Samuel C. C. Ting

Samuel Chao Chung Ting (Chinese: 丁肇中; pinyin: Dīng Zhàozhōng, born January 27, 1936) is an American physicist who received the Nobel Prize in 1976, with Burton Richter, for discovering the subatomic J/ψ particle. He is the founder and principal investigator for the international $2 billion Alpha Magnetic Spectrometer experiment which was installed on the International Space Station on 19 May 2011.

Samuel Chao Chung Ting
Samuel Ting after a presentation at the Kennedy Space Center in October 2010
Born (1936-01-27) January 27, 1936
Ann Arbor, MI, United States
Alma materUniversity of Michigan
Known forDiscovery of the J/ψ particle
Founder of the Alpha Magnetic Spectrometer experiment
Spouse(s)Kay Kuhne (divorced)
Susan Marks
Children3
AwardsErnest Orlando Lawrence Award (1975)
Nobel Prize for Physics (1976)
Eringen Medal (1977)
De Gasperi Award (1988)
Gold Medal for Science from Brescia (1988)
NASA Public Service Medal (2001)
Scientific career
FieldsPhysics
InstitutionsColumbia University
Massachusetts Institute of Technology
Chinese name
Chinese丁肇中
WebsiteSamuel Ting

Biography

Samuel Ting was born to Chinese parents both from Shandong province on January 27, 1936, in Ann Arbor, MI, United States of America.[1] His parents, Kuan-hai Ting and Tsun-ying Wong, met and married as graduate students at the University of Michigan.[2]

Ting's parents returned to China two months after his birth.[2] Due to the Japanese invasion, his education was disrupted. Because of the Chinese Civil War and the subsequent split of China into the two separate regions, his parents moved to Taiwan. His father started to teach engineering and his mother teach psychology at National Taiwan University (NTU). Ting attended Middle School in Taiwan.[3][4]

In 1956, Ting attended the University of Michigan. There, he studied engineering, mathematics, and physics. In 1959, he was awarded B.S.E. (in mathematics) and B.S.E. (in physics), and in 1962, he earned a doctorate in physics. In 1963, he worked at the European Organization for Nuclear Research (CERN). From 1965, he taught at Columbia University and worked at the Deutsches Elektronen-Synchrotron (DESY) in Germany. Since 1969, Ting has been a professor at the Massachusetts Institute of Technology (MIT).

Ting was awarded Ernest Orlando Lawrence Award (in 1976), Nobel Prize in Physics (in 1976), Eringen Medal (in 1977), DeGaspari Award in Science from the Government of Italy (in 1988), Gold Medal for Science from Brescia, Italy (in 1988), and NASA Public Service Medal (in 2001).[3]

Nobel Prize

In 1976, Ting was awarded the Nobel Prize in Physics, which he shared with Burton Richter of the Stanford Linear Accelerator Center, for the discovery of the J/ψ meson nuclear particle. They were chosen for the award, in the words of the Nobel committee, "for their pioneering work in the discovery of a heavy elementary particle of a new kind."[5] The discovery was made in 1974 when Ting was heading a research team at MIT exploring new regimes of high energy particle physics.[6]

Ting gave his Nobel Prize acceptance speech in Mandarin. Although there had been Chinese recipients before (Tsung-Dao Lee and Chen Ning Yang), none had previously delivered the acceptance speech in Chinese. In his Nobel banquet speech, Ting emphasized the importance of experimental work:

In reality, a theory in natural science cannot be without experimental foundations; physics, in particular, comes from experimental work. I hope that awarding the Nobel Prize to me will awaken the interest of students from the developing nations so that they will realize the importance of experimental work.[7]

Alpha Magnetic Spectrometer

A picture of Samuel Ting after he delivered a lecture on the topic of Alpha Magnetic Spectrometer (AMS) in Shandong University on October 16, 2011

