George Smoot at POVO conference in The Netherlands
|Born||George Fitzgerald Smoot III
February 20, 1945
Yukon, Florida, United States
|Institutions||UC Berkeley/Lawrence Berkeley National Laboratory/Université Paris Diderot-Paris 7|
|Alma mater||Massachusetts Institute of Technology|
|Doctoral advisor||David H. Frisch|
|Known for||Cosmic microwave background radiation|
|Notable awards||NASA Medal for Exceptional Scientific Achievement (1992)
Kilby Award (1993)
American Achievement Golden Plate Award (1994)
E. O. Lawrence Award (1994)
Albert Einstein Medal (2003)
Nobel Prize in Physics (2006)
Gruber Prize (2006)
Daniel Chalonge Medal (2006)
Oersted Medal (2009)
George Fitzgerald Smoot III (born February 20, 1945) is an American astrophysicist, cosmologist, Nobel laureate, and one of two contestants to win the US$1 million prize on Are You Smarter than a 5th Grader?. He won the Nobel Prize in Physics in 2006 for his work on the Cosmic Background Explorer with John C. Mather that led to the "discovery of the black body form and anisotropy of the cosmic microwave background radiation," making Smoot the only Nobel laureate born in Florida.
This work helped further the Big Bang theory of the universe using the Cosmic Background Explorer (COBE) satellite. According to the Nobel Prize committee, "the COBE project can also be regarded as the starting point for cosmology as a precision science." Smoot donated his share of the Nobel Prize money, less travel costs, to a charitable foundation.
Currently Smoot is a professor of physics at the University of California, Berkeley, senior scientist at the Lawrence Berkeley National Laboratory, and since 2010, a professor of physics at the Paris Diderot University, France. In 2003, he was awarded the Einstein Medal and the Oersted Medal in 2009.
Smoot was born in Yukon, Florida. He graduated from Upper Arlington High School in Upper Arlington, Ohio, in 1962. He studied mathematics before switching to the Massachusetts Institute of Technology where he obtained dual bachelor's degrees in mathematics and physics in 1966 and a Ph.D. in particle physics in 1970.
George Smoot switched to cosmology and began work at Lawrence Berkeley National Laboratory, collaborating with Luis Walter Alvarez on the High Altitude Particle Physics Experiment, a stratospheric weather balloon designed to detect antimatter in Earth's upper atmosphere, the presence of which was predicted by the now discredited steady state theory of cosmology.
He then took up an interest in cosmic microwave background radiation (CMB), previously discovered by Arno Allan Penzias and Robert Woodrow Wilson in 1964. There were, at that time, several open questions about this topic, relating directly to fundamental questions about the structure of the universe. Certain models predicted the universe as a whole was rotating, which would have an effect on the CMB: its temperature would depend on the direction of observation. With the help of Alvarez and Richard A. Muller, Smoot developed a differential radiometer which measured the difference in temperature of the CMB between two directions 60 degrees apart. The instrument, which was mounted on a Lockheed U-2 plane, made it possible to determine that the overall rotation of the universe was zero, which was within the limits of accuracy of the instrument. It did, however, detect a variation in the temperature of the CMB of a different sort. That the CMB appears to be at a higher temperature on one side of the sky than on the opposite side, referred to as a dipole pattern, has been explained as a Doppler effect of the Earth's motion relative to the area of CMB emission, which is called the last scattering surface. Such a Doppler effect arises because the Sun, and in fact the Milky Way as a whole, is not stationary, but rather is moving at nearly 600 km/s with respect to the last scattering surface. This is probably due to the gravitational attraction between our galaxy and a concentration of mass like the Great Attractor.
At that time, the CMB appeared to be perfectly uniform excluding the distortion caused by the Doppler effect as mentioned above. This result contradicted observations of the universe, with various structures such as galaxies and galaxy clusters indicating that the universe was relatively heterogeneous on a small scale. However, these structures formed slowly. Thus, if the universe is heterogeneous today, it would have been heterogeneous at the time of the emission of the CMB as well, and observable today through weak variations in the temperature of the CMB. It was the detection of these anisotropies that Smoot was working on in the late 1970s. He then proposed to NASA a project involving a satellite equipped with a detector that was similar to the one mounted on the U-2 but was more sensitive and not influenced by air pollution. The proposal was accepted and incorporated as one of the instruments of the satellite COBE, which cost $160 million. COBE was launched on November 18, 1989, after a delay owing to the destruction of the Space Shuttle Challenger. After more than two years of observation and analysis, the COBE research team announced on 23 April 1992 that the satellite had detected tiny fluctuations in the CMB, a breakthrough in the study of the early universe. The observations were "evidence for the birth of the universe" and led Smoot to say regarding the importance of his discovery that "if you're religious, it's like looking at God."
