Transient large-scale dynamos in supernova progenitors

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

A large-scale, transient interface dynamo model is presented in the context of a supernova progenitor. Torodial and polodial field strengths are calculated at the boundary between the strong shear layer and the surrounding convective envelope. Dynamical shear is included and drained through field amplification and turbulent diffusion. For a 15 solar mass progenitor with varying outer shear layer rotation rates, we present a range of models which may provide enough energy to help power a supernova through poynting flux, viscous dissipation or a combination of both.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Transient large-scale dynamos in supernova progenitors does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Transient large-scale dynamos in supernova progenitors, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Transient large-scale dynamos in supernova progenitors will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1620082

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.