George Smoot

Last updated
George Smoot
George smoot 06N7133a.jpg
Smoot at 2009 POVO conference in The Netherlands
Born
George Fitzgerald Smoot III

(1945-02-20) February 20, 1945 (age 79)
NationalityAmerican
Alma mater Massachusetts Institute of Technology
Known for Cosmic microwave background radiation
Awards NASA Medal for Exceptional Scientific Achievement (1992)
Kilby Award (1993)
American Academy of Achievement Golden Plate Award (1994) [1]
E. O. Lawrence Award (1994)
Albert Einstein Medal (2003)
Nobel Prize in Physics (2006)
Gruber Prize (2006)
Daniel Chalonge Medal (2006)
Oersted Medal (2009)
Scientific career
Fields Physics
Institutions UC Berkeley/Lawrence Berkeley National Laboratory/Paris Diderot University/Hong Kong University of Science and Technology
Thesis Charge exchange of positive Kaon on platinum at three GeV/C  (1971)
Doctoral advisor David H. Frisch [2]

George Fitzgerald Smoot III (born February 20, 1945) is an American astrophysicist, cosmologist, Nobel laureate, and the second contestant to win the $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".

Contents

This work helped further the Big Bang theory of the universe using the Cosmic Background Explorer (COBE) satellite. [3] According to the Nobel Prize committee, "the COBE project can also be regarded as the starting point for cosmology as a precision science." [4] Smoot donated his share of the Nobel Prize money, less travel costs, to a charitable foundation. [5]

Smoot has been at the University of California, Berkeley and the Lawrence Berkeley National Laboratory since 1970. He is Chair of the Endowment Fund "Physics of the Universe" of Paris Center for Cosmological Physics. Apart from being elected a member of the US National Academy of Sciences and a Fellow of the American Physical Society, Smoot has been honored by several universities worldwide with doctorates or professorships. He was also the recipient of Gruber Prize in Cosmology (2006), Daniel Chalonge Medal from the International School of Astrophysics (2006), Einstein Medal from Albert Einstein Society (2003), Ernest Orlando Lawrence Award from the US Department of Energy (1995), and the Exceptional Scientific Achievement Medal from NASA (1991). He is a member of the Advisory Board of the journal Universe.

Smoot is one of the 20 American recipients of the Nobel Prize in Physics to sign a letter addressed to President George W. Bush in May 2008, urging him to "reverse the damage done to basic science research in the Fiscal Year 2008 Omnibus Appropriations Bill" by requesting additional emergency funding for the Department of Energy's Office of Science, the National Science Foundation, and the National Institute of Standards and Technology. [6]

Early life

Smoot was born in Yukon, Florida. His maternal grandfather was Johnson Tal Crawford. He graduated from Upper Arlington High School in Upper Arlington, Ohio, in 1962. [7] He studied mathematics before switching to physics at 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. [8] [9] A distant relative, Oliver R. Smoot, was the MIT student who was used as the unit of measure known as the smoot. [10] [11]

Initial research

George Smoot switched to cosmology and began work at Berkeley, 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.

COBE

Map of the CMB fluctuations found by COBE. COBE cmb fluctuations.png
Map of the CMB fluctuations found by COBE.

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. [12] 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." [13] [14]

Smoot celebrating his Nobel Prize at Lawrence Berkeley National Laboratory, 3 October 2006 George Smoot.jpg
Smoot celebrating his Nobel Prize at Lawrence Berkeley National Laboratory, 3 October 2006

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. [15]

Smoot collaborated with San Francisco Chronicle journalist Keay Davidson to write the general-audience book Wrinkles in Time , that chronicled his team's efforts. [16] In the book The Very First Light, John Mather and John Boslough complement and broaden the COBE story, [17] 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. [18]

Other projects

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 was a collaborator on the third generation CMB anisotropy observatory 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. [19] He has also assisted in analyzing data from the Spitzer Space Telescope in connection with measuring far infrared background radiation. [20] Smoot also was a leader in a group that launched the Mikhailo Lomonosov April 28, 2016.[ citation needed ]

Smoot is credited by Mickey Hart for inspiring the album Mysterium Tremendum , which is based, in part on "sounds" that can be extracted from the background signature of the Big Bang. [21]

As of September 2019, Smoot is an artificial intelligence scientist for the GTA Foundation, whose business is storing genomic sequencing data and using it in scientific applications. [22]

In November 2020, he joined Dead Sea Premier as head of research for their NUNA advanced technology anti-aging medical device development.[ citation needed ]

In April 2021, he joined the Xiaomi eco-system company Viomi as chief scientist for their AI-development.[ citation needed ]

In January 2023, George Fitzgerald Smoot III joined the National Council for Science and Technology under the President of the Republic of Kazakhstan. [23]

Media appearances

Smoot had a cameo appearance as himself in "The Terminator Decoupling" episode of The Big Bang Theory . [24] 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. [25] He is also credited by the producer of the show with providing a joke told by Penny in the episode "The Dead Hooker Juxtaposition". [26] In April 2019 he also appeared in the episode The Laureate Accumulation.

