In astrophysics, the "lithium problem" refers to the discrepancy between the abundance of lithium-7 () predicted by Big Bang nucleosynthesis (BBN) models and the much lower abundance actually observed in ancient, metal-poor stars. Some theorists suggest that this discrepancy is due to stellar depletion, where turbulent mixing transports surface lithium down into hot stellar interiors where it is destroyed. To evaluate this hypothesis, astrophysicist Elena Rossi measured the abundance in a sample of ancient stars at various stages of stellar evolution. Rossi observed that despite having widely different internal temperatures and mixing rates, all the stars in the sample displayed nearly identical, uniformly low abundances. Which choice most logically completes the text?
- Astellar depletion of occurs at a much faster rate in younger, metal-rich stars than in ancient, metal-poor stars.
- the low observed abundance of in these stars is likely not the result of depletion processes occurring during their lifetimes.Cevap
- Cthe stars in the sample with the highest mixing rates had significantly lower abundances than those with lower mixing rates.
- DBBN models fail to accurately predict the abundances of other light elements in ancient, metal-poor stars.