In 1995, not long after the cancellation of the Superconducting Super Collider project had severely reduced the possibilities for experimental high-energy physics on Earth, Ting proposed the Alpha Magnetic Spectrometer, a space-borne cosmic-ray detector. The proposal was accepted and he became the principal investigator and has been directing the development since then. A prototype, AMS-01, was flown and tested on Space Shuttle mission STS-91 in 1998. The main mission, AMS-02, was then planned for launch by the Shuttle and mounting on the International Space Station.[8]

This project is a massive $2 billion undertaking involving 500 scientists from 56 institutions and 16 countries.[9] After the 2003 Space Shuttle Columbia disaster, NASA announced that the Shuttle was to be retired by 2010 and that AMS-02 was not on the manifest of any of the remaining Shuttle flights. Dr. Ting was forced to (successfully) lobby the United States Congress and the public to secure an additional Shuttle flight dedicated to this project. Also during this time, Ting had to deal with numerous technical problems in fabricating and qualifying the large, extremely sensitive and delicate detector module for space.[10] AMS-02 was successfully launched on Shuttle mission STS-134 on 16 May 2011 and was installed on the International Space Station on 19 May 2011.[11][12]

Research

Honors and awards

Major Awards

Member or Foreign Member of Scientific Academies

Doctor Honoris Causa degrees

Personal life

Ting lived in a turbulent age during his childhood and his family was a big influence on him. In his biographical for the Nobel Prize, he recalled:

Since both my parents were working, I was brought up by my maternal grandmother. My maternal grandfather lost his life during the first Chinese Revolution. After that, at the age of thirty-three, my grandmother decided to go to school, became a teacher, and brought my mother up alone. When I was young I often heard stories from my mother and grandmother recalling the difficult lives they had during that turbulent period and the efforts they made to provide my mother with a good education. Both of them were daring, original, and determined people, and they have left an indelible impression on me.
When I was twenty years old I decided to return to the United States for a better education. My parents’ friend, G.G. Brown, Dean of the School of Engineering, University of Michigan, told my parents I would be welcome to stay with him and his family. At that time I knew very little English and had no idea of the cost of living in the United States. In China, I had read that many American students go through college on their own resources. I informed my parents that I would do likewise. I arrived at the Detroit airport on 6 September 1956 with $100, which at the time seemed more than adequate. I was somewhat frightened, did not know anyone, and communication was difficult.[4]

In 1960 Ting married Kay Louise Kuhne, an architect, and together they had two daughters, Jeanne Ting Chowning and Amy Ting. In 1985 he married Dr. Susan Carol Marks, and they had one son, Christopher, born in 1986.[4]

Selected publications

See also

References

  1. "Samuel Ting". Physics Today. 2016. doi:10.1063/PT.5.031142.
  2. Ng, Franklin (1995). The Asian American encyclopedia. Marshall Cavendish. pp. 1, 490. ISBN 978-1-85435-684-0.
  3. "About The Programs - Personal Journeys: Samuel C.C. Ting". A Bill Moyers Special - Becoming American - The Chinese Experience. 2003. Retrieved June 2, 2014.
  4. "Samuel C.C. Ting - Biographical". Nobel prizes and laureates. Nobel Foundation. 1976. Retrieved June 3, 2014.
  5. "The Nobel Prize in Physics 1976". nobelprize.org. Retrieved 2009-10-09.
  6. Aubert, J. J.; et al. (1974). "Experimental Observation of a Heavy Particle J". Physical Review Letters. 33 (23): 1404–1406. Bibcode:1974PhRvL..33.1404A. doi:10.1103/PhysRevLett.33.1404.
  7. "Samuel C.C.Ting - Banquet Speech". Nobelprize.org. Nobel Media AB 2013. Dec 10, 1976. Retrieved June 1, 2014.
  8. "Alpha Magnetic Spectrometer - 02 (AMS-02)". NASA. 2009-08-21. Archived from the original on 2009-08-16. Retrieved 2009-09-03.
  9. William Harwood (2011-05-19). "Endeavour astronauts install $2 billion cosmic ray detector". cbsnews.com. Retrieved 2019-04-18.
  10. NASA Presents: AMS - The Fight for Flight
  11. Jeremy Hsu (2009-09-02). "Space Station Experiment to Hunt