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. [27]

On December 10, 2009, he appeared in a BBC interview of Nobel laureates, discussing the value science has to offer society.

Smoot gave a 2014 TEDx lecture in which he suggested that certain aspects of physics support the simulation hypothesis, the idea that our reality is a computer-generated virtual reality. [28] [29]

In 2016, Smoot appeared in a TV commercial for Intuit TurboTax, advising a user of the software on what to do. [30]

Selected publications

Related Research Articles

<span class="mw-page-title-main">Big Bang</span> Physical theory describing the expansion of the universe

The Big Bang is a physical theory that describes how the universe expanded from an initial state of high density and temperature. It was first proposed in 1927 by Roman Catholic priest and physicist Georges Lemaître. Various cosmological models of the Big Bang explain the evolution of the observable universe from the earliest known periods through its subsequent large-scale form. These models offer a comprehensive explanation for a broad range of observed phenomena, including the abundance of light elements, the cosmic microwave background (CMB) radiation, and large-scale structure. The overall uniformity of the universe, known as the flatness problem, is explained through cosmic inflation: a sudden and very rapid expansion of space during the earliest moments. However, physics currently lacks a widely accepted theory of quantum gravity that can successfully model the earliest conditions of the Big Bang.

<span class="mw-page-title-main">Cosmic microwave background</span> Trace radiation from the early universe

The cosmic microwave background is microwave radiation that fills all space in the observable universe. It is a remnant that provides an important source of data on the primordial universe. With a standard optical telescope, the background space between stars and galaxies is almost completely dark. However, a sufficiently sensitive radio telescope detects a faint background glow that is almost uniform and is not associated with any star, galaxy, or other object. This glow is strongest in the microwave region of the radio spectrum. The accidental discovery of the CMB in 1965 by American radio astronomers Arno Penzias and Robert Wilson was the culmination of work initiated in the 1940s.

<span class="mw-page-title-main">Lawrence Berkeley National Laboratory</span> National laboratory located near Berkeley, California, U.S.

Lawrence Berkeley National Laboratory (LBNL) is a federally funded research and development center in the hills of Berkeley, California, United States. Established in 1931 by the University of California (UC), the laboratory is sponsored by the United States Department of Energy and administered by the UC system. Ernest Lawrence, who won the Nobel prize for inventing the cyclotron, founded the Lab and served as its Director until his death in 1958. Located in the Berkeley Hills, the lab overlooks the campus of the University of California, Berkeley.

<span class="mw-page-title-main">Wilkinson Microwave Anisotropy Probe</span> NASA satellite of the Explorer program

The Wilkinson Microwave Anisotropy Probe (WMAP), originally known as the Microwave Anisotropy Probe, was a NASA spacecraft operating from 2001 to 2010 which measured temperature differences across the sky in the cosmic microwave background (CMB) – the radiant heat remaining from the Big Bang. Headed by Professor Charles L. Bennett of Johns Hopkins University, the mission was developed in a joint partnership between the NASA Goddard Space Flight Center and Princeton University. The WMAP spacecraft was launched on 30 June 2001 from Florida. The WMAP mission succeeded the COBE space mission and was the second medium-class (MIDEX) spacecraft in the NASA Explorer program. In 2003, MAP was renamed WMAP in honor of cosmologist David Todd Wilkinson (1935–2002), who had been a member of the mission's science team. After nine years of operations, WMAP was switched off in 2010, following the launch of the more advanced Planck spacecraft by European Space Agency (ESA) in 2009.

<span class="mw-page-title-main">Cosmic Background Explorer</span> NASA satellite of the Explorer program

The Cosmic Background Explorer, also referred to as Explorer 66, was a NASA satellite dedicated to cosmology, which operated from 1989 to 1993. Its goals were to investigate the cosmic microwave background radiation of the universe and provide measurements that would help shape our understanding of the cosmos.

<span class="mw-page-title-main">Rainer Weiss</span> Nobel Prize-winning American physicist

Rainer "Rai" Weiss is a German-born American physicist, known for his contributions in gravitational physics and astrophysics. He is a professor of physics emeritus at MIT and an adjunct professor at LSU. He is best known for inventing the laser interferometric technique which is the basic operation of LIGO. He was Chair of the COBE Science Working Group.

