Stirling Colgate

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Stirling Colgate
StirlingColgate2001.jpg
Stirling Colgate in 2001
Born (1925-11-14)November 14, 1925
New York City, New York
Died December 1, 2013(2013-12-01) (aged 88)
Los Alamos, New Mexico
Citizenship American
Fields physics
Institutions Los Alamos National Laboratory
New Mexico Institute of Mining and Technology
Alma mater Cornell University
University of California, Berkeley

Stirling Auchincloss Colgate (November 14, 1925 – December 1, 2013) was an American physicist at Los Alamos National Laboratory and a professor emeritus of physics, past president at the New Mexico Institute of Mining and Technology (New Mexico Tech),[1] and an heir to the Colgate toothpaste family fortune.[2] He was America's premier[citation needed] diagnostician of thermonuclear weapons during the early years at the Lawrence Livermore National Laboratory in California. While much of his involvement with physics is still highly classified, he made many contributions in the open literature including physics education and astrophysics.[3] He was born in New York City in 1925, to Henry Auchincloss and Jeanette Thurber (née Pruyn) Colgate.[4]

Early Life and Education[edit]

Colgate attended Los Alamos Ranch School until 1942 when a military delegation along with input from Robert Oppenheimer and Ernest O. Lawrence decided to close the school. Colgate and others in the class were then graduated without notice. The following year he attended Cornell University to study electrical engineering.

In 1944 Colgate enlisted in the merchant marine. After Hiroshima, the captain called upon him to "tell us what it means." At that time what he explained was strictly confidential, most of all the description of nuclear fission.

After being discharged in 1946, Colgate returned to Cornell University. He then completed a Bachelor of Science and a PhD in nuclear physics, taking up a position as postdoctoral fellow at Berkeley.

The Development of the Hydrogen Bomb[edit]

In 1952 he moved to Livermore National Laboratory. The laboratory had been recently created by Edward Teller with encouragement from the United States Air Force in order to compete with Los Alamos weapons research. For the purposes of developing a hydrogen bomb, Teller assigned Colgate to the diagnostic measurements for their nuclear tests.

Colgate studied the radioactive products of an explosion which were scooped from the atmosphere by specially designed aircraft. His second job was measuring the range of energy of the neutrons and higher frequency gamma rays created by the nuclear tests.

Colgate's work required him to shuffle between Livermore and Los Alamos. During one trip to Los Alamos he met Subrahmanyan Chandrasekhar, whom he worked with again almost ten years later.

In the 1950s Colgate was in charge of thousands during the Bravo test, the first deliverable thermonuclear bomb. Upon this success, Teller encouraged Colgate to begin research on thermonuclear fusion and plasma physics.

Later career[edit]

In 1956 Colgate and colleague Montgomery H. Johnson were recruited to investigate the resultant radiation and debris from a hydrogen bomb explosion in space. They realized that the X-ray and gamma-ray emissions of supernovae could also set off satellites designed to detect hydrogen bomb explosions.

Colgate's supernova research during this investigation ignited his interest in astrophysics. Colgate and Johnson's first attempts to understand the mechanism of a supernova began with determining the actual cause of one. They assumed that "a shockwave from the core bounce smashes into nuclear ash plummeting inwards due to the inward tug of gravity". The shock wave would turn this matter around, heating it up, causing the supernova.[5] However this turned out to be wrong, as Richard H. White used computer simulations to show that the shock wave would not be strong enough to trigger the event. Colgate and White began developing models of stars on the verge of collapse. White wrote a computer program combining software used to design bombs with equations of state for a star.[6] In discussions with a friend, Colgate found that neutrinos can develop degeneracy pressure. This pressure aided the shock wave in blowing off the outer shells of an expiring star, leaving a neutron star behind. While this research helped validate Chandrasekhar's work on limits, neutron stars were still purely hypothetical.

In 1959, upon the advice of Los Alamos and Livermore National Laboratories, the State Department recruited Colgate as the scientific consultant on nuclear test ban negotiations in Geneva. It was here that he proposed the detection of nuclear testing by use of spy satellites, specifically the Vela satellites.[7][8] However he also raised the possibility of false alarms caused by supernovae.[9]

Despite encouragement by Teller to follow up on the detonation of the 50 megaton Czar bomb which the Soviet Union had just detonated in breach of the Soviet-American moratorium on nuclear weapons, Colgate decided to continue his prior research on supernovae.

In 1966 his research with Johnson and White finally emerged in a paper carefully edited by Chandrasekhar.

Colgate went on to serve as the president of New Mexico Tech in Socorro, New Mexico from the beginning of 1965[10] through the end of 1974.[11] While there he conducted research programs in astrophysics and atmospheric physics as well as leading the college. Many of his projects had colorful names inspired by the experimental configurations and goals. Some of these included DigAs (a search for early supernova in galaxies with a remote controlled telescope in real time using an IBM 360-44 mainframe computer through a digital microwave link from the New Mexico Tech campus to the school's Langmuir Laboratory)(see the PBS NOVA episode "Death of a Star", 1987, ~ 8 minutes in), Paul Bunyan's Condom (aka PBC - a long plastic tube inflated by a B-26 bomber engine/propeller pumping charged smoke up into a thunder storm cloud), and SNORT (supernova observational radio telescope - a search for radio frequency chirps caused by the dispersive media between the receiver and the distant supernova).

From 1975 until his death, Colgate worked at the Los Alamos National Laboratory (LANL) and was a professor emeritus at New Mexico Tech. He continued his research into supernova and received the 2006 Los Alamos medal from LANL. Colgate had a specially-designed laboratory on the New Mexico Tech campus where he continued his research until mid-2013, when he ceased work due to failing health.[12]

In 1984 Colgate co-founded the Santa Fe Institute.[1]

Quote[edit]

  • "I was always enamored with explosives, and eventually I graduated to dynamite and then nuclear bombs."

Sources[edit]

http://www.nmt.edu/about/history/storms/index.htm

Notes[edit]

  1. ^ a b "SFI co-founder Stirling Colgate passes away". Santa Fe Institute. Dec 2, 2013. Retrieved 3 December 2013. 
  2. ^ http://davidleesummers.wordpress.com/2013/12/07/remembering-stirling-colgate/
  3. ^ Colgate, Stirling A. (1952). Gamma ray absorption measurement. Ithaca, New York: Cornell University Press. [page needed]
  4. ^ World Who's Who in Science. 1968. p. 356. 
  5. ^ Colgate, Stirling A.; Johnson, Montgomery H. (1960). "Hydrodynamic Origin of Cosmic Rays". Physical Review Letters 5: 235–238. 
  6. ^ A Contribution from Richard White
  7. ^ Schilling, Govert (2002). Flash! The hunt for the biggest explosions in the universe. Naomi Greenberg-Slovin (translator). Cambridge University Press. pp. 7–10. ISBN 0521800536. 
  8. ^ "The Death Star". Horizon. BBC. 2001-10-18. Retrieved 27 June 2012. 
  9. ^ Schilling, 2002. pp. 9-10
  10. ^ Staff (6 June 1964) "Nuclear Physics Teacher Named Tech President" The Albuquerque Journal page A-1, column 2
  11. ^ Staff (13 December 1974) "Kuellmer Named President" Silver City Daily Press page 4, column 6
  12. ^ "Former Tech Pres. Colgate Passes Away". 4 December 2013. Archived from the original on 5 December 2013. 
  13. ^ Athearn, Frederic J. (Feb 1989). "Review: Storms above the Desert: Atmospheric Research in New Mexico, 1935-1985 and Big Bend on the Rio Grande". The Western Historical Quarterly 20 (1): 75–77.