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Matteo Cantiello edited figures/integral_1.6/caption.tex
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Fraction of mode energy reflected at the bottom of the acoustic cavity for a 1.6$\mso$ star ascending the red giant branch (decreasing $\nu_{max}$). The lines show values for modes with $\ell=1$ and
$\ell=1$ $\ell=2$ and their ratio.
The degree of reflection is determined by the tunneling integral through the evanescent region as $1-T^2$, where the tunneling integral $T$ is defined in Eq.~\ref{Eq:integral}. The range of values for the fraction of $\ell=1$ mode energy reflected during core He-burning is also shown (hatched region).