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A Turn: Things are not as they are Assumed to be

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Celestial Messengers

Part of the book series: Astronomers' Universe ((ASTRONOM))

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Abstract

The current belief was that cosmic rays were simply photons of greater energy than the ones observed in radioactive transformations. In fact, still in 1929, the German literature usually referred to cosmic rays as Ultragammastrahlung (ultra-gamma radiation). The reason is that the most penetrating radiations known at those times were the gamma rays from radioactive substances. Indeed, the mean free path of gamma ray photons emitted by these substances in air were hundreds of metres, while beta rays of similar energies had ranges of a few metres only, and the ranges of alpha particles were even shorter.

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Notes

  1. 1.

    One should assign these beta rays to the secondary electrons created by Hess ultra gamma rays.

  2. 2.

    Enrico Fermi was born in 1901 in Rome. He studied at the Scuola Normale di Pisa earning his PhD in physics in 1924. After spending some time abroad in Gottingen and Leiden he returned in Italy where he was appointed Professor of Physics at the University of Roma. He performed outstanding work both in theoretical and experimental physics and created at the Physics Institute in via Panisperna in Roma a very famous group of young researchers (later called “I ragazzi di via Panisperna”). His main contributions are the beta decay theory, the discovery of slow neutrons and of the reactions produced by them. In 1938, he was awarded the Nobel Prize for physics and in the same year migrated in the United States, first at Columbia University (1939–1942) and then at Chicago University. There he constructed the first atomic reactor in 1942. He died in 1954 in Chicago.

  3. 3.

    The use of three aligned counters was already proposed by M.A. Tuve [26] and L.M. Mott-Smith [27].

  4. 4.

    The underlined text is in italics in the paper.

  5. 5.

    The theory was discussed also in Millikan [50].

