Nuclear-Chemical Processes in the Solar Atmosphere
International Journal of Astrophysics and Space Science
Volume 2, Issue 6, December 2014, Pages: 88-92
Received: Dec. 10, 2014; Accepted: Dec. 19, 2014; Published: Dec. 27, 2014
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Timashev Serge, Karpov Institute of Physical Chemistry, Moscow, Russia; Institute of Laser and Information Technologies, Russian Academy of Sciences, Moscow, Russia
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The ideas put forward earlier about the initiation of nuclear processes in a low-temperature plasma as a result of interaction between electrons of high (on chemical scales) energies and nuclei are demonstrated to be helpful in clearing some debatable issues concerning the synthesis of light elements in the solar atmosphere. Specifically the case in point is one of the puzzles associated with the radioactive isotope beryllium-7 whose abundance in the solar atmosphere exceeds the concentration of the stable isotope lithium-7 that is formed from beryllium-7, too, upon K-electron capture with a half-life of 53 days.
Nuclear-Chemical Processes, Synthesis of Elements in the Solar Atmosphere
To cite this article
Timashev Serge, Nuclear-Chemical Processes in the Solar Atmosphere, International Journal of Astrophysics and Space Science. Vol. 2, No. 6, 2014, pp. 88-92. doi: 10.11648/j.ijass.20140206.12
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