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• W2098986009 endingPage "2757" @default.
• W2098986009 startingPage "2754" @default.
• W2098986009 abstract "We compute 3D models of supersonic, sub-Alfv'enic, and super-Alfv'enic decaying turbulence, with an isothermal equation of state appropriate for star-forming interstellar clouds of molecular gas. We find that in 3D the kinetic energy decays as ${t}^{ensuremath{-}ensuremath{eta}}$, with $0.85<ensuremath{eta}<1.2$. In 1D magnetized turbulence actually decays faster than unmagnetized turbulence. We compared different algorithms, and performed resolution studies reaching ${256}^{3}$ zones or ${70}^{3}$ particles. External driving must produce the observed long lifetimes and supersonic motions in molecular clouds, as undriven turbulence decays too fast." @default.
• W2098986009 created "2016-06-24" @default.
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• W2098986009 date "1998-03-30" @default.
• W2098986009 modified "2023-10-17" @default.
• W2098986009 title "Kinetic Energy Decay Rates of Supersonic and Super-Alfvénic Turbulence in Star-Forming Clouds" @default.
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• W2098986009 doi "https://doi.org/10.1103/physrevlett.80.2754" @default.
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