References

  1. D. Skobelzyn, Die Intensitatsverteilung in dem Spektrum der γ-Strahlen von RaC. Z. Phys. 43, 354 (1927)

    Article  ADS  Google Scholar 

  2. D. Skobelzyn, Uber eine neue Art sehr schneller β-Strahlen. Z. Phys. 54, 686 (1929)

    Article  ADS  Google Scholar 

  3. B. Rossi, Rev. Mod. Phys. 20, 539 (1948)

    Article  ADS  Google Scholar 

  4. W. Bothe, W. Kolhoerster, Naturwissenschaften 16, 1044, 1045 (1928)

    Article  ADS  Google Scholar 

  5. W. Bothe, W. Kolhoerster, Z. Phys. 56, 751 (1929)

    Article  ADS  MATH  Google Scholar 

  6. H. Geiger, W. Müller, Phys. Z. 29, 839 (1928)

    Google Scholar 

  7. H. Geiger, W. Müller, Phys. Z. 30, 489 (1929)

    Google Scholar 

  8. E. Rutherford, H. Geiger, Proc. R. Soc. A81, 141 (1908)

    ADS  Google Scholar 

  9. E. Rutherford, H. Geiger, Proc. R. Soc. Lond. A 81, 162 (1908)

    Article  ADS  Google Scholar 

  10. E. Rutherford, T. Royds, Philos. Mag. 17(6), 281 (1909)

    Google Scholar 

  11. H. Geiger, E. Marsden, Proc. R. Soc. London A 82, 495 (1909)

    Article  ADS  Google Scholar 

  12. H. Geiger, E. Marsden, Philos. Mag. 25(6), 604 (1913)

    Google Scholar 

  13. E. Rutherford, Philos. Mag. 21(6), 669 (1911)

    MATH  Google Scholar 

  14. W. Bothe, H. Geiger, Z. Phys. 25, 44 (1924)

    ADS  Google Scholar 

  15. W. Bothe, H. Geiger, Naturwissenschaften 13, 440 (1925)

    Article  ADS  Google Scholar 

  16. W. Bothe, H. Geiger, Z. Phys. 32, 639 (1925)

    Article  ADS  Google Scholar 

  17. N. Bohr, H.A. Kramers, J.C. Slater, Philos. Mag. 47(6), 785 (1924)

    Google Scholar 

  18. W. Bothe, W. Kolhoerster, Z. Phys. 56, 751 (1929)

    Article  ADS  MATH  Google Scholar 

  19. W. Bothe, W. Kolhoer Die Natur der Hohenstrahlung Naturw 17, 17 (1929)

    Google Scholar 

  20. A. Pascolini (ed.), The Scientific Legacy of B. Rossi (University of Padova, Padova, 2006)

    Google Scholar 

  21. B. Rossi, Linc. Rend. 11, 831 (1931)

    Google Scholar 

  22. B. Rossi, Nature 125, 636 (1930)

    Article  ADS  Google Scholar 

  23. B. Rossi, Moments in the Life of a Scientist (Cambridge University Press, Cambridge, UK, 1990)

    Google Scholar 

  24. B. Rossi, Naturwissenschaften 20, 65 (1932)

    Article  ADS  Google Scholar 

  25. B. Rossi, Z. Phys. 82, 151 (1933)

    Article  ADS  Google Scholar 

  26. M.A. Tuve, Phys. Rev. 35, 651 (1930)

    Article  ADS  Google Scholar 

  27. L.M. Mott-Smith, Phys. Rev. 35, 1125 (1930)

    Article  ADS  Google Scholar 

  28. J.C. Street, R.H. Woodward, E.C. Stevenson, Phys. Rev. 47, 891 (1935)

    Article  ADS  Google Scholar 

  29. P. Auger, P. Ehrenfest, J. Phys. Rad. 7, 65 (1936)

    Article  Google Scholar 

  30. L. Leprince-Ringuet, J. Phys. Rad. 7, 67 (1936)

    Article  Google Scholar 

  31. R.A. Millikan, D. Anderson, Phys. Rev. 40, 325 (1932)

    Article  ADS  Google Scholar 

  32. D. Anderson, Phys. Rev. 41, 405 (1932)

    Article  ADS  Google Scholar 

  33. H. Kulenkampff, Phys. Z. 30, 561 (1929)

    MATH  Google Scholar 

  34. E. Regener, W. Kramer, E. Lenz, Z. Phys. 85, 411 (1933)

    Article  Google Scholar 

  35. I.S. Bowen, R.A. Millikan, H.V. Neher, in Address before the London Conference on Physics, October 1934, London, 1935, p. 206

    Google Scholar 

  36. I.S. Bowen, R.A. Millikan, H.V. Neher, Phys. Rev. 46, 641 (1934)

    Article  ADS  Google Scholar 

  37. A.H. Compton, Guthrie Lecture of the Physical Society, 1 Feb. 1935

    Google Scholar 

  38. A.H. Compton, Proc. Phys. Soc. Lond. 47, 747 (1935)

    Article  ADS  Google Scholar 

  39. A.H. Compton, Proc. Am. Philos. Soc. 75, 251 (1935)

    Google Scholar 

  40. A.H. Compton, Am. Phys. Soc. (Address before 6 Jan. 1936)

    Google Scholar 

  41. A.H. Compton, Rev. Sci. Instrum. 7, 71 (1936)

    Article  ADS  Google Scholar 

  42. A.H. Compton, Phys. Rev. 50, 1119 (1936)

    Article  ADS  MATH  Google Scholar 

  43. P. Auger, P. Ehrenfest, CR 199, 1609 (1934)

    Google Scholar 

  44. R.A. Millikan, Phys. Rev. 43, 661 (1933)

    Article  ADS  Google Scholar 

  45. C. Anderson, R.A. Millikan, S. Neddermeyer, W. Pickering, Phys. Rev. 45, 352 (1934)

    Article  ADS  Google Scholar 

  46. R.A. Millikan, in Institut Poincarè Proceedings (1933)

    Google Scholar 

  47. R.A. Millikan, H.V. Neher, W.H. Pickering, Phys. Rev. 61, 397 (1942)

    Article  ADS  Google Scholar 

  48. R.A. Millikan, H.V. Neher, W.H. Pickering, Phys. Rev. 63, 234 (1943)

    Article  ADS  Google Scholar 

  49. R.A. Millikan, Rev. Mod. Phys. 21, 1 (1949)

    Article  ADS  Google Scholar 

  50. R.A. Millikan, Electrons (+ and −), Protons, Photons, Neutrons, Mesotrons and Cosmic Rays (University of Chicago Press, Chicago, 1947)

    MATH  Google Scholar 

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Bertolotti, M. (2013). A Turn: Things are not as they are Assumed to be. In: Celestial Messengers. Astronomers' Universe. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-28371-0_4

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  • DOI: https://doi.org/10.1007/978-3-642-28371-0_4

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