Smoothed particle hydrodynamics (SPH): an overview and recent developments

MB Liu, GR Liu - Archives of computational methods in engineering, 2010 - Springer
Smoothed particle hydrodynamics (SPH) is a meshfree particle method based on
Lagrangian formulation, and has been widely applied to different areas in engineering and …

Smoothed particle hydrodynamics in astrophysics

V Springel - Annual Review of Astronomy and Astrophysics, 2010 - annualreviews.org
This review discusses smoothed particle hydrodynamics (SPH) in the astrophysical context,
with a focus on inviscid gas dynamics. The particle-based SPH technique allows an intuitive …

[图书][B] Smoothed particle hydrodynamics: a meshfree particle method

GR Liu, MB Liu - 2003 - books.google.com
Page 1 Smoothed Particle Hydrodynamics a meshfree particle method GR Liu ↑ MB Liu Page
2 Page 3 1 Smoothed Particle Hydrodynamics a meshfree particle method This One …

Statistical properties of x-ray clusters: Analytic and numerical comparisons

GL Bryan, ML Norman - The Astrophysical Journal, 1998 - iopscience.iop.org
We compare the results of Eulerian hydrodynamic simulations of cluster formation against
virial scaling relations between four bulk quantities: the cluster mass, the dark matter velocity …

Cosmological smoothed particle hydrodynamics simulations: the entropy equation

V Springel, L Hernquist - Monthly Notices of the Royal …, 2002 - academic.oup.com
We discuss differences in simulation results that arise between the use of either the thermal
energy or the entropy as an independent variable in smoothed particle hydrodynamics …

Simulations of structure formation in the universe

E Bertschinger - Annual Review of Astronomy and Astrophysics, 1998 - annualreviews.org
▪ Abstract Cosmic structure has formed as a result of gravitational amplification of primordial
density fluctuations together with the action of other physical processes (adiabatic gas …

The santa barbara cluster comparison project: A comparison of cosmological hydrodynamics solutions

CS Frenk, SDM White, P Bode, JR Bond… - The Astrophysical …, 1999 - iopscience.iop.org
We have simulated the formation of an X-ray cluster in a cold dark matter universe using 12
different codes. The codes span the range of numerical techniques and implementations …

Versatile surface tension and adhesion for SPH fluids

N Akinci, G Akinci, M Teschner - ACM Transactions on Graphics (TOG), 2013 - dl.acm.org
Realistic handling of fluid-air and fluid-solid interfaces in SPH is a challenging problem. The
main reason is that some important physical phenomena such as surface tension and …

The history of the baryon budget-Cosmic logistics in a hierarchical universe

Y Rasera, R Teyssier - Astronomy & Astrophysics, 2006 - aanda.org
Using a series of high-resolution N-body hydrodynamical numerical simulations, we
investigate several scenarios for the evolution of the baryon budget in galactic halos. We …

Embedding Lagrangian sink particles in Eulerian grids

MR Krumholz, CF McKee, RI Klein - The Astrophysical Journal, 2004 - iopscience.iop.org
We introduce a new computational method for embedding Lagrangian sink particles into a
Eulerian calculation. Simulations of gravitational collapse or accretion generally produce …