M. S. Cunha, D. Stello, P. P. Avelino, J. Christensen-Dalsgaard
Abstract
In this work we consider the sensitivity of gravity-mode period spacings to sharp changes in the inner structure of red giant stars, more specifically in the buoyancy frequency inside the g-mode propagation cavity. Based on a comparison between the solutions to the linear pulsation equations in the Cowling approximation for pure g-modes with results obtained with a full oscillation code we identify and correctly interpret the signature of the above-mentioned sharp variations in the period spacings. Two examples, of red giant models in different evolutionary phases, are discussed. Detection of these signatures in CoRoT, Kepler or future PLATO red-giant stars would pin down their evolutionary state in an unprecedented way.
The Space Photometry Revolution
R.A. García, J. Ballot
EPJ Web of Conferences
Volume 101, Page 01014
2015 September
