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On the relativisticK-shell photoeffect

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Il Nuovo Cimento (1955-1965)

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References

  1. S. Hultberg et al.:Ark. f. Fys.,9, 245 (1955);13, 117 (1958);14, 565 (1959);Nucl. Phys.,4, 120 (1657);10, 118 (1959);E. P. Grigoryev andA. V. Zolotavin:Żurn. Ėksp. Teor. Fiz.,36, 393 (1959);W. Titus:Phys. Rev.,115, 351 (1959).

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  2. New theoretical results have been obtained also for theL shell, that is: the relativistic differential and total cross sections for lowZ (M. Gavrila: to be published); the extreme relativistic total cross sections, exact inZ (R. H. Pratt: to be published).

  3. M. Gavrila:Phys. Rev.,113, 514 (1959), hereafter referred to as (G).

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  4. H. Banerjee:Nuovo Cimento,10, 863 (1958), hereafter referred to as (B);11, 220 (1959).

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  5. The same method has been used previously in an unpublished work byF. G. Nagasaka (Ph. D. Thesis, University of Notre Dame, 1955) with similar results.

  6. F. Sauter andH. Wüster:Zeits. f. Phys.,141, 83 (1955).

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  7. K. Mc Voy:Phys. Rev.,108, 365 (1958);U. Fano, K. Mc Voy andJ. Albers: to be published.

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  8. M. Gavrila:Nuovo Cimento,9, 327 (1958).R. H. Pratt:Ph. D. Thesis, University of Chicago (1959) (to be published); this contains an extensive comparison of various results obtained for the high energy limit.

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  9. SeeF. Sauter:Ann. d. Phys.,11, 454 (1931); also reference (6).

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  1. Department of Physics, Parhon University, Bucharest

    M. Gavrila

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  1. M. Gavrila
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Gavrila, M. On the relativisticK-shell photoeffect. Nuovo Cim 15, 691–694 (1960). https://doi.org/10.1007/BF02724999

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