Isomer residual ratio of odd-odd isotope 180Ta in supernova nucleosynthsis

Details Isomer residual ratio of odd-odd isotope 180Ta in supernova nucleosynthsis Isomer residual ratio of odd-odd isotope 180Ta in supernova nucleosynthsis

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1238..222h&link_type=abstract

TOURS SYMPOSIUM ON NUCLEAR PHYSICS AND ASTROPHYSICS-VII. AIP Conference Proceedings, Volume 1238, pp. 222-224 (2010).

Physics

Nuclear Physics

Neutrino-Nucleus Reactions, Supernovae, Nuclear Structure, Beta-Decay, Excited States, Neutrino Scattering, Supernovae, Collective Levels, Weak-Interaction And Lepton Aspects, Potential Energy Surfaces For Excited Electronic States

Scientific paper

The nucleosynthesis of 180Ta has remained an unsolved problem and as its origin many nucleosynthesis mechanisms have been proposed. This isotope has the unique feature that the naturally occurring abundance of 180Ta is actually a meta-stable isomer (half-life of >=1015 yr), while the ground state is a 1+ unstable state which β-decays with a half-life of only 8.15 hr. We have made a new time-dependent calculation of 180Ta meta-stable isomer residual ratio after supernova neutrino-induced reactions. This residual isomer ratio is crucial for understanding the production and survival of this naturally occurring rare isotope. We have constructed a new model under temperature evolution after type II supernova explosion. We include the explicit linking between the isomer and all known excited states and found that the residual ratio is insensitive to astrophysical parameters such as neutrino energy spectrum, explosion energy, decay time constant. We find that the explicit time evolution of the synthesis of 180Ta avoids the overproduction relative to 138La for a neutrino process neutrino temperature of 4 MeV.

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