The success of COBE was the outcome of extensive teamwork involving more than 1,000 researchers, engineers and other participants. John Mather coordinated the entire process and also had primary responsibility for the experiment that revealed the blackbody form of the CMB measured by COBE. Smoot had the main responsibility of measuring the small variations in the temperature of the radiation.
Smoot collaborated with San Francisco Chronicle journalist Keay Davidson to write the general-audience book Wrinkles in Time, that chronicled his team's efforts. In the book The Very First Light, John Mather and John Boslough complement and broaden the COBE story, and suggest that Smoot violated team policy by leaking news of COBE's discoveries to the press before NASA's formal announcement, a leak that, to Mather, smacked of self-promotion and betrayal. Smoot eventually apologized for not following the agreed publicity plan and Mather said tensions eventually eased. Mather acknowledged that Smoot had "brought COBE worldwide publicity" the project might not normally have received.
After COBE, Smoot took part in another experiment involving a stratospheric balloon, Millimeter Anisotropy eXperiment IMaging Array, which had improved angular resolution compared to COBE, and refined the measurements of the anisotropies of the CMB. Smoot has continued CMB observations and analysis and is currently a collaborator on the third generation CMB anisotropy Planck satellite. He is also a collaborator of the design of the Supernova/Acceleration Probe, a satellite which is proposed to measure the properties of dark energy. He has also assisted in analyzing data from the Spitzer Space Telescope in connection with measuring far infrared background radiation.
Smoot had a cameo appearance as himself in "The Terminator Decoupling" episode of The Big Bang Theory. He contacted the show as a fan of their often physics-based plots and was incorporated into an episode featuring him lecturing at a fictional physics symposium. He is also credited by the producer of the show with providing a joke told by Penny in the episode "The Dead Hooker Juxtaposition".
On September 18, 2009, Smoot appeared on an episode of the Fox television show Are You Smarter Than a 5th Grader?. During filming, he reached the final question, "What U.S. state is home to Acadia National Park?", to which he gave the correct answer "Maine", becoming the second person to win the one million dollar prize.
On December 10, 2009, he appeared in a BBC interview of Nobel laureates, discussing the value science has to offer society.
- Lubin, P. M. & G. F. Smoot. "Search for Linear Polarization of the Cosmic Background Radiation", Lawrence Berkeley National Laboratory (LBNL), United States Department of Energy, (Oct. 1978).
- Gorenstein, M. V.& G. F. Smoot. "Large-Angular-Scale Anisotropy in the Cosmic Background Radiation", Lawrence Berkeley National Laboratory (LBNL), United States Department of Energy, (May 1980).
- Smoot, G. F., De Amici, G., Friedman, S. D., Witebsky, C., Mandolesi, N., Partridge, R. B., Sironi, G., Danese, L. & G. De Zotti. "Low Frequency Measurement of the Spectrum of the Cosmic Background Radiation", Lawrence Berkeley National Laboratory (LBNL), United States Department of Energy, (June 1983).
- Smoot, G. F., De Amici, G., Levin, S. & C. Witebsky. "New Measurements of the Cosmic Background Radiation Spectrum", Lawrence Berkeley National Laboratory (LBNL), United States Department of Energy, (Dec. 1984).
- Smoot, G., Levin, S. M., Witebsky, C., De Amici, G., Y. Rephaeli. "An Analysis of Recent Measurements of the Temperature of the Cosmic Microwave Background Radiation", Lawrence Berkeley National Laboratory (LBNL), United States Department of Energy, (July 1987).
