Commit 2b8d1469 authored by Josh Borrow's avatar Josh Borrow
Browse files

removed abstracts no longer used

parent d7a1830c
......@@ -34,12 +34,14 @@ archivePrefix = "arXiv",
@ARTICLE{Hopkins2013,
author = {{Hopkins}, P.~F.},
title = "{A general class of Lagrangian smoothed particle hydrodynamics methods and implications for fluid mixing problems}",
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},
keywords = {hydrodynamics, instabilities, turbulence, methods: numerical,
cosmology: theory},
year = 2013,
month = feb,
volume = 428,
......@@ -51,10 +53,12 @@ archivePrefix = "arXiv",
@ARTICLE{Springel2002,
author = {{Springel}, V. and {Hernquist}, L.},
title = "{Cosmological smoothed particle hydrodynamics simulations: the entropy equation}",
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},
keywords = {methods: numerical, galaxies: evolution, galaxies: starburst,
methods: numerical, galaxies: evolution, galaxies: starburst},
year = 2002,
month = jul,
volume = 333,
......@@ -66,7 +70,8 @@ archivePrefix = "arXiv",
@ARTICLE{Balsara1995,
author = {{Balsara}, D.~S.},
title = "{von Neumann stability analysis of smooth particle hydrodynamics--suggestions for optimal algorithms}",
title = "{von Neumann stability analysis of smooth particle
hydrodynamics--suggestions for optimal algorithms}",
journal = {Journal of Computational Physics},
year = 1995,
volume = 121,
......@@ -81,11 +86,13 @@ archivePrefix = "arXiv",
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}",
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},
keywords = {methods: numerical, galaxies: clusters: intracluster medium,
galaxies: formation, cosmology: theory},
year = 2015,
month = dec,
volume = 454,
......@@ -100,7 +107,8 @@ archivePrefix = "arXiv",
@ARTICLE{Dehnen2012,
author = {{Dehnen}, W. and {Aly}, H.},
title = "{Improving convergence in smoothed particle hydrodynamics simulations without pairing instability}",
title = "{Improving convergence in smoothed particle hydrodynamics simulations
without pairing instability}",
journal = {\mnras},
archivePrefix = "arXiv",
eprint = {1204.2471},
......@@ -118,7 +126,6 @@ archivePrefix = "arXiv",
@article{Saitoh2013,
abstract = {In the standard formulation of the smoothed particle hydrodynamics (SPH), it is assumed that the local density distribution is differentiable. This assumption is used to derive the spatial derivatives of other quantities. However, this assumption breaks down at the contact discontinuity, which appears often in simulations of astronomical objects. At the contact discontinuity, the density of the low-density side is overestimated while that of the high-density side is underestimated. As a result, the pressure of the low (high) density side is over (under) estimated. Thus, unphysical repulsive force appears at the contact discontinuity, resulting in the effective surface tension. This effective surface tension suppresses instabilities such as the Kelvin-Helmholtz and Rayleigh-Taylor instabilities. In this paper, we present a new formulation of SPH, which does not require the differentiability of density and thus can handle contact discontinuity without numerical problems. The results of standard tests such as the shock tube, Kelvin-Helmholtz and Rayleigh-Taylor instabilities, and the blob tests are all very favorable to our new formulation. We conclude that our new formulation solved practically all known difficulties of the standard SPH, without introducing additional numerical diffusion or breaking the exact force symmetry or energy conservation.},
archivePrefix = {arXiv},
arxivId = {1202.4277},
author = {Saitoh, Takayuki R. and Makino, Junichiro},
......@@ -130,7 +137,8 @@ issn = {15384357},
journal = {Astrophysical Journal},
keywords = {galaxies: ISM,galaxies: evolution,methods: numerical},
number = {1},
title = {{A density-independent formulation of smoothed particle hydrodynamics}},
title = {{A density-independent formulation of smoothed particle
hydrodynamics}},
volume = {768},
year = {2013}
}
......@@ -138,7 +146,6 @@ year = {2013}
@article{Hosono2013,
abstract = {The smoothed particle hydrodynamics (SPH) method is a useful numerical tool for the study of a variety of astrophysical and planetlogical problems. However, it turned out that the standard SPH algorithm has problems in dealing with hydrodynamical instabilities. This problem is due to the assumption that the local density distribution is differentiable. In order to solve this problem, a new SPH formulation, which does not require the differentiability of the density, have been proposed. This new SPH method improved the treatment of hydrodynamical instabilities. This method, however, is applicable only to the equation of state (EOS) of the ideal gas. In this paper, we describe how to extend the new SPH method to non-ideal EOS. We present the results of various standard numerical tests for non-ideal EOS. Our new method works well for non-ideal EOS. We conclude that our new SPH can handle hydrodynamical instabilities for an arbitrary EOS and that it is an attractive alternative to the standard SPH.},
archivePrefix = {arXiv},
arxivId = {1307.0916},
author = {Hosono, Natsuki and Saitoh, Takayuki R. and Makino, Junichiro},
......@@ -149,8 +156,10 @@ issn = {0004-6264},
keywords = {hydrodynamics,methods,numerical},
number = {May},
pages = {1--11},
title = {{Density Independent Smoothed Particle Hydrodynamics for Non-Ideal Equation of State}},
url = {http://arxiv.org/abs/1307.0916{\%}0Ahttp://dx.doi.org/10.1093/pasj/65.5.108},
title = {{Density Independent Smoothed Particle Hydrodynamics for Non-Ideal
Equation of State}},
url =
{http://arxiv.org/abs/1307.0916{\%}0Ahttp://dx.doi.org/10.1093/pasj/65.5.108},
year = {2013}
}
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