Hartland Snyder Explained

Hartland Sweet Snyder
Birth Date:1913
Birth Place:Salt Lake City, U.S.
Death Place:Berkeley, California, U.S.
Fields:Theoretical physics
Doctoral Advisor:J. Robert Oppenheimer
Known For:Courant–Snyder parameters
Oppenheimer–Snyder model
Strong focusing

Hartland Sweet Snyder (1913 – May 22, 1962) was an American physicist[1] who, together with J. Robert Oppenheimer, showed how large stars would collapse to form black holes.[2] This work modeled the gravitational collapse of a pressure-free homogeneous fluid sphere and found that it would be unable to communicate with the rest of the universe.[3] This discovery was depicted in the movie Oppenheimer, where Snyder was portrayed by actor Rory Keane.[4] Historian of physics David C. Cassidy assessed that this prediction of black holes might have won a Nobel Prize in Physics had the authors been alive in the 1990s when evidence was available.[5]

Some publications Snyder authored together with Ernest Courant laid the foundations for the field of accelerator physics.[6] In particular, Snyder with Courant and Milton Stanley Livingston developed the principle of strong focusing that made modern particle accelerators possible. The Courant–Snyder parameters, a method of characterizing the distribution of particles in a beam, were an important part of that contribution.[7]

Life and Career

Snyder was born in Salt Lake City. He received a bachelor of science degree from the University of Utah in 1937, followed by a PhD from the University of California at Berkeley in 1940. His doctoral dissertation was supervised by Oppenheimer. He served on the physics faculty at Northwestern University from 1940 to 1947, then joined Brookhaven National Laboratory.

In 1954, Snyder bet against Maurice Goldhaber that antiprotons existed, and won.[8]

Snyder died May 22, 1962 after a heart attack. When he died, he was on leave from his position as a senior physicist at Brookhaven National Laboratory while working at the Lawrence Radiation Laboratory.

See also

References

  1. July 1962 . Hartland S. Snyder . Physics Today . 15 . 7 . 78 . 10.1063/1.3058300.
  2. Web site: Oppenheimer Almost Discovered Black Holes Before He Became 'Destroyer of Worlds'. Bartels . Meghan. Scientific American. 21 July 2023. 30 July 2023.
  3. Oppenheimer . J. R. . Snyder . H. . On Continued Gravitational Contraction . Physical Review . American Physical Society (APS) . 56 . 5 . 1 September 1939 . 0031-899X . 10.1103/physrev.56.455 . 455–459. free .
  4. Web site: Oppenheimer Cast: Every Celebrity & Actor In the Movie. Thompson. David. The Direct. 29 July 2023. 30 July 2023.
  5. https://www.science.org/content/article/movie-adds-oppenheimer-s-celebrity-just-how-good-physicist-was-he Hollywood movie aside, just how good a physicist was Oppenheimer? A-bomb architect "was no Einstein", historian says, but he did Nobel-level work on black holes
  6. Courant . E. D. . Ernest Courant . Livingston . M. S. . Milton Stanley Livingston . Snyder . H. S. . Hartland Sweet Snyder . 1952 . The Strong-Focusing Synchrotron—A New High Energy Accelerator . . 88 . 5 . 1190–1196 . 1952PhRv...88.1190C . 10.1103/PhysRev.88.1190 . free . 2027/mdp.39015086454124.
  7. Courant . E. D. . Ernest Courant . Snyder . H. S. . Hartland Sweet Snyder . Jan 1958 . Theory of the alternating-gradient synchrotron . Annals of Physics . 3 . 1 . 360–408 . 10.1006/aphy.2000.6012 . 2000AnPhy.281..360C .
  8. Web site: Putting Money Where Their Minds Are; Where Scientists Gather, Wagering Flourishes (Published 1998) . nytimes.com . 25 August 1998 . 30 July 2023 .