Cloud Chamber Observation of Photo-alpha Particles Produced by 17 MeV Gamma Rays

1946 ◽  
Vol 1 (1) ◽  
pp. 24-25
Author(s):  
Bunsaku Arakatsu ◽  
Sakae Shimizu ◽  
Terukazu Hanatani ◽  
Jiro Muto
Author(s):  
Roger H. Stuewer

In December 1931, Harold Urey discovered deuterium (and its nucleus, the deuteron) by spectroscopically detecting the faint companion lines in the Balmer spectrum of atomic hydrogen that were produced by the heavy hydrogen isotope. In February 1932, James Chadwick, stimulated by the claim of the wife-and-husband team of Irène Curie and Frédéric Joliot that polonium alpha particles cause the emission of energetic gamma rays from beryllium, proved experimentally that not gamma rays but neutrons are emitted, thereby discovering the particle whose existence had been predicted a dozen years earlier by Chadwick’s mentor, Ernest Rutherford. In August 1932, Carl Anderson took a cloud-chamber photograph of a positron traversing a lead plate, unaware that Paul Dirac had predicted the existence of the anti-electron in 1931. These three new particles, the deuteron, neutron, and positron, were immediately incorporated into the experimental and theoretical foundations of nuclear physics.


Author(s):  
Roger H. Stuewer

Serious contradictions to the existence of electrons in nuclei impinged in one way or another on the theory of beta decay and became acute when Charles Ellis and William Wooster proved, in an experimental tour de force in 1927, that beta particles are emitted from a radioactive nucleus with a continuous distribution of energies. Bohr concluded that energy is not conserved in the nucleus, an idea that Wolfgang Pauli vigorously opposed. Another puzzle arose in alpha-particle experiments. Walther Bothe and his co-workers used his coincidence method in 1928–30 and concluded that energetic gamma rays are produced when polonium alpha particles bombard beryllium and other light nuclei. That stimulated Frédéric Joliot and Irène Curie to carry out related experiments. These experimental results were thoroughly discussed at a conference that Enrico Fermi organized in Rome in October 1931, whose proceedings included the first publication of Pauli’s neutrino hypothesis.


1954 ◽  
Vol 96 (3) ◽  
pp. 673-678 ◽  
Author(s):  
S. Barile ◽  
R. Webeler ◽  
G. Allen

1951 ◽  
Vol 29 (2) ◽  
pp. 129-136 ◽  
Author(s):  
D. A. Bromley

The energy spectrum of the neutrons emitted when beryllium is bombarded with alpha particles from Th (C + C′) has been determined by measuring the ranges and directions of recoil of protons produced in a cloud chamber by the neutrons. The maximum energy of the neutrons was found to be about 15.5 Mev., within experimental error of the calculated maximum, 14.4 Mev. Many neutrons were found with energy of about 2.15 Mev. and the structure in the remainder of the spectrum can be attributed to the existence of energy levels in C12 at about 7.1 and 4.5 Mev. The angular distribution of the protons scattered by the neutrons from this source was isotropic to within experimental error.


2021 ◽  
Vol 16 (11) ◽  
pp. P11002
Author(s):  
H.V. Souza ◽  
E. Segreto ◽  
A.A. Machado ◽  
R.R. Sarmento ◽  
M.C.Q. Bazetto ◽  
...  

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