Speaker
Mr
Anton Sokolov
(INR RAS)
Description
We consider the poorly studied before non-diffusive energy transport solutions to the solar abundance problem. We find the luminous flux change inside the Sun required to reconcile the Standard solar model with helioseismology. An example of a WISP extension of the Standard model is suggested which can alleviate the discrepancies.
Primary author
Mr
Anton Sokolov
(INR RAS)
