William Draper Harkins

William Draper Harkins (December 28, 1873 March 7, 1951) was an American physical chemist, noted for his contributions to surface chemistry[1] and nuclear chemistry. Harkins researched the structure of the atomic nucleus and was the first to propose the principle of nuclear fusion,[2][3] four years before Jean Baptiste Perrin published his theory in 1919-20. His findings enabled, among other things, the development of the H-bomb. As a visiting professor with Fritz Haber in 1909, he was introduced to the study of surface tension, and he began work on the theory of solutions and solubility during a visit to MIT in 1909-1910.[3]

William Draper Harkins
BornDecember 28, 1873
DiedMarch 7, 1951 (1951-03-08) (aged 77)
NationalityAmerican
Alma materStanford University
AwardsWillard Gibbs Award (1928)
Scientific career
Fieldsnuclear chemistry
InstitutionsUniversity of Montana
University of Chicago
Doctoral studentsLyle Benjamin Borst Robert S. Mulliken

Harkins was born in Titusville, Pennsylvania, and graduated with a PhD from Stanford University in 1907.[4] He subsequently taught chemistry at the University of Montana from 1900 to 1912, and then spent the rest of his career at the University of Chicago.

Harkins correctly predicted the existence of the neutron in 1920 (as a proton–electron complex) and was the first to use the word "neutron" in connection with the atomic nucleus.[5][6] The neutron was detected experimentally by James Chadwick in 1932. In the beginning of the 1930s, Harkins built a cyclotron. From experiments with this, he concluded that the sun might be powered by nuclear fusion. Among other University of Chicago scientists who made use of this cyclotron was Enrico Fermi, who performed neutron diffusion experiments.[7] Since 1978, the magnet yoke of the cyclotron Harkins built has been on display at Fermilab.

The magnet yoke from the cyclotron built in 1935 by Professor William D. Harkins and colleagues at the University of Chicago was moved in 1978 to Fermi National Accelerator Laboratory near Batavia, Illinois, where it is on display. Photo: William S. Higgins

Harkins was elected to the United States National Academy of Sciences in 1921 and the American Philosophical Society in 1925.[8][9]

Among his students were Robert Mulliken, Lyle Benjamin Borst, Calvin Souther Fuller, Martin Kamen, Henry W. Newson, Samuel Allison, and Robert James Moon, Jr. (1911–1989).

Harkins died in Chicago. He is buried at Oak Woods Cemetery.

References

  1. Harkins, William D. (1952). Physical Chemistry of Surface Films. Reinhold.
  2. Michael, R. Blake (1992). The Origins of Vīraśaiva Sects: A Typological Analysis of Ritual and Associational Patterns in the Śūnyasaṃpādane. Motilal Banarsidass Publishing. p. 173. ISBN 9788120806986. OCLC 490456056.
  3. Robert S. Mulliken (1975). "William Draper Harkins 1873 - 1951" (PDF). Biographical Memoirs. National Academy of Sciences. 47: 48–81.
  4. Draper Harkins, William (1907). Excess-Potential and the Marsh Test (PhD thesis). Stanford University.
  5. Harkins, William (1921). "The constitution and stability of atomic nuclei. (A contribution to the subject of inorganic evolution.)". Philos. Mag. 42 (249): 305. doi:10.1080/14786442108633770.
  6. Linus Pauling, General Chemistry, second edition, 1970, p. 102
  7. "New Outdoor Display" (PDF). Ferminews: Fermi National Accelerator Laboratory. 8 June 1978. p. 4. Retrieved 8 June 2017.
  8. "William Harkins". www.nasonline.org. Retrieved 2023-08-15.
  9. "APS Member History". search.amphilsoc.org. Retrieved 2023-08-15.
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