The lithium isotope ratio in Population II halo dwarfs - A proposed test of the late decaying massive particle nucleosynthesis scenario

Details The lithium isotope ratio in Population II halo dwarfs - A proposed test of the late decaying massive particle nucleosynthesis scenario The lithium isotope ratio in Population II halo dwarfs - A proposed test of the late decaying massive particle nucleosynthesis scenario

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...329l.103b&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 329, June 15, 1988, p. L103-L106. NSF-DOE-NASA-supported research

Mathematics

Logic

41

Abundance, Big Bang Cosmology, Dwarf Stars, Elementary Particles, Lithium Isotopes, Nuclear Fusion, Baryons, Light Elements, Neutrinos, Universe

Scientific paper

It is shown that observations of the lithium isotope ratio in high
surface temperature Population II stars may be critical to cosmological
nucleosynthesis models. In particular, decaying particle scenarios as
derived in some supersymmetric models may stand or fall with such
observations.

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