Speaker
Alessandro Mirizzi
Description
Stars have been recognized as optimal laboratories to probe axion properties. In the last decades there have been significant advances in this field due to a better modelling of stellar systems and accurate observational data. In this talk I review the current status of constraints on axions from stellar physics and present the future perspectives. The focus is i on the Sun, globular cluster stars, white dwarfs and (proto)-neutron stars.
https://cern.zoom.us/j/62219760813?pwd=cgiDpf7DPkV3kmb9xVTqvTV1p1a7kX.1