Hostname: page-component-745bb68f8f-lrblm Total loading time: 0 Render date: 2025-01-15T00:27:14.672Z Has data issue: false hasContentIssue false
  • English
  • Français

An Explanation for the Solar Neutrino Problem—a New Mechanism of Thermonuclear Reaction

Published online by Cambridge University Press:  25 April 2016

Hongzhang Wang
Hongzhang Wang*
Affiliation:
Department of Physics, Huaihai University, Lianyungang, Jiangsu, China
Get access Rights & Permissions [Opens in a new window]

Abstract

A new mechanism of thermonuclear reaction is briefly introduced. It shows that a certain amount of thermonuclear reaction can take place in dense, low temperature (T < 1 × 105 K) plasmas. As most regions in the Sun are at moderate and low temperature, a sufficient amount of fusion energy is generated there. Therefore, the current standard solar models, in which the solar central temperature must be slightly lower than 15 × 106 K, must be modified, and this would make the flux of high-energy neutrinos conform with the observational results.

Type
Solar & Solar System
Information
Publications of the Astronomical Society of Australia , Volume 9 , Issue 2 , 1991 , pp. 313 - 314
Copyright
Copyright © Astronomical Society of Australia 1991

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Arnold, W. A. et al., 1954, Phys. Rev., 93, 483.CrossRefGoogle Scholar
Bahcall, J. N. and Davis, R., 1981, ‘Essay in Nuclear Astrophysics’, Barness, C.A., Clayton, D. D. and Schramm, D. N. (eds), CUP, p. 243.Google Scholar
Fowler, W. A., 1984, Rev. Mod. Phys., 56, 149.CrossRefGoogle Scholar
Gamow, G., 1928, Z Physik, 51, 204.Google Scholar
Gaughlan, G. R., Fowler, W. A. et al., 1985, Atomic Data and Nuclear Data Tables, 32, 198.Google Scholar
Glass, I.I. and Sagie, D., 1982, Phys. Fluids, 25, 269.Google Scholar
Griem, H. R., 1974, Spectral Line Broadening by Plasmas, Academia Press, New York.Google Scholar
Wang, H., 1982, Acta Optica Sinica, 2, 72.Google Scholar
Wang, H., 1986, Research Report of the Institute of Plasma Physics, Academia Sinica, No. 18.Google Scholar
Wang, H., 1990, Acta Astrophysica Sinica, 10, 82.Google Scholar