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.

Autorentext
Claudia Aguilera-Gómez received her PhD in 2017 from Institute of Astrophysics at the Pontificia Universidad Católica de Chile. She currently holds a position at Universidad Andrés Bello, Chile.

Inhalt
Contents1 Introduction 11.1 Stellar evolutionary models . . . . . . . . . . . . . . . . . . . . . . . . 21.2 Lithium in astrophysics . . . . . . . . . . . . . . . . . . . . . . . . . . 31.2.1 Big Bang Nucleosynthesis and the Lithium Problem . . . . . . 41.2.2 Chemical Enrichment of the Galaxy . . . . . . . . . . . . . . . 71.2.3 Lithium in stars . . . . . . . . . . . . . . . . . . . . . . . . . . 81.3 Red Giant Branch Stars . . . . . . . . . . . . . . . . . . . . . . . . . 111.3.1 Lithium rich giants . . . . . . . . . . . . . . . . . . . . . . . . 141.4 Outline of this thesis . . . . . . . . . . . . . . . . . . . . . . . . . . . 19I Scenarios of Lithium enrichment 212 Internal Mechanisms 222.1 Rotationally-induced mixing . . . . . . . . . . . . . . . . . . . . . . . 242.2 Thermohaline mixing . . . . . . . . . . . . . . . . . . . . . . . . . . . 282.3 Magnetic mechanisms and Magneto-Thermohaline Mixing . . . . . . 312.4 Summary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 333 External Mechanisms 353.1 Binary companions . . . . . . . . . . . . . . . . . . . . . . . . . . . . 353.2 Substellar companion engulfment . . . . . . . . . . . . . . . . . . . . 393.2.1 Models . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 403.2.2 Point of SSC dissipation . . . . . . . . . . . . . . . . . . . . . 453.2.3 Evolution of the supercial Li abundance . . . . . . . . . . . . 533.2.4 Rates of Li-enrichment . . . . . . . . . . . . . . . . . . . . . . 663.2.5 SSC models in perspective . . . . . . . . . . . . . . . . . . . . 723.2.6 Other observational constraints . . . . . . . . . . . . . . . . . 763.2.7 Evolution of 6Li abundance . . . . . . . . . . . . . . . . . . . 783.3 Summary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 85II Observational Applications 914 Trumpler 20 944.1 The possibility of extra mixing in the Trumpler 20 giants . . . . . . . 954.2 The two Li-rich giants in Trumpler 20: Possible engulfment . . . . . . 1014.3 Summary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1045 Field Giants 1055.1 Sample selection . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1065.2 Measuring the Li abundance of the sample . . . . . . . . . . . . . . . 1095.3 Comparison with other works . . . . . . . . . . . . . . . . . . . . . . 1215.4 Results . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1225.5 Summary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1246 Stars with low main sequence Li abundances 1276.1 Assembling the catalog . . . . . . . . . . . . . . . . . . . . . . . . . . 1286.2 An overview of the catalog . . . . . . . . . . . . . . . . . . . . . . . . 1376.3 The lithium desert . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1416.3.1 Characterizing the Li desert: Mass and metallicity . . . . . . . 1436.3.2 Characterizing the Li Desert: Evolutionary stage . . . . . . . 1456.3.3 The origin of the Li Desert . . . . . . . . . . . . . . . . . . . . 1486.4 Discussion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1586.5 Summary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 159III Summary and Future Work 163Bibliography 183