The Trojan Horse Method in nuclear astrophysics

The study of energy production and nucleosynthesis in stars requires an increasingly precise knowledge of the nuclear reaction rates at the energies of interest. To overcome the experimental difficulties arising from the small cross sections at those energies and from the presence of the electron sc...

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Veröffentlicht in:Physics of atomic nuclei 2011-12, Vol.74 (12), p.1725-1739
Hauptverfasser: Spitaleri, C., Mukhamedzhanov, A. M., Blokhintsev, L. D., Cognata, M. La, Pizzone, R. G., Tumino, A.
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container_end_page 1739
container_issue 12
container_start_page 1725
container_title Physics of atomic nuclei
container_volume 74
creator Spitaleri, C.
Mukhamedzhanov, A. M.
Blokhintsev, L. D.
Cognata, M. La
Pizzone, R. G.
Tumino, A.
description The study of energy production and nucleosynthesis in stars requires an increasingly precise knowledge of the nuclear reaction rates at the energies of interest. To overcome the experimental difficulties arising from the small cross sections at those energies and from the presence of the electron screening, the Trojan Horse Method has been introduced. The method provides a valid alternative path to measure unscreened low-energy cross sections of reactions between charged particles, and to retrieve information on the electron screening potential when ultra-low energy direct measurements are available.
doi_str_mv 10.1134/S1063778811110184
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ispartof Physics of atomic nuclei, 2011-12, Vol.74 (12), p.1725-1739
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source SpringerNature Journals
subjects Analysis
ASTROPHYSICS
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
CROSS SECTIONS
ELECTRONS
Elementary Particles and Fields
Methods
NUCLEAR PHYSICS AND RADIATION PHYSICS
NUCLEAR REACTION KINETICS
NUCLEAR REACTIONS
NUCLEOSYNTHESIS
Particle and Nuclear Physics
Physics
Physics and Astronomy
POTENTIALS
Spyware
STARS
title The Trojan Horse Method in nuclear astrophysics
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