http://arxiv.org/abs/1907.06928
We consider the poorly studied before non-diffusive energy transport solutions to the solar abundance problem. We find the additional energy flux inside the Sun required to reconcile the Standard solar model with helioseismology. An example of an extension of the Standard model is suggested which can provide for this flux.
A. Sokolov
Wed, 17 Jul 19
52/75
Comments: N/A
You must be logged in to post a comment.