Lithium synthesis in microquasar accretion

Abstract

We study the synthesis of lithium isotopes in the hot tori formed around stellar mass black holes by accretion of the companion star. We find that sizable amounts of both stable isotopes 6Li and 7Li can be produced, the exact figures varying with the characteristics of the torus and reaching as much as 1e-2 Msun for each isotope. This mass output is enough to contaminate the entire Galaxy at a level comparable with the original, pre-galactic amount of lithium and to overcome other sources such as cosmic-ray spallation or stellar nucleosynthesis.

References in corpus (5)

• X-ray Properties of Black-Hole Binaries
• Primordial Nucleosynthesis: from precision cosmology to fundamental physics
• The Formation of Population III Binaries from Cosmological Initial Conditions
• A probable stellar solution to the cosmological lithium discrepancy
• Probing the Galaxy's bars via the Hercules stream

Cited by in corpus (1)

• Neutron-induced background by an alpha-beam incident on a deuterium gas target and its implications for the study of the 2H(alpha,gamma)6Li reaction at LUNA