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Abstract. High-resolution inelastic electron scattering experiments were performed at the S-DALINAC for a precise determination of the partial pair width Γπ ...

Jul 1, 2022 · The rate of carbon production in stars depends on the radiative width of the Hoyle state.

Jul 9, 2010 · The pair decay width of the first excited 0 + state in 1 2 C (the Hoyle state) is deduced from a novel analysis of the world data on inelastic electron ...

In the 1950s Hoyle proposed the existence of the state in order to account for the stellar abundance of carbon. Aside from its key role in the synthesis of the ...

We form the Hoyle state by scattering protons, produced by the Tandem accelerator at. Western Michigan University, from a carbon target at an energy and ...

Electron scattering off the first excited 0+ state in 12C (the Hoyle state) has been performed at low momentum transfers at the S-DALINAC.

Electron scattering on the Hoyle state and carbon production in stars. M ... temperature, and Q3α the energy released in the decay of the Hoyle state into three.

PDF | High-resolution inelastic electron scattering experiments were performed at the S-DALINAC for a precise determination of the partial pair width.

May 15, 2023 · We find that the well-known but enigmatic Hoyle state is composed of a “bent-arm” or obtuse triangular arrangement of alpha clusters.