15th Patras Workshop on Axions, WIMPs and WISPs

WISP solutions to the solar abundance problem: general requirements and an example

6 Jun 2019, 10:15

20m

Main Lecture Hall (Physics Department)

Oral Morning 41

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.

Presentation materials

Slides

11_4__Sokolov.pdf