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20022013
most citedSpin qubits in graphene quantum dots

1.1k citations

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15 papers · 1 filter

astro-ph.SR20135 cited

Proton-rich nucleosynthesis and nuclear physics

T. Rauscher, C. Fröhlich

Although the detailed conditions for explosive nucleosynthesis are derived from astrophysical modeling, nuclear physics determines fundamental patterns in abundance yields, not onl…

astro-ph.SR201320 cited

Europium s-process signature at close-to-solar metallicity in stardust SiC grains from AGB stars

Janaina N. Avila, Trevor R. Ireland, Maria Lugaro +5

Individual mainstream stardust silicon carbide (SiC) grains and a SiC-enriched bulk sample from the Murchison carbonaceous meteorite have been analyzed by the Sensitive High Resolu…

astro-ph.SR2012130 cited

The 12C + 12C reaction and the impact on nucleosynthesis in massive stars

M. Pignatari, R. Hirschi, M. Wiescher +7

Despite much effort in the past decades, the C-burning reaction rate is uncertain by several orders of magnitude, and the relative strength between the different channels 12C(12C,a…

astro-ph.SR2012

Nova Framework: A New Tool For Modeling of Nova Outbursts and Nucleosynthesis

Pavel A. Denissenkov, Falk Herwig, Marco Pignatari +1

Classical novae are the results of surface thermonuclear explosions of H-rich material accreted by white dwarfs (WDs) from their low-mass main-sequence or red-giant binary companio…

astro-ph.SR2012558 cited

Magnetorotationally driven Supernovae as the origin of early galaxy -process elements?

Christian Winteler, Roger Kaeppeli, Albino Perego +5

We examine magnetorotationally driven supernovae as sources of -process elements in the early Galaxy. On the basis of thermodynamic histories of tracer particles from a three-di…

astro-ph.SR201241 cited

Impact of New beta-decay Half-lives on r-process Nucleosynthesis

Nobuya Nishimura, Toshitaka Kajino, Grant J. Mathews +2

We investigate the effects of newly measured beta-decay half-lives on r-process nucleosynthesis. These new rates were determined by recent experiments at the radioactive isotope be…