- Smoothed Particle Hydrodynamics and Magnetohydrodynamics Daniel J. Price
- Smoothed particle hydrodynamics and magnetohydrodynamics q Daniel J. Price
- Mon. Not. R. Astron. Soc. 000, 115 (2007) Printed 15 February 2007 (MN LATEX style file v2.2) The impact of magnetic fields on single and binary star formation
- SMOOTHED PARTICLESMOOTHED PARTICLESMOOTHED PARTICLESMOOTHED PARTICLESMOOTHED PARTICLESMOOTHED PARTICLESMOOTHED PARTICLESMOOTHED PARTICLESMOOTHED PARTICLESMOOTHED PARTICLE MAGNETOHYDRODYNAMICSMAGNETOHYDRODYNAMICSMAGNETOHYDRODYNAMICSMAGNETOHYDRODYNAMICSMAGN
- Mon. Not. R. Astron. Soc. 000, 116 (2010) Printed 14 February 2010 (MN LATEX style file v2.2) On the diffusive propagation of warps in thin accretion discs
- Mon. Not. R. Astron. Soc. 000, 125 (2009) Printed 20 October 2009 (MN LATEX style file v2.2) Smoothed Particle Magnetohydrodynamics IV -Using the Vector
- Mon. Not. R. Astron. Soc. 000, 1--26 (2004) Printed 5 September 2005 (MN L A T E X style file v2.2) Smoothed Particle Magnetohydrodynamics
- Mon. Not. R. Astron. Soc. 000, 000000 (0000) Printed 9 May 2007 (MN LATEX style file v2.2) MAGMA: a 3D, Lagrangian magnetohydrodynamics code for
- Modelling discontinuities and Kelvin-Helmholtz instabilities in SPH
- Computational Star Formation Proceedings IAU Symposium No. 270, 2010
- Discretization scheme for nonrelativistic equations The discretization scheme used in Chapter 2 for the nonrelativistic fluid equations is summarised in
- Mon. Not. R. Astron. Soc. 000, 1--13 (2006) Printed 30 October 2006 (MN L A T E X style file v2.2) An energyconserving formalism for adaptive gravitational
- ``I hope we get to the bottom of the answer. It's what I'm interested to GEORGE W. BUSH
- Variational Principles Relativistic SPH
- Mon. Not. R. Astron. Soc. 000, 116 (2009) Printed 10 May 2010 (MN LATEX style file v2.2) A comparison between grid and particle methods on the statistics of
- Mon. Not. R. Astron. Soc. 000, 116 (2007) Printed 15 January 2008 (MN LATEX style file v2.2) The effect of magnetic fields on star cluster formation
- Mon. Not. R. Astron. Soc. 401, 14751499 (2010) doi:10.1111/j.1365-2966.2009.15763.x Smoothed Particle Magnetohydrodynamics IV. Using the vector
- Mon. Not. R. Astron. Soc. 000, 1--16 (2005) Printed 25 October 2005 (MN L A T E X style file v2.2) Toy Stars in two dimensions
- Magnetic fields in Astrophysics Thesis submitted for the degree of
- Mon. Not. R. Astron. Soc. 339, 12231236 (2003) A comparison of the acceleration mechanisms in young stellar
- Mon. Not. R. Astron. Soc. 364, 384406 (2005) doi:10.1111/j.1365-2966.2005.09576.x Smoothed Particle Magnetohydrodynamics III. Multidimensional tests
- ``Part of the inhumanity of the computer is that, once it is competently programmed and working smoothly, it is completely honest.''
- Mon. Not. R. Astron. Soc. 000, 116 (0000) Magnetic fields and the dynamics of spiral galaxies
- ``The Americans, they always depend on a method what I call . . . stupid, silly. All I ask is check yourself. Do not in fact repeat their lies''
- Mon. Not. R. Astron. Soc. 000, 126 (2004) Printed 30 August 2005 (MN LATEX style file v2.2) Smoothed Particle Magnetohydrodynamics
- SPLASH: An interactive visualisation tool for Smoothed Particle Hydrodynamics simulations
- Magnetic fields and radiative feedback in the star formation process
- **FULL TITLE** ASP Conference Series, Vol. **VOLUME**, **YEAR OF PUBLICATION**
- Magnetic fields in Astrophysics Thesis submitted for the degree of
- "If I had only known, I would have been a locksmith." ALBERT EINSTEIN
- "I went on to test the program in every way I could devise. I strained it to expose its weaknesses. I ran it for high-mass stars and low-mass
- "Part of the inhumanity of the computer is that, once it is competently programmed and working smoothly, it is completely honest."
