On Lithium-6 as diagnostic of the lithium-enrichment mechanism in red giants
arXiv:2005.14209 · doi:10.3847/2041-8213/ab9d26
Abstract
High lithium-7 () abundances in giants are indicative of non-standard physical processes affecting the star. Mechanisms that could produce this signature include contamination from an external source, such as planets, or internal production and subsequent mixing to the stellar surface. However, distinguishing between different families of solutions has proven challenging, and there is no current consensus model that explains all the data. The lithium-6 () abundance may be a potentially important discriminant, as the relative and abundances are expected to be different if the enrichment were to come from internal production or from engulfment. In this work, we model the and abundances of different giants after the engulfment of a substellar mass companion. Given that is more strongly affected by Galactic chemical evolution than , is not a good discriminant at low metallicities, where it is expected to be low in both star and planet. For modeled metallicities ([Fe/H]), we use a "best case" initial ratio equal to the solar value. increases significantly after the engulfment of a companion. However, at metallicities close to solar and higher, the signal does not last long in the stellar surface. As such, detection of surface in metal-rich red giants would most likely indicate the action of a mechanism for -enrichment other than planet engulfment. At the same time, should not be used to reject the hypothesis of engulfment in a -enriched giant or to support a particular -enhancement mechanism.
References in corpus (12)
- Standard big bang nucleosynthesis and primordial CNO Abundances after Planck
- Observable Signatures of Planet Accretion in Red Giant Stars I: Rapid Rotation and Light Element Replenishment
- Constraining Metallicity-dependent Mixing and Extra Mixing using [C/N] in Alpha-Rich Field Giants
- Rapid Rotation of Low-Mass Red Giants Using APOKASC: A Measure of Interaction Rates on the Post-main-sequence
- The lithium abundances for a large sample of red giants
- The Penn State - Torun Centre for Astronomy Planet Search stars. II. Lithium abundance analysis of the Red Giant Clump sample
- Study of Lithium Rich Giants with the GALAH Spectroscopic Survey
- A super lithium-rich red-clump star in the open cluster Trumpler 5
- The AMBRE project: a study of Li evolution in the Galactic thin and thick discs
- On Lithium-Rich Red Giants. II. Engulfment on the Giant Branch of Trumpler 20
- The Chemical Compositions and Evolutionary Status of Red Giants in the Open Cluster NGC 752
- On the observational characteristics of lithium-enhanced giant stars in comparison with normal red giants