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Simulation of passage of gallactic cosmic ray nuclei in meteorite-pallasite substance

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Abstract

The results are presented of model calculation of the interaction and yield of galactic-cosmic-ray superheavy-element nuclear fragmentation products from the 50 < Z < 92 range of their charges as they pass through a certain meteorite-pallasite substance thickness.

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Authors and Affiliations

  1. P. N. Lebedev Physical Institute of the Russian Academy of Science, Russia, 119991, Moscow, Leninsky prospect, 53

    A. B. Aleksandrov, A. V. Bagulya, M. S. Vladimirov, N. V. Galkina, L. A. Goncharova, N. S. Konovalova, N. M. Okat’eva, N. G. Polukhina & N. I. Starkov

  2. V. I. Vernadsky Institute of Geochemistry and Analytical Chemistry of the Russian Academy of Science, Russia, 119991, Moscow, Kosygina street 19

    G. V. Kalinina & L. L. Kashkarov

Authors
  1. A. B. Aleksandrov
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  2. A. V. Bagulya
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  3. M. S. Vladimirov
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  4. N. V. Galkina
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  5. L. A. Goncharova
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  6. G. V. Kalinina
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  7. L. L. Kashkarov
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  8. N. S. Konovalova
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  9. N. M. Okat’eva
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  10. N. G. Polukhina
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  11. N. I. Starkov
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Corresponding author

Correspondence to N. M. Okat’eva.

Additional information

Original Russian Text © A.B. Aleksandrov, A.V. Bagulya, M.S. Vladimirov, N.V. Galkina, L.A. Goncharova, G.V. Kalinina, L.L. Kashkarov, N.S. Konovalova, N.M. Okat’eva, N.G. Polukhina, N.I. Starkov, 2013, published in Kratkie Soobshcheniya po Fizike, 2013, Vol. 40, No. 5, pp. 29–38.

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Aleksandrov, A.B., Bagulya, A.V., Vladimirov, M.S. et al. Simulation of passage of gallactic cosmic ray nuclei in meteorite-pallasite substance. Bull. Lebedev Phys. Inst. 40, 126–131 (2013). https://doi.org/10.3103/S1068335613050059

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  • DOI: https://doi.org/10.3103/S1068335613050059

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