| Peer-Reviewed

Nuclear-Chemical Processes in the Solar Atmosphere

Received: 10 December 2014     Accepted: 19 December 2014     Published: 27 December 2014
Views:       Downloads:
Abstract

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.

Published in International Journal of Astrophysics and Space Science (Volume 2, Issue 6)
DOI 10.11648/j.ijass.20140206.12
Page(s) 88-92
Creative Commons

This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited.

Copyright

Copyright © The Author(s), 2014. Published by Science Publishing Group

Keywords

Nuclear-Chemical Processes, Synthesis of Elements in the Solar Atmosphere

References
[1] Kramarovskii Ya.M., Chechev V.P. The puzzle of the lightest elements: observations, predictions, hypotheses // Phys. Usp. 1999. V. 42. N 6/ P. 563-572.
[2] Klapdor-Kleingrothaus H.V., Zuber K. Teilchenastrophysik. B.G. Teubner GmbH, Stuttgart, 1997.
[3] Bednyakov V.A. About creation of the chemical elements // Physics of Elementary Particles and Atomic Nuclei. 2002. part 4. P. 914-963 (in Russian).
[4] Kuzhevskii B.M. Oject of research – the Sun // Journal Science in Russia. 2002. vol. 4. P. 4-11 (in Russian).
[5] Bezuglov M.V., Malyshevsky V.S., Malykhina T.V. et al. Photoproduction cosmogenic beryllium-7 in the earth's atmosphere // Electronic scientific journal “Studied in Russia” 2011. 589-591 (in Russian); http://zhurnal.ape.relarn.ru/articles/2011/046.pdf
[6] Buraeva E.A., Davydov M.G., Zorina L.V. et al. The content of cosmogenic Be-7 in surface air temperate latitudes //Atomic Energy. 2007. V.102. N 6. P. 370-374 (in Russian)
[7] Kocharov G.E. The puzzles of the Sun // The Soros Education Journal. 1998. N 3. P. 100-1004 (in Russian)
[8] Timashev S. F. Physical vacuum as a system manifesting itself on various scales – from nuclear physics to cosmology; http://arxiv.org/abs/1107.1799v7
[9] Savvatimova I.B., Timashev S.F. Nuclear-Chemical processes in the initiated tungsten and tantalum nuclei decay under actions of deuterium-containing low-temperature plasma to the cathodes of these materials // Condensed Matter Nucl. Sci., in press
[10] Timashev S. F., Simakin A. V., Shafeev G. A. Nuclear–Chemical processes under the conditions of laser ablation of metals in aqueous media (Problems of “cold fusion”) // Russian Journal of Physical Chemistry A. 2014. V. 88. N. 11. P. 1980-1988
[11] Savvatimova I.B., Gavritenkov D.V. In: Condensed Matter Nuclear Science. Proc. 12th Intern. Conf. on Cold Fusion, Yokohamacity, Japan. 27 Nov-2 Dec 2005. World Scientific Publishing Co. Pte. Ltd.: Singapore, 231-252 p.
[12] Savvatimova I. Creation of more light elements in tungsten irradiated by low-energy deuterium ions. Proc.13th Int. Conf.ICCF13, Sochy, Russia, 2007. P. 505-517.
[13] Savvatimova I., Savvatimov G., Kornilova A. Decay in tungsten irradiated by low energy deuterium ions, Proc.13th Int. Conf.ICCF13, Sochy, Russia, 2007
[14] Shafeev G.A., Simakin A.V., Bozon-Verduraz F., Robert M. // Applied Surface Science. 2007. V. 254 P. 1022-1026.
[15] Simakin A.V., Shafeev G.A. // Applied Physics A. 2009. V. 101. N. 1. P. 199-203.
[16] Barmina E.V., Sukhov I.A., Lepekhin N.M. et al // Quantum Electronics. 2013. V. 43. N 6. P. 591-596 (in Russian).
[17] Simakin A.V., Shafeev G.A. // Physics of Wave Phenomena. 2008. V. 16. N. 4. P. 268–274.
[18] Barmina E.V., Kuzmin P.G., Timashev S.F., Shafeev G.A. / http://arxiv.org/abs/1306.0830
[19] Timashev S. Dynamical essence of the basic relations of the special theory of relativity and the origin of fundamental interactions: Phenomenology // International Journal of Astrophysics and Space Science, 2014. V. 2(2). P. 22-32.
[20] Timashev Serge. Planckian energy-mass source and the dynamics of the Universe: Phenomenology // International Journal of Astrophysics and Space Science, 2014. V. 2(3). P. 33-45.
[21] J. Milton K.A., DeRaad L.L., Jr, Schwinger J. Casimir self-stress on a perfectly conducting spherical shell // Annals of Physics. 1978. V. 115. P. 388-403.
[22] Balian R., Duplantier B. Electromagnetic waves near perfect conductors. II. Casimir effect // Annals of Physics. 1978. V. 112. P. 165-208.
[23] Baranovskii E.A., Musorina S.A., Taraschuk V.P. Барановский Э.А., Мусорина С.А., Таращук В.П. Determination of lithium in sunspots, the observations in 2007 // Proceedings of the Crimean Astrophysical Observatory. 2013. V.109. N. 1. P. 165−172 (in Russian).
[24] Jung M., Bosh F., Beckert K. et al. First observation of bound-state β– decay // Phys. Rev. Lett. 1992. V. 69. N 15. P. 2164-2167.
[25] Bosh F.,Faestermann T., Friese J. et al. Observation of bound-state β– decay of fully ionized 187Re: 187Re - 187Os Cosmochronometry // Phys. Rev. Lett. 1996. V. 77. N 26. P. 5190-5193.
[26] Igashov S.Yu., Tchuvil’sky Yu.M. Electron shell and α-decay //arxiv:1212.0419v1 [nucl-th].
Cite This Article
  • APA Style

