Closed-form expressions for particle relative velocities induced by turbulence (Research Note)

C. W. Ormel*, J. N. Cuzzi

*Corresponding author for this work

Research output: Contribution to journalArticleAcademicpeer-review

336 Citations (Scopus)
106 Downloads (Pure)

Abstract

In this note we present complete, closed-form expressions for random relative velocities between colliding particles of arbitrary size in nebula turbulence. These results are exact for very small particles ( those with stopping times much shorter than the large eddy overturn time) and are also surprisingly accurate in complete generality ( that is, also apply for particles with stopping times comparable to, or much longer than, the large eddy overturn time). We note that some previous studies may have adopted previous simple expressions, which we find to be in error regarding the size dependence in the large particle regime.

Original languageEnglish
Pages (from-to)413-420
Number of pages8
JournalAstronomy & Astrophysics
Volume466
Issue number2
DOIs
Publication statusPublished - May-2007

Keywords

  • turbulence
  • dust,extinction
  • planetary systems : protoplanetary disks
  • PROTOPLANETARY DISKS
  • DUST COAGULATION
  • SOLAR NEBULA
  • GRAINS
  • EVOLUTION
  • GROWTH
  • GAS

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