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Small‐Scale Interaction of Turbulence with Thermonuclear Flames in Type Ia Supernovae
Author(s) -
J. C. Niemeyer,
W. K. Bushe,
G. R. Ruetsch
Publication year - 1999
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/307813
Subject(s) - laminar flow , turbulence , physics , thermonuclear fusion , supernova , mechanics , flame speed , detonation , laminar flame speed , deflagration , context (archaeology) , premixed flame , astrophysics , chemistry , plasma , explosive material , combustion , nuclear physics , geology , combustor , organic chemistry , paleontology
Microscopic turbulence-flame interactions of thermonuclear fusion flamesoccuring in Type Ia Supernovae were studied by means of incompressible directnumerical simulations with a highly simplified flame description. The flame istreated as a single diffusive scalar field with a nonlinear source term. It ischaracterized by its Prandtl number, Pr << 1, and laminar flame speed, S_L. Wefind that if S_L ~ u', where u' is the rms amplitude of turbulent velocityfluctuations, the local flame propagation speed does not significantly deviatefrom S_L even in the presence of velocity fluctuations on scales below thelaminar flame thickness. This result is interpreted in the context ofsubgrid-scale modeling of supernova explosions and the mechanism fordeflagration-detonation-transitions.Comment: 8 pages, 6 figures, accepted by Astrophys.

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