Computation of <SUP>7</SUP>Be Electron-Capture Rate in the Solar Interior

YE Zi-Piao; HU Bao-Jian; KUANG Hao-Huai

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2024年10月30日

Chinese Physics C> 2002, Vol. 26> Issue(1) : 17-20

Computation of ⁷Be Electron-Capture Rate in the Solar Interior

Laboratory of Cosmic Ray and Astrophysics, Institute of High Energy Physics, The Chinese Academy of Sciences, Beijing 100039, China2 Department of Physics, Zhaoqing University, Zhaoqing 526061, China

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Abstract：
Under conditions near the center of the Sun, it shows that ⁷Be atoms are completely ionized between R=0 to R=0.1217R_⊙. The newly calculated ⁷Be and ⁸B solar neutrino fluxes are about 4.00×10⁹cm^－2·s^－1 and 6.18×10⁶cm^－2·s^－1, while the corresponding predicted values of the standard solar model are 4.80×10⁹cm^－2·s^－1 and 5.15×10⁶cm^－2·s^－1,respectively. It will further increase the discrepancy between the observed and the predicted neutrino fluxes in Super Kamiokande neutrino experiment.

References

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YE Zi-Piao, HU Bao-Jian and KUANG Hao-Huai. Computation of ⁷Be Electron-Capture Rate in the Solar Interior[J]. Chinese Physics C, 2002, 26(1): 17-20.

YE Zi-Piao, HU Bao-Jian and KUANG Hao-Huai. Computation of ⁷Be Electron-Capture Rate in the Solar Interior[J]. Chinese Physics C, 2002, 26(1): 17-20. shu

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Received: 2000-12-07
Revised: 1900-01-01

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1.
沈阳化工大学材料科学与工程学院沈阳 110142

Computation of ⁷Be Electron-Capture Rate in the Solar Interior

Corresponding author: YE Zi-Piao,

Laboratory of Cosmic Ray and Astrophysics, Institute of High Energy Physics, The Chinese Academy of Sciences, Beijing 100039, China2 Department of Physics, Zhaoqing University, Zhaoqing 526061, China

Received Date: 2000-12-07
Accepted Date: 1900-01-01
Available Online: 2002-01-05

Abstract: Under conditions near the center of the Sun, it shows that ⁷Be atoms are completely ionized between R=0 to R=0.1217R_⊙. The newly calculated ⁷Be and ⁸B solar neutrino fluxes are about 4.00×10⁹cm^－2·s^－1 and 6.18×10⁶cm^－2·s^－1, while the corresponding predicted values of the standard solar model are 4.80×10⁹cm^－2·s^－1 and 5.15×10⁶cm^－2·s^－1,respectively. It will further increase the discrepancy between the observed and the predicted neutrino fluxes in Super Kamiokande neutrino experiment.