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ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 05/2011, Volume 732, Issue 2
The statistics of dark matter halos is an essential component of precision cosmology. The mass distribution of halos, as specified by the halo mass function,... 
INITIAL CONDITIONS | COLD DARK-MATTER | GRAVITATIONAL-INSTABILITY | MATTER POWER SPECTRUM | COSMIC STRUCTURE FORMATION | methods: numerical | COSMOLOGICAL CONSTRAINTS | N-BODY SIMULATIONS | PEAK-BACKGROUND SPLIT | ASTRONOMY & ASTROPHYSICS | LARGE-SCALE BIAS | large-scale structure of universe | PRECISION DETERMINATION
Journal Article
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2013, Volume 433, Issue 2, pp. 1573 - 1587
The nature of structure formation around the particle free streaming scale is still far from understood. Many attempts to simulate hot, warm and cold dark... 
Dark matter | Cosmology: theory | INITIAL CONDITIONS | GAUSSIAN FLUCTUATIONS | PROBE WMAP OBSERVATIONS | SUBHALOES | cosmology: theory | WARM DARK-MATTER | EVOLUTION | MODELS | ASTRONOMY & ASTROPHYSICS | TRANSIENTS | SIMULATIONS | UNIVERSE | dark matter | Physics - Cosmology and Nongalactic Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2017, Volume 465, Issue 1, pp. 105 - 105
We test the hypothesis that the initial mass function (IMF) is determined by the density probability distribution function (PDF) produced by supersonic... 
Turbulence | Turbulent flow | Symbols | Initial mass function | Star clusters | Density | Star formation rate | Probability density functions
Journal Article
Astrophysical Journal, ISSN 0004-637X, 09/2015, Volume 810, Issue 1, pp. 8 - 12
Journal Article