Astrophysical s-factor for 16O + 16O within the adiabatic molecular picture

Alexis Diaz-Torres; Leandro Romero Gasques; Michael Wiescher

doi:10.1142/S0218301308011331

Astrophysical s-factor for 16O + 16O within the adiabatic molecular picture

Alexis Diaz-Torres^*, Leandro Romero Gasques, Michael Wiescher

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

1 Citation (Scopus)

Abstract

The astrophysical S-factor for ¹⁶O+¹⁶O is investigated within the adiabatic molecular picture. It very well explains the available experimental data. The collective radial mass causes a pronounced resonant structure in the S-factor excitation function, providing a motivation for measuring the ¹⁶O+¹⁶O fusion cross section at deep sub-barrier energies

Original language	English
Pages (from-to)	2194-2198
Number of pages	5
Journal	International Journal of Modern Physics E
Volume	17
Issue number	10
DOIs	https://doi.org/10.1142/S0218301308011331
Publication status	Published - Nov 2008

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@article{e3248dd1732c4de8868e2026700a5472,

title = "Astrophysical s-factor for 16O + 16O within the adiabatic molecular picture",

abstract = "The astrophysical S-factor for 16O+16O is investigated within the adiabatic molecular picture. It very well explains the available experimental data. The collective radial mass causes a pronounced resonant structure in the S-factor excitation function, providing a motivation for measuring the 16O+16O fusion cross section at deep sub-barrier energies",

author = "Alexis Diaz-Torres and Gasques, {Leandro Romero} and Michael Wiescher",

year = "2008",

month = nov,

doi = "10.1142/S0218301308011331",

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journal = "International Journal of Modern Physics E",

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AU - Diaz-Torres, Alexis

AU - Gasques, Leandro Romero

AU - Wiescher, Michael

PY - 2008/11

Y1 - 2008/11

N2 - The astrophysical S-factor for 16O+16O is investigated within the adiabatic molecular picture. It very well explains the available experimental data. The collective radial mass causes a pronounced resonant structure in the S-factor excitation function, providing a motivation for measuring the 16O+16O fusion cross section at deep sub-barrier energies

AB - The astrophysical S-factor for 16O+16O is investigated within the adiabatic molecular picture. It very well explains the available experimental data. The collective radial mass causes a pronounced resonant structure in the S-factor excitation function, providing a motivation for measuring the 16O+16O fusion cross section at deep sub-barrier energies

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U2 - 10.1142/S0218301308011331

DO - 10.1142/S0218301308011331

M3 - Article

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VL - 17

SP - 2194

EP - 2198

JO - International Journal of Modern Physics E

JF - International Journal of Modern Physics E

IS - 10

ER -

Astrophysical s-factor for 16O + 16O within the adiabatic molecular picture

Abstract

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