The detailed modeling of the solar interior has been in crisis for more than 15 years so far, after the development of 3D models of solar atmospheres. Turning a crisis into an opportunity, this has led to revision of the paradigm of the standard solar model as a framework for modeling the Sun (and other stars) as well as the microscopic physics involved. In this talk, Prof. Serenelli will discuss the latest results on helioseismology, solar neutrinos and solar modeling, placing them in the context of the solar modeling crisis. Regarding the microphysics, he will present the latest advances in the determination of radiative opacities.
Time: Wednesday, April 28, 2021, 17:00 CEST (st!)
Meeting: https://unigraz.webex.com/meet/paul.beck