The discovery of cosmic microwave background radiation constitutes a major development in modern physical cosmology. In 1964, US physicist Arno Allan Penzias and radio-astronomer Robert Woodrow Wilson discovered the cosmic microwave background (CMB), estimating its temperature as 3.5 K, as they experimented with the Holmdel Horn Antenna. The new measurements were accepted as important evidence for a hot early Universe and as evidence against the rival steady state theory as theoretical work around 1950 showed the need for a CMB for consistency with the simplest relativistic universe models. In 1978, Penzias and Wilson were awarded the Nobel Prize for Physics for their joint measurement. There had been a prior measurement of the cosmic background radiation (CMB) by Andrew McKellar in 1941 at an effective temperature of 2.3 K using CN stellar absorption lines observed by W. S. Adams. Although no reference to the CMB is made by McKellar, it was not until much later after the Penzias and Wilson measurements that the significance of this measurement was understood.

Observational cosmology is the study of the structure, the evolution and the origin of the universe through observation, using instruments such as telescopes and cosmic ray detectors.

<span class="mw-page-title-main">Ralph Alpher</span> American cosmologist (1921–2007)

Ralph Asher Alpher was an American cosmologist, who carried out pioneering work in the early 1950s on the Big Bang model, including Big Bang nucleosynthesis and predictions of the cosmic microwave background radiation.

<span class="mw-page-title-main">David Todd Wilkinson</span> American cosmologist (1935–2002)

David Todd Wilkinson was an American cosmologist, specializing in the study of the cosmic microwave background radiation (CMB).

The cosmic neutrino background is the universe's background particle radiation composed of neutrinos. They are sometimes known as relic neutrinos.

<span class="mw-page-title-main">History of the Big Bang theory</span> History of a cosmological theory

The history of the Big Bang theory began with the Big Bang's development from observations and theoretical considerations. Much of the theoretical work in cosmology now involves extensions and refinements to the basic Big Bang model. The theory itself was originally formalised by Father Georges Lemaître in 1927. Hubble's Law of the expansion of the universe provided foundational support for the theory.

<span class="mw-page-title-main">John C. Mather</span> American astrophysicist and cosmologist (born 1946)

John Cromwell Mather is an American astrophysicist, cosmologist and Nobel Prize in Physics laureate for his work on the Cosmic Background Explorer Satellite (COBE) with George Smoot.

<span class="mw-page-title-main">Charles L. Bennett</span> American astronomer

Charles L. Bennett is an American observational astrophysicist. He is a Bloomberg Distinguished Professor, the Alumni Centennial Professor of Physics and Astronomy and a Gilman Scholar at Johns Hopkins University. He is the Principal Investigator of NASA's highly successful Wilkinson Microwave Anisotropy Probe (WMAP).

The Degree Angular Scale Interferometer (DASI) was a telescope installed at the U.S. National Science Foundation's Amundsen–Scott South Pole Station in Antarctica. It was a 13-element interferometer operating between 26 and 36 GHz in ten bands. The instrument is similar in design to the Cosmic Background Imager (CBI) and the Very Small Array (VSA). In 2001 The DASI team announced the most detailed measurements of the temperature, or power spectrum of the cosmic microwave background (CMB). These results contained the first detection of the 2nd and 3rd acoustic peaks in the CMB, which were important evidence for inflation theory. This announcement was done in conjunction with the BOOMERanG and MAXIMA experiment. In 2002 the team reported the first detection of polarization anisotropies in the CMB.

<span class="mw-page-title-main">Delta 5000</span>

The Delta 5000 series was an American expendable launch system which was used to conduct an orbital launch in 1989. It was a member of the Delta family of rockets. Although several variants were put forward, only the Delta 5920 was launched. The designation used a four digit numerical code to store information on the configuration of the rocket. It was built from a combination of spare parts left over from earlier Delta rockets, which were being retired, and parts from the Delta II 6000-series, which was just entering service.

Andrew E. Lange was an astrophysicist and Goldberger Professor of Physics at the California Institute of Technology in Pasadena, California. Lange came to Caltech in 1993 and was most recently the chair of the Division of Physics, Mathematics and Astronomy. Caltech's president Jean-Lou Chameau called him "a truly great physicist and astronomer who had made seminal discoveries in observational cosmology".

Michele Limon is an Italian research scientist at the University of Pennsylvania. Limon studied physics at the Università degli Studi di Milano in Milan, Italy and completed his post-doctoral work at the University of California, Berkeley. He has been conducting research for more than 30 years and has experience in the design of ground, balloon and space-based instrumentation. His academic specialties include Astrophysics, Cosmology, Instrumentation Development, and Cryogenics.

<span class="mw-page-title-main">Cosmic microwave background spectral distortions</span> Fluctuations in the energy spectrum of the microwave background

CMB spectral distortions are tiny departures of the average cosmic microwave background (CMB) frequency spectrum from the predictions given by a perfect black body. They can be produced by a number of standard and non-standard processes occurring at the early stages of cosmic history, and therefore allow us to probe the standard picture of cosmology. Importantly, the CMB frequency spectrum and its distortions should not be confused with the CMB anisotropy power spectrum, which relates to spatial fluctuations of the CMB temperature in different directions of the sky.

