Commit 3e463812 authored by Matthieu Schaller's avatar Matthieu Schaller
Browse files

Added general SPH theory file and EoS description

parent a4ac9d6d
......@@ -84,6 +84,8 @@ theory/SPH/Kernels/kernels.pdf
theory/SPH/Kernels/kernel_derivatives.pdf
theory/SPH/Kernels/kernel_definitions.pdf
theory/SPH/Flavours/sph_flavours.pdf
theory/SPH/EoS/eos.pdf
theory/SPH/*.pdf
theory/paper_pasc/pasc_paper.pdf
m4/libtool.m4
......
\documentclass[fleqn, usenatbib, useAMS,a4paper]{mnras}
\usepackage{graphicx}
\usepackage{amsmath,paralist,xcolor,xspace,amssymb}
\usepackage{times}
\newcommand{\swift}{{\sc Swift}\xspace}
%opening
\title{Equation of state in SWIFT}
\author{Matthieu Schaller}
\begin{document}
\maketitle
\input{eos}
\bibliographystyle{mnras}
\bibliography{./bibliography.bib}
\end{document}
#!/bin/bash
python kernels.py
pdflatex -jobname=eos eos_standalone.tex
bibtex eos.aux
pdflatex -jobname=eos eos_standalone.tex
pdflatex -jobname=eos eos_standalone.tex
@ARTICLE{Price2012,
author = {{Price}, D.~J.},
title = "{Smoothed particle hydrodynamics and magnetohydrodynamics}",
journal = {Journal of Computational Physics},
archivePrefix = "arXiv",
eprint = {1012.1885},
primaryClass = "astro-ph.IM",
year = 2012,
month = feb,
volume = 231,
pages = {759-794},
doi = {10.1016/j.jcp.2010.12.011},
adsurl = {http://adsabs.harvard.edu/abs/2012JCoPh.231..759P},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Springel2005,
author = {{Springel}, V.},
title = "{The cosmological simulation code GADGET-2}",
journal = {\mnras},
eprint = {astro-ph/0505010},
keywords = {methods: numerical, galaxies: interactions, dark matter},
year = 2005,
month = dec,
volume = 364,
pages = {1105-1134},
doi = {10.1111/j.1365-2966.2005.09655.x},
adsurl = {http://adsabs.harvard.edu/abs/2005MNRAS.364.1105S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Hopkins2013,
author = {{Hopkins}, P.~F.},
title = "{A general class of Lagrangian smoothed particle hydrodynamics methods and implications for fluid mixing problems}",
journal = {\mnras},
archivePrefix = "arXiv",
eprint = {1206.5006},
primaryClass = "astro-ph.IM",
keywords = {hydrodynamics, instabilities, turbulence, methods: numerical, cosmology: theory},
year = 2013,
month = feb,
volume = 428,
pages = {2840-2856},
doi = {10.1093/mnras/sts210},
adsurl = {http://adsabs.harvard.edu/abs/2013MNRAS.428.2840H},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Springel2002,
author = {{Springel}, V. and {Hernquist}, L.},
title = "{Cosmological smoothed particle hydrodynamics simulations: the entropy equation}",
journal = {\mnras},
eprint = {astro-ph/0111016},
keywords = {methods: numerical, galaxies: evolution, galaxies: starburst, methods: numerical, galaxies: evolution, galaxies: starburst},
year = 2002,
month = jul,
volume = 333,
pages = {649-664},
doi = {10.1046/j.1365-8711.2002.05445.x},
adsurl = {http://adsabs.harvard.edu/abs/2002MNRAS.333..649S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Balsara1995,
author = {{Balsara}, D.~S.},
title = "{von Neumann stability analysis of smooth particle hydrodynamics--suggestions for optimal algorithms}",
journal = {Journal of Computational Physics},
year = 1995,
volume = 121,
pages = {357-372},
doi = {10.1016/S0021-9991(95)90221-X},
adsurl = {http://adsabs.harvard.edu/abs/1995JCoPh.121..357B},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Schaller2015,
author = {{Schaller}, M. and {Dalla Vecchia}, C. and {Schaye}, J. and
{Bower}, R.~G. and {Theuns}, T. and {Crain}, R.~A. and {Furlong}, M. and
{McCarthy}, I.~G.},
title = "{The EAGLE simulations of galaxy formation: the importance of the hydrodynamics scheme}",
journal = {\mnras},
archivePrefix = "arXiv",
eprint = {1509.05056},
keywords = {methods: numerical, galaxies: clusters: intracluster medium, galaxies: formation, cosmology: theory},
year = 2015,
month = dec,
volume = 454,
pages = {2277-2291},
doi = {10.1093/mnras/stv2169},
adsurl = {http://adsabs.harvard.edu/abs/2015MNRAS.454.2277S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Dehnen2012,
author = {{Dehnen}, W. and {Aly}, H.},
title = "{Improving convergence in smoothed particle hydrodynamics simulations without pairing instability}",
journal = {\mnras},
archivePrefix = "arXiv",
eprint = {1204.2471},
primaryClass = "astro-ph.IM",
keywords = {hydrodynamics, methods: numerical },
year = 2012,
month = sep,
volume = 425,
pages = {1068-1082},
doi = {10.1111/j.1365-2966.2012.21439.x},
adsurl = {http://adsabs.harvard.edu/abs/2012MNRAS.425.1068D},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
#!/bin/bash
cd Kernels
python kernels.py
cp kernels.pdf ..
cp kernel_derivatives.pdf ..
cd ..
pdflatex swift_sph.tex
bibtex swift_sph.aux
pdflatex swift_sph.tex
pdflatex swift_sph.tex
\documentclass[fleqn, usenatbib, useAMS]{mnras}
\usepackage{graphicx}
\usepackage{amsmath,paralist,xcolor,xspace,amssymb}
\usepackage{times}
\usepackage[super]{nth}
\newcommand{\swift}{{\sc swift}\xspace}
\newcommand{\gadget}{{\sc gadget}\xspace}
\newcommand{\dd}[2]{\frac{\partial #1}{\partial #2}}
\renewcommand{\vec}[1]{{\mathbf{#1}}}
\newcommand{\Wij}{\overline{\nabla_xW_{ij}}}
\newcommand{\tbd}{\textcolor{red}{TO BE DONE}}
\newcommand{\MinimalSPH}{\textsc{minimal-sph}\xspace}
\newcommand{\GadgetSPH}{\textsc{gadget-sph}\xspace}
\newcommand{\PESPH}{\textsc{pe-sph}\xspace}
%\setlength{\mathindent}{0pt}
%opening
\title{SPH implementation in \swift}
\author{Matthieu Schaller}
\begin{document}
\maketitle
\section{Kernel functions}
\input{Kernels/kernel_definitions}
\section{Equation of state}
\input{EoS/eos}
\section{SPH flavours}
\input{Flavours/sph_flavours}
\bibliographystyle{mnras}
\bibliography{./bibliography}
\end{document}
Supports Markdown
0% or .
You are about to add 0 people to the discussion. Proceed with caution.
Finish editing this message first!
Please register or to comment