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Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2015, Volume 450, Issue 1, pp. 53 - 110
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2013, Volume 428, Issue 4, pp. 2840 - 2856
Various formulations of smoothed particle hydrodynamics (SPH) have been proposed, intended to resolve certain difficulties in the treatment of fluid mixing... 
Hydrodynamics | Turbulence | Cosmology: theory | Instabilities | Methods: numerical | GALAXY-FORMATION | STABILITY | STAR-FORMATION | hydrodynamics | SPH | turbulence | methods: numerical | instabilities | cosmology: theory | KELVIN-HELMHOLTZ INSTABILITIES | CLOUDS | ASTRONOMY & ASTROPHYSICS | GAS | SIMULATIONS | FEEDBACK
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 04/2017, Volume 466, Issue 3, p. 3387
  We extend recently developed mesh-free Lagrangian methods for numerical magnetohydrodynamics (MHD) to arbitrary anisotropic diffusion equations, including:... 
Viscosity | Fluid mechanics | Anisotropy | Magnetism | Diffusion | Astronomy
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 04/2017, Volume 466, Issue 3, pp. 3387 - 3387
We extend recently developed mesh-free Lagrangian methods for numerical magnetohydrodynamics (MHD) to arbitrary anisotropic diffusion equations, including:... 
Turbulent flow | Magnetohydrodynamic turbulence | Anisotropy | Mathematical analysis | Meshless methods | Diffusion effects | Mathematical models | Diffusion
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 10/2019, Volume 489, Issue 1, pp. 325 - 338
We study the non-linear evolution of the acoustic 'resonant drag instability' (RDI) using numerical simulations. The acoustic RDI is excited in a dust-gas... 
SOLID PARTICLES | ISM: kinematics and dynamics | ISOTROPIC TURBULENCE | STREAMING INSTABILITY | turbulence | instabilities | galaxies: formation | GRAINS | DISKS | ASTRONOMY & ASTROPHYSICS | DYNAMICS | GAS | NUMERICAL SIMULATIONS | planets and satellites: formation | MODULATION
Journal Article
Nature, ISSN 0028-0836, 12/2014, Volume 516, Issue 729, pp. 44 - 45
According to the simplest cosmological models, nearly all the baryonic matter - the 'normal' matter in the Universe - should sit at the centres of galaxies in... 
Wind | Universe | Cosmology | Supernovae | Star & galaxy formation | Stars & galaxies
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2016, Volume 455, Issue 1, pp. 89 - 89
We propose a simple model for density fluctuations of aerodynamic grains, embedded in a turbulent, gravitating gas disc. The model combines a calculation for... 
Turbulence | Turbulent flow | Computational fluid dynamics | Grains | Mathematical analysis | Fluctuation | Mathematical models | Density
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2016, Volume 455, Issue 1, p. 89
  We propose a simple model for density fluctuations of aerodynamic grains, embedded in a turbulent, gravitating gas disc. The model combines a calculation for... 
Phenomenology | Turbulence | Simulation | Grain | Experiments | Density
Journal Article
Physics Today, ISSN 0031-9228, 04/2017, Volume 70, Issue 4, pp. 70 - 71
Perhaps the oldest question confronted by humanity is, "Where do we come from?" Philosophers pondered the issue thousands of years ago, and many people... 
PHYSICS, MULTIDISCIPLINARY
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2016, Volume 462, Issue 1, p. 576
  In numerical magnetohydrodynamics (MHD), a major challenge is maintaining ...-B=0. Constrained transport (CT) schemes achieve this but have been restricted... 
Fluid mechanics | Star & galaxy formation | Astronomy | Convergence
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2016, Volume 462, Issue 1, pp. 576 - 576
In numerical magnetohydrodynamics (MHD), a major challenge is maintaining ...-B=0. Constrained transport (CT) schemes achieve this but have been restricted to... 
Reconstruction | Errors | Magnetohydrodynamics | Constraints | Meshless methods | MHD | Mathematical models | Cleaning
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 09/2019, Volume 488, Issue 2, pp. 2970 - 2975
Most simulations of galaxies and massive giant molecular clouds (GMCs) cannot explicitly resolve the formation (or predict the main-sequence masses) of... 
SYSTEM | WINDS | CLUSTER FORMATION | DEPENDENCE | stars: formation | galaxies: formation | PRESSURE | DISRUPTION | COLLAPSE | SIMULATING RADIATIVE FEEDBACK | ASTRONOMY & ASTROPHYSICS | stars: massive | ACCRETION | ISM: clouds | GALAXIES
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 09/2019, Volume 882, Issue 1, p. 46
Galaxies covering several orders of magnitude in stellar mass and a variety of Hubble types have been shown to follow the radial acceleration relation (RAR), a... 
ASTRONOMY & ASTROPHYSICS | galaxies: fundamental parameters | DARK-MATTER | galaxies: kinematics and dynamics | GALAXIES | MODEL | STELLAR MASS
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 05/2019, Volume 485, Issue 3, pp. 3991 - 3998
We investigate, for the first time, the non-linear evolution of the magnetized 'resonant drag instabilities' (RDIs). We explore magnetohydrodynamic simulations... 
PROTOPLANETARY | ISM: kinematics and dynamics | VISCOSITY | turbulence | accretion, accretion discs | instabilities | GRADIENT | cosmology: theory | DUST | AMPLIFICATION | ASTRONOMY & ASTROPHYSICS | SOLAR | DYNAMICS | PLANETESIMAL FORMATION | INTERSTELLAR TURBULENCE | planets and satellites: formation
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2016, Volume 456, Issue 3, pp. 2383 - 2383
In a turbulent proto-planetary disc, dust grains undergo large-density fluctuations and under the right circumstances, grain overdensities can collapse under... 
Grains | Planet formation | Fluctuation | Gravitational collapse | Disks | Mathematical models | Formations | Density
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2016, Volume 456, Issue 3, p. 2383
  In a turbulent proto-planetary disc, dust grains undergo large-density fluctuations and under the right circumstances, grain overdensities can collapse under... 
Dust | Astronomy | Gravity
Journal Article
Nature, ISSN 0028-0836, 12/2014, Volume 516, Issue 7529, pp. 44 - 45
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2013, Volume 430, Issue 3, pp. 1653 - 1693
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 06/2016, Volume 459, Issue 1, p. 9
  Turbulence is thought to be a primary driving force behind the early stages of star formation. In this framework large, self-gravitating, turbulent clouds... 
Turbulence | Astrophysics | Clouds | Temperature effects | Star & galaxy formation | Protostars | Gravity
Journal Article
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