30. Wide World

31. Bibliothek und Archiv fur Geschichte der Max-Planck-Gesellschaft

32. Segre Collection, AIP Niels Bohr Library

33/34. Bibliothek und Archiv fur Geschichte der Max-Planck-Gesellschaft

35. Mary Evans Rhodes

36. Argonne National Laboratory

37. Picture People

38. Department of Terrestrial Magnetism, Carnegie Institution of Washington

39. Wide World

40. Lawrence Berkeley Laboratory

41. Picture People

42. Rudolf Peierls

43. Smithsonian Institution Science Service Collection, AIP Niels Bohr Library

44. UPI/Bettmann Newsphotos

45. UPI/Bettmann Newsphotos

46. Alfred O. C. Nier

47. Photo by P. Ehrenfest, Weisskopf Collection, AIP Niels Bohr Library

48. Lawrence Berkeley Laboratory

49. Picture People

50. UPI/Bettmann Newsphotos

51. Picture People

52. Lawrence Berkeley Laboratory

53. Argonne National Laboratory

54/55. Martin Marietta

56. Philip Abelson

57–61. National Archives

62/63. Norsk Hydro

64–67. Los Alamos National Laboratory

68. Luis W. Alvarez

69. Niels Bohr Institute

70. Francoise Ulam

71/72. Los Alamos National Laboratory

73. Oppenheimer Memorial Committee

74. Emilio Segre

75. Picture People

76. Picture People

77. Mrs. George Kistiakowsky

78–83. Los Alamos National Laboratory

84. AIP Niels Bohr Library

85–96. Los Alamos National Laboratory

97. USAF

98. Picture People

99. Henry L. Stimson Papers, Yale University Library

100. Robert Muldrow Cooper Library, Clemson University

101. National Archives

102. Harold Agnew

103–105. USAF

106. Yoshito Matsushige

107. Hiroshima Peace Memorial Museum

108/109. Hiroshima Peace Culture Foundation

110/111. Hiroshima Peace Memorial Museum

112. Hiroshima Peace Culture Foundation

113. National Archives

114/115. Issei Nishimori

116. Hiroshima Peace Memorial Museum

117. Yosuke Yamabata

118. Issei Nishimori

119. Yosuke Yamabata

120. Peter Wyden

121. UPI/Bettmann Newsphotos

122–126. Los Alamos National Laboratory

127. Dr. Harold E. Edgerton, MIT, Cambridge, MA

128. Niels Bohr Institute

,

Примечания

1

Nagaoka indicates indirectly that the visit took place sometime prior to July 1910 — after Marsden's 1909 discovery and before Rutherford's announcement to Geiger at Christmastime 1910 that he had worked out an explanation.

2

George Gamow had proposed such a model in Copenhagen in 1928. Bohr credited it to Gamow at the October 1933 Solvay conference, as did Heisenberg. Bohr and his student Fritz Kalkar subsequently developed the model and physicists customarily attribute it to him.

3

Fractionation — fractional crystallization — was a technique of chemical analysis pioneered by Marie Curie in the course of purifying polonium and radium. Most substances are more soluble at a high temperature than a low. Make a strong boiling solution of a substance — for rock candy, for example, sugar in water — cool the solution, and at some point the substance will emerge out of solution to form pure crystals. Fractional crystallization further involves separating out of the same solution several different, chemically similar substances by taking advantage of their tendency to crystallize at different temperatures according to differences in their atomic weights, lighter elements crystallizing first.

4

Вы читаете The Making of the Atomic Bomb
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