- "I hope we get to the bottom of the answer. It's what I'm interested to GEORGE W. BUSH
- BIBLIOGRAPHY Balbus, S. A. and J. F. Hawley: 1991, `A powerful local shear instability in weakly magnetized disks. I -
- Astronomy & Astrophysics manuscript no. turbulencepaper c ESO 2009 September 29, 2009
- Mon. Not. R. Astron. Soc. 000, 114 (2009) Printed 20 May 2009 (MN LATEX style file v2.2) Inefficient star formation: The combined effects of magnetic fields
- Astrophysics and Space Science DOI 10.1007/sXXXXX-XXX-XXXX-X
- Mon. Not. R. Astron. Soc. 000, 113 (2006) Printed 30 October 2006 (MN LATEX style file v2.2) An energy-conserving formalism for adaptive gravitational
- Mon. Not. R. Astron. Soc. 350, 14491456 (2004) doi:10.1111/j.1365-2966.2004.07748.x Toy stars in one dimension
- Mon. Not. R. Astron. Soc. 348, 139152 (2004) Smoothed Particle Magnetohydrodynamics II. Variational principles
- Variational principles for relativistic smoothed particle hydrodynamics J. J. MonaghanP
- Mon. Not. R. Astron. Soc. 000, 116 (2005) Printed 24 October 2005 (MN LATEX style file v2.2) Toy Stars in two dimensions
- Mon. Not. R. Astron. Soc. 000, 126 (2004) Printed 5 September 2005 (MN LATEX style file v2.2) Smoothed Particle Magnetohydrodynamics
- Discretization scheme for non-relativistic equations The discretization scheme used in Chapter 2 for the non-relativistic fluid equations is summarised in
- BIBLIOGRAPHY Balbus, S. A. and J. F. Hawley: 1991, `A powerful local shear instability in weakly magnetized disks. I
- Mon. Not. R. Astron. Soc. 000, 1{19 (2002) Printed 15 November 2002 (MN L A T E X style le v2.2) A comparison of the acceleration mechanisms in YSO and
- Mon. Not. R. Astron. Soc. 000, 17 (2011) Printed 9 June 2011 (MN LATEX style file v2.2) DUSTYBOX and DUSTYWAVE: Two test problems for numerical
- Mon. Not. R. Astron. Soc. 365, 9911006 (2006) doi:10.1111/j.1365-2966.2005.09783.x Toy Stars in two dimensions
- ``If I had only known, I would have been a locksmith.'' ALBERT EINSTEIN
- ``I never satisfy myself until I can make a mechanical model of a thing. If I can make a mechanical model I can understand it. As long as I cannot
- "I never satisfy myself until I can make a mechanical model of a thing. If I can make a mechanical model I can understand it. As long as I cannot
- Producing ultra-strong magnetic fields in neutron star D.J. Price1
- To appear in "Magnetic fields in the Universe II (2008)" RevMexAA(SC) MAGNETIC FIELDS IN STAR FORMATION: FROM GALAXIES TO STARS
- Mon. Not. R. Astron. Soc. 348, 123138 (2004) Smoothed Particle Magnetohydrodynamics I. Algorithm
- "The Americans, they always depend on a method what I call ...stupid, silly. All I ask is check yourself. Do not in fact repeat their lies"
- ``I went on to test the program in every way I could devise. I strained it to expose its weaknesses. I ran it for highmass stars and lowmass
- Variational Principles for
- **Volume Title** ASP Conference Series, Vol. **Volume Number**
- Mon. Not. R. Astron. Soc. 000, 119 (2011) Printed 14 November 2011 (MN LATEX style file v2.2) Dusty gas with SPH --I. Algorithm and test suite
- Mon. Not. R. Astron. Soc. 000, L1L5 (2011) Printed 30 November 2011 (MN LATEX style file v2.2) Resolving high Reynolds numbers in SPH simulations of subsonic
- Mon. Not. R. Astron. Soc. 000, 112 (2011) Printed 14 November 2011 (MN LATEX style file v2.2) Dusty gas with SPH --II. Implicit timestepping and astrophysical
- Constrained Hyperbolic Divergence Cleaning for Smoothed Particle Magnetohydrodynamics
