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Explaining Lithium Enriched Red Giant Branch Stars (Hardcover, 1st ed. 2018)
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Explaining Lithium Enriched Red Giant Branch Stars (Hardcover, 1st ed. 2018)
Series: Springer Theses
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This thesis provides new insights into the seemingly anomalous
ubiquity of lithium-rich red giant stars. The theory of stellar
evolution, one of the most successful models of modern
astrophysics, predicts that red giant stars should display
negligible levels of lithium (Li) on their surfaces. However,
Li-rich giants, defined as those showing more than three times the
Li content of the Sun, are found everywhere astronomers look in
apparent defiance of established theory. The author addresses this
problem, analyzing the different possible explanations for such an
anomaly, which include interaction with a binary companion, the
production of Li in the interior of the star with its subsequent
transport to stellar exteriors, and the stellar interaction with
planets. The author focuses on this last possibility, where the Li
enrichment may be due to the ingestion of planets or brown dwarfs
as the stars in question grew in size while becoming giants. She
shows that this process is indeed able to explain an important
fraction of giants with Li levels above the three times solar
threshold, but that some other mechanism is needed to explain the
remaining fraction. While this is an important discovery in its own
right, the result that makes this thesis groundbreaking is its
demonstration that the threshold between Li-normal and Li-rich is
mass dependent rather than a fixed proportion of the Sun's content.
This corrects a fundamental misapprehension of the phenomenon and
opens up a new framework in which to understand and solve the
problem. Finally, the author presents interesting observational
applications and samples with which to test this new approach to
the problem of Li enrichment in giants.
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