    Timashev Serge. (2014). Nuclear-Chemical Processes in the Solar Atmosphere. International Journal of Astrophysics and Space Science, 2(6), 88-92. https://doi.org/10.11648/j.ijass.20140206.12

    Copy | Download

    ACS Style

    Timashev Serge. Nuclear-Chemical Processes in the Solar Atmosphere. Int. J. Astrophys. Space Sci. 2014, 2(6), 88-92. doi: 10.11648/j.ijass.20140206.12

    Copy | Download

    AMA Style

    Timashev Serge. Nuclear-Chemical Processes in the Solar Atmosphere. Int J Astrophys Space Sci. 2014;2(6):88-92. doi: 10.11648/j.ijass.20140206.12

    Copy | Download

  • @article{10.11648/j.ijass.20140206.12,
      author = {Timashev Serge},
      title = {Nuclear-Chemical Processes in the Solar Atmosphere},
      journal = {International Journal of Astrophysics and Space Science},
      volume = {2},
      number = {6},
      pages = {88-92},
      doi = {10.11648/j.ijass.20140206.12},
      url = {https://doi.org/10.11648/j.ijass.20140206.12},
      eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ijass.20140206.12},
      abstract = {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.},
     year = {2014}
    }
    

    Copy | Download

  • TY  - JOUR
    T1  - Nuclear-Chemical Processes in the Solar Atmosphere
    AU  - Timashev Serge
    Y1  - 2014/12/27
    PY  - 2014
    N1  - https://doi.org/10.11648/j.ijass.20140206.12
    DO  - 10.11648/j.ijass.20140206.12
    T2  - International Journal of Astrophysics and Space Science
    JF  - International Journal of Astrophysics and Space Science
    JO  - International Journal of Astrophysics and Space Science
    SP  - 88
    EP  - 92
    PB  - Science Publishing Group
    SN  - 2376-7022
    UR  - https://doi.org/10.11648/j.ijass.20140206.12
    AB  - 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.
    VL  - 2
    IS  - 6
    ER  - 

    Copy | Download

Author Information
  • Karpov Institute of Physical Chemistry, Moscow, Russia

  • Sections