Calculation of the 3He(3He,2p)4He and 3H(3H,2n)4He astrophysical S factor at low energies

S. Winkler; H. Krauss; K. Grun; T. Rauscher; H. Oberhummer; H. Abele; G. Staudt

doi:10.1088/0954-3899/18/8/004

Calculation of the ³He(³He,2p)⁴He and ³H(³H,2n)⁴He astrophysical S factor at low energies

S. Winkler, H. Krauss, K. Grun, T. Rauscher, H. Oberhummer, H. Abele, G. Staudt

School of Physics, Engineering & Computer Science

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

6 Citations (Scopus)

Abstract

The authors have calculated the cross sections for the charge symmetric reactions 3He(3He,2p)4He and 3He(3He,2p)4He at sub-Coulomb energies in the potential model. Good agreement with the experimental data is obtained. The astrophysical S factors in the thermonuclear energy range are calculated.

Original language	English
Article number	004
Pages (from-to)	L147-L152
Journal	Journal of Physics G: Nuclear and Particle Physics
Volume	18
Issue number	8
DOIs	https://doi.org/10.1088/0954-3899/18/8/004
Publication status	Published - Aug 1992

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title = "Calculation of the 3He(3He,2p)4He and 3H(3H,2n)4He astrophysical S factor at low energies",

abstract = "The authors have calculated the cross sections for the charge symmetric reactions 3He(3He,2p)4He and 3He(3He,2p)4He at sub-Coulomb energies in the potential model. Good agreement with the experimental data is obtained. The astrophysical S factors in the thermonuclear energy range are calculated.",

author = "S. Winkler and H. Krauss and K. Grun and T. Rauscher and H. Oberhummer and H. Abele and G. Staudt",

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T1 - Calculation of the 3He(3He,2p)4He and 3H(3H,2n)4He astrophysical S factor at low energies

AU - Winkler, S.

AU - Krauss, H.

AU - Grun, K.

AU - Rauscher, T.

AU - Oberhummer, H.

AU - Abele, H.

AU - Staudt, G.

PY - 1992/8

Y1 - 1992/8

N2 - The authors have calculated the cross sections for the charge symmetric reactions 3He(3He,2p)4He and 3He(3He,2p)4He at sub-Coulomb energies in the potential model. Good agreement with the experimental data is obtained. The astrophysical S factors in the thermonuclear energy range are calculated.

AB - The authors have calculated the cross sections for the charge symmetric reactions 3He(3He,2p)4He and 3He(3He,2p)4He at sub-Coulomb energies in the potential model. Good agreement with the experimental data is obtained. The astrophysical S factors in the thermonuclear energy range are calculated.

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AN - SCOPUS:4243720642

SN - 0954-3899

VL - 18

SP - L147-L152

JO - Journal of Physics G: Nuclear and Particle Physics

JF - Journal of Physics G: Nuclear and Particle Physics

IS - 8

M1 - 004

ER -

Calculation of the ³He(³He,2p)⁴He and ³H(³H,2n)⁴He astrophysical S factor at low energies

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