Nancy Elizabeth Weber Boggess was an astrophysicist known for her work in developing telescopes that were used in space by NASA.

References

  1. "Golden Plate Awardees of the American Academy of Achievement". www.achievement.org. American Academy of Achievement.
  2. Katherine Bourzac (12 January 2007). "Nobel Causes". Technology Review. Archived from the original on 2012-01-29. 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.
  3. Horgan, J. (1992) Profile: George F. Smoot – COBE's Cosmic Cartographer, Scientific American 267(1), 34–41.
  4. "The Nobel Prize in Physics 2006" (Press release). The Royal Swedish Academy of Sciences. 3 October 2006. Archived from the original (PDF) on 2010-08-15. Retrieved 2006-10-05.
  5. "Berkeley Nobel laureates donate prize money to charity" (PDF). Associated Press. 22 March 2007. Archived from the original (PDF) on 26 July 2011. Retrieved 31 March 2010.
  6. "A Letter from America's Physics Nobel Laureates" (PDF).
  7. Jones, Gregory L (18 April 2007). "Nobel Prize winner returns home" (PDF). Upper Arlington News. Retrieved 30 November 2016.
  8. Smoot, George Fitzgerald III (1971). Charge exchange of positive Kaon on platinum at three GeV/C (Ph.D. thesis). Massachusetts Institute of Technology. OCLC   25256702 via ProQuest.
  9. "Nobelists' work supports big-bang theory" (Press release). MIT Press Office. 3 October 2006. Retrieved 2006-10-03.
  10. "At MIT, future Nobelist not above a prank or two". The Boston Globe . October 4, 2006. Retrieved 2022-03-24.
  11. "The SMOOT as unit of Length". Aether.lbl.gov. Retrieved 2022-03-24.
  12. Smoot, G.F.; et al. (September 1992). "Structure in the COBE differential microwave radiometer first-year maps". Astrophysical Journal. 396 (1): L1–L5. Bibcode:1992ApJ...396L...1S. doi: 10.1086/186504 . S2CID   120701913.
  13. "U.S. Scientists Find a 'Holy Grail': Ripples at Edge of the Universe". International Herald Tribune . Associated Press. April 24, 1992. p. 1.
  14. Thomas H. Maugh, II (April 24, 1992). "Relics of Big Bang, Seen for First Time". Los Angeles Times . pp. A1, A30.
  15. "Pictures of a Newborn Universe" (Press release). Royal Swedish Academy of Sciences. 3 October 2006. Retrieved 2007-09-05.
  16. Smoot, George; Davidson, Keay (1993). Wrinkles in Time. New York: W. Morrow. ISBN   0-688-12330-9.
  17. 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.
  18. Lynn Yarris (26 October 2006). "After the Phone Call". Science@Berkeley Lab. Archived from the original on 2008-05-06. Retrieved 2007-09-05.
  19. "Supernova/Acceleration Probe (SNAP)". Lawrence Berkeley National Laboratory . Retrieved 2007-09-05.
  20. "Spitzer Cosmic Far-IR Background Project". Lawrence Berkeley National Laboratory. Retrieved 2007-09-05.
  21. "Into the Heart of Music: Recording the Mickey Hart Band's "Mysterium Tremendum" | Grateful Dead". www.dead.net. Retrieved 2016-01-02.
  22. "The Grand Opening of GTA Gene Data Storage and Application Summit Forum Heralds A Promising Future of Gene Technology". Benzinga. 27 September 2019. Retrieved 10 January 2022.
  23. "Касым-Жомарт Токаев подписал указ о создании Нацсовета по науке и технологиям при Президенте РК". www.inform.kz (in Russian). 2023-01-26.
  24. "The Terminator Decoupling". The Big Bang Theory . Season 2. Episode 17. 9 March 2009. 20 minutes in. CBS.
  25. "The Big Bang Theory Videos". CBS. Retrieved 2012-08-04.
  26. Lorre, Chuck. "Big Bang Theory Season 2 Episode 19 Vanity Card" . Retrieved 2014-01-17.
  27. "Are You Smarter Than 5th Grader? Season 3 Ep. 27". FOX, Mark Burnett Productions. Archived from the original on September 22, 2009. Retrieved 2009-09-26.
  28. "You are a Simulation & Physics Can Prove It: George Smoot at TEDxSalford". Tedx Talks. 11 February 2014.
  29. Sean Martin (24 February 2016). "Humans already living in a COMPUTER SIMULATION, leading Nobel Prize astrophysicist warns". Express.co.uk.
  30. 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"