Test of stellar hydrodynamics predictions
Test of stellar hydrodynamics predictions
Test of stellar hydrodynamics predictions
Create successful ePaper yourself
Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.
Summary<br />
SN Ia: Binary white dwarf mergers: shear and turbulence<br />
Unequal masses: no evidence for prompt ignition<br />
Equal masses: no evidence for prompt ignition<br />
Expect central ignitions with fast rotating envelopes<br />
Likely different from typical models with smooth rotation<br />
Perhaps similar to Yoon & Langer structure<br />
Shear/KHI HED studied and analyzed; HED turbulence experiment concept developed<br />
SN Ia: In-situ generated magnetic fields for Type Ia deflagrations<br />
Identified as a possible new physics in HED RTI experiments<br />
For supernova conditions, reduced turbulence near the flame<br />
Smoother flame surface<br />
Lower effective flame speed, large scales more important<br />
Flame remains RT-driven and mushroom-like in appearance<br />
SN II: Core-collapse<br />
Exploring possible SASI experimental designs<br />
SASI asymmetries may suffice to explain SN 1987A and alikes<br />
Crab-like spongy morphologies for young ccSNR<br />
Diverging SNRT to be executed on NIF!<br />
April 26, 2011<br />
46
Change language