Matteo Cantiello edited SETTING_UP_FOR_THE_PRESENTATION__.tex  almost 9 years ago

Commit id: eef726f63da137ca7bebc9fbfd25d2dc6b92e27e

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%only tentative conclusions that this phenomona probably concerns stars  %more massive than 1.3\msol for which strong coupling between envelope and  %core modes would increase the mode mass, reducing the observed amplitude.]   Recent theoretical work has shown that the $\ell =1 $ modes suppression can be explained if waves entering the core are prevented from returning to the envelope. This occurs in the presence of strong magnetic fields, which give rise to a ``magnetic greenhouse'' effect, efficiently trapping the  wave energy tunneling that tunnels  into the stellar core (Fuller et al. 2015). %and provides a mechanism that can cause such an effect in the  %presence of a strong core magnetic field near the hydrogen-burning shell[ref