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Convective Overshoot Daniel Lecoanet Josiah Schwab, Eliot Quataert - PowerPoint PPT Presentation

The Turbulent Diffusivity of Convective Overshoot Daniel Lecoanet Josiah Schwab, Eliot Quataert Lars Bildsten, Frank Timmes Geoff Vasil, Keaton Burns Jeff Oishi, Ben Brown Supported by: NSF, Hertz Foundation, NASA, ARC The problem Stably


  1. The Turbulent Diffusivity of Convective Overshoot Daniel Lecoanet Josiah Schwab, Eliot Quataert Lars Bildsten, Frank Timmes Geoff Vasil, Keaton Burns Jeff Oishi, Ben Brown Supported by: NSF, Hertz Foundation, NASA, ARC

  2. The problem Stably stratified Convection

  3. The problem Stably stratified Convection

  4. The problem how much Stably stratified mix ixing? what kin ind? Convection

  5. Super Asymptotic Giant Branch stars H MS

  6. Super Asymptotic Giant Branch stars H He MS RGB

  7. Super Asymptotic Giant Branch stars H He CO MS RGB AGB

  8. Super Asymptotic Giant Branch stars H He CO MS RGB AGB

  9. Super Asymptotic Giant Branch stars H He CO MS RGB AGB SAGB

  10. Frank Timmes Flame Carbon Temperature Density Energy Generation Inner star Outer star

  11. Farmer+ 2015

  12. Does flame reach center??? Farmer+ 2015

  13. Does flame reach center??? Yes: ONe core e - capture SNe SNe II-P Farmer+ 2015

  14. Does flame reach center??? Yes: No: ONe core ``Hybrid’’ WD e - capture SNe SNe Ia? SNe II-P ??? Farmer+ 2015

  15. Carbon Flames

  16. Carbon Flames

  17. Carbon Flames flame dies

  18. Carbon Flames flame dies flame is fine

  19. Carbon Flames flame dies flame is fine

  20. Carbon Flames Properties

  21. Carbon Flames Properties

  22. Carbon Flames Properties

  23. Carbon Flames Model

  24. Carbon Flames Model negative in conv VERY positive in flame

  25. Carbon Flames Model

  26. Carbon Flames Model BC’s: no slip, no temperature perturbation 3D domain, 4H x 4H x 2H

  27. Carbon Flames Model BC’s: no slip, no temperature perturbation 3D domain, 4H x 4H x 2H

  28. Carbon Flames Properties

  29. Carbon Flames Properties

  30. Dedalus Pseudo-spectral Open-source Pyth ython ** Very ry fl flexible equations **

  31. The team so far Daniel Lecoanet (Berkeley) Keaton Burns (MIT) Jeff Oishi (Bates College) Ben Brown (Colorado) Geoff Vasil (Sydney)

  32. flame

  33. Passive Scalar Field

  34. Passive Scalar Field

  35. Passive Scalar Field

  36. Passive Scalar Field

  37. Passive Scalar Field Ansatz:

  38. Passive Scalar Field

  39. Turbulent Diffusivity

  40. Turbulent Diffusivity Solve: Does it work?

  41. Turbulent Diffusivity Solve: Does it work? fit

  42. Turbulent Diffusivity Solve: Turbulent diffusivity is a good approximation!

  43. Do Carbon Flames Mix? Need deep within the flame

  44. Conclusion 1. Penetrative convection mixes fluid like a turbulent diffusivity 2. Very little mixing in regions which are very stable 3. Convective overshoot probably can’t stall flames

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