- Ade, P., Balbi, A., Bock, J., Borrill, J., Boscaleri, A., de Bernardis, P., Ferreira, P. G., Hanany, S., Hristov, V. V., Jaffe, A. H., Lange, A. E., Lee, A. T., Mauskopf, P. D., Netterfield, C. B., Oh, S., Pascale, E., Rabii, B., Richards, P. L., Smoot, G. F., Stompor, R., Winant, C. D. & J. H. P. Wu. "MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on Angular Scales of 10' to 5 degrees", Lawrence Berkeley National Laboratory (LBNL), United States Department of Energy, National Aeronautics and Space Administration (NASA), National Science Foundation (NSF), KDI Precision Products, Inc., Particle Physics and Astronomy Research Council UK, (June 4, 2005).
- Smoot, George; Keay Davidson (1994). Wrinkles in Time. William Morrow & Company. ISBN 0-380-72044-2.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
- Katherine Bourzac (12 January 2007). "Nobel Causes". Technology Review. Retrieved 2007-09-05.
And Smoot himself can still vividly recall playing a practical joke on his graduate thesis advisor, MIT physics professor David Frisch.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
- Horgan, J. (1992) Profile: George F. Smoot – COBE's Cosmic Cartographer, Scientific American 267(1), 34-41.
- "The Nobel Prize in Physics 2006" (.PDF) (Press release). The Royal Swedish Academy of Sciences. 3 October 2006. Retrieved 2006-10-05.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
- "Berkeley Nobel laureates donate prize money to charity" (PDF). Associated Press. 22 March 2007.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
- "Nobelists' work supports big-bang theory" (Press release). MIT Press Office. 3 October 2006. Retrieved 2006-10-03.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
- Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).
- Associated Press (April 24, 1992). "U.S. Scientists Find a 'Holy Grail': Ripples at Edge of the Universe". International Herald Tribune. p. 1.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
- Thomas H. Maugh, II (April 24, 1992). "Relics of Big Bang, Seen for First Time". Los Angeles Times. pp. A1, A30.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
- "Pictures of a Newborn Universe" (Press release). Royal Swedish Academy of Sciences. 3 October 2006. Retrieved 2007-09-05.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
- Smoot, George; Davidson, Keay (1993). Wrinkles in Time. New York: W. Morrow. ISBN 0-688-12330-9.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
- Mather, John; Boslough, John (1997). The Very First Light: The True Inside Story of the Scientific Journey Back to the Dawn of the Universe. New York: Basic Books. ISBN 0-465-01575-1.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
- Lynn Yarris (26 October 2006). "After the Phone Call". Science@Berkeley Lab. Retrieved 2007-09-05.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
- "Supernova/Acceleration Probe (SNAP)". Lawrence Berkeley National Laboratory. Retrieved 2007-09-05.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
- "Spitzer Cosmic Far-IR Background Project". Lawrence Berkeley National Laboratory. Retrieved 2007-09-05.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
- "Into the Heart of Music: Recording the Mickey Hart Band's "Mysterium Tremendum" | Grateful Dead". www.dead.net. Retrieved 2016-01-02.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
- "The Terminator Decoupling". The Big Bang Theory. Season 2. Episode 17. 9 March 2009. 20 minutes in. CBS.
- "The Big Bang Theory Videos". CBS. Retrieved 2012-08-04.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
- Lorre, Chuck. "Big Bang Theory Season 2 Episode 19 Vanity Card". Retrieved 2014-01-17.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
- "Are You Smarter Than 5th Grader? Season 3 Ep. 27". FOX, Mark Burnett Productions. Retrieved 2009-09-26.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>[dead link]
- Staff. (January 4, 2016) "Physics Geniuses Illustrate the Mind-Bending Simplicity of TurboTax in W+K's New Ads; Campaign will include a Super Bowl spot By David Gianatasio" Adweek"
- Official website
- Biography and Bibliographic Resources, from the Office of Scientific and Technical Information, United States Department of Energy
- Smoot Group Cosmology official website at the Lawrence Berkeley National Laboratory
- Low gravity phase separator U.S. Patent 4027494
- Nobel Prize announcement
- Contemplating the birth of the universe
- George Smoot on the design of the universe
- George Smoot at the Internet Movie Database
- George Smoot chairs the Eutelsat Star Awards
- George Smoot accepts position in Moscow State University
- Pariscosmo.fr Paris Center for Cosmological Physics at APC Laboratory