan 2004) $ $}
\date{2012-05-07}

\maketitle

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% Add all definitions used in this documentation here
%   \def\mydef etc

% Add an abstract for this thorn's documentation
\begin{abstract}
Thorn ADMMass can compute the ADM mass from quantities in ADMBase.
\end{abstract}

% The following sections are suggestive only.
% Remove them or add your own.

\section{Introduction}
The ADM mass evaluated as either surface integrals at infinity or volume
integrals over entire hypersurfaces give a measure of the total energy in the
spacetime.

 The ADM mass can be defined~\cite{ADM_mass_Omurchadha74} as a surface integral over a
 sphere with infinite radius:
 \begin{equation}
 \label{eq:ADM_mass}
  M_{\mbox{\tiny ADM}}=\frac{1}{16\pi}\oint_\infty
  \sqrt{\gamma}\gamma^{ij}\gamma^{kl}
  (\gamma_{ik,j}-\gamma_{ij,k})\text{d}\! S_l
 \end{equation}.
 This is, assuming $\alpha=1$ at infinity, equivalent to
 \begin{equation}
 \label{eq:ADM_mass_volume}
  M_{\mbox{\tiny ADM}}=\frac{1}{16\pi}\int
  \left(\alpha\sqrt{\gamma}\gamma^{ij}\gamma^{kl}
  (\gamma_{ik,j}-\gamma_{ij,k})\right)_{,l}\text{d}\!^{\,3}\!\!x
 \end{equation}.
In practice, the following equation can also be used within the thorn:
  \begin{equation}
   \label{eq:ADM_mass_lapse}
   M_{\mbox{\tiny ADM}}=\frac{1}{16\pi}\oint_\infty
   \alpha\sqrt{\gamma}\gamma^{ij}\gamma^{kl}
   (\gamma_{ik,j}-\gamma_{ij,k})\text{d}\! S_l.
  \end{equation}
  This differs from equation~(\ref{eq:ADM_mass}) by the factor $\alpha$ inside
  the integral. For evaluations of those equations at infinity, $\alpha=1$ is
  assumed, and they are equal. For evaluations at a finite distance, however,
  this is usually not the case and the approximation of the ADM mass is
  gauge-dependent~\cite{ADM_mass_Omurchadha74}. Depending on circumstances,
  either~(\ref{eq:ADM_mass}),~(\ref{eq:ADM_mass_lapse} or~~(\ref{eq:ADM_mass_volume})
  might give better results.

\section{Using This Thorn}

Multiple measurements can be done for both volume and surface integral, but the
limit for both is 100 (change param.ccl if you need more). You need to
specify the number of integrations with \texttt{ADMMass\_number} (and ADMMass
will perform both integrations that many times).

Also note that this thorn uses the ADMMacros for derivatives. Thus, converegence
of results is limited to the order of these derivatives (ADMMacros::spatial\_order).

ADMMass provides several possibilities to specify the (finite) integration domain,
both for surface and volume integral, which we list in the following:

\begin{itemize}
 \item Surface Integral (over rectangular domain)
  \begin{itemize}
   \item \texttt{ADMMass\_distance\_from\_grid\_boundary}: specifies the distance
         between the physical domain boundary and the integration domain. If
         this is set, this fully specifies the domain boundary.
   \item \texttt{ADMMass\_surface\_distance}: specifies a distance of the integration
         boundary from a given point, specified using \texttt{ADMMass\_x\_pos[3]}.
   \item Otherwise, \texttt{ADMMass\_[xyz]\_[min|max]} specify a rectangular
         integration domain.
  \end{itemize}
 \item Volume Integral (over sphere)
  \begin{itemize}
   \item If \texttt{ADMMass\_use\_all\_volume\_as\_volume\_radius} is set,
         the whole volume is used for integration.
   \item If \texttt{ADMMass\_use\_surface\_distance\_as\_volume\_radius} is set
         and \texttt{ADMMass\_volume\_radius} is not (negative),
         \texttt{ADMMass\_surface\_distance} is used to specify the integration
         radius.
   \item Otherwise, \texttt{ADMMass\_volume\_radius} specifies this radius.
   \item \texttt{ADMMass\_[xyz]\_pos} specify the position of the integration
         sphere.
   \item Use \texttt{ADMMass\_Excise\_Horizons} to exclude domains where
         thorn \texttt{OutsideMask} didn't specify domain as \texttt{outside}.
         This can be used to, e.g. excise black hole apparent horizons.
  \end{itemize}
\end{itemize}

You should output \texttt{ADMMass::ADMMass\_Masses} for the result of the
integrations, which will include the results for the volume integral, the
usual surface integral and the sorface integral including the lapse.

\begin{thebibliography}{1}
\bibitem{ADM_mass_Omurchadha74}
N.~O Murchadha and J.~W.~York,
  ``Gravitational energy,''
  Phys.\ Rev.\ D {\bf 10}, 2345 (1974).
  doi:10.1103/PhysRevD.10.2345
  %%CITATION = doi:10.1103/PhysRevD.10.2345;%%  %%CITATION = doi:10.1103/PhysRevD.10.428;%%
\end{thebibliography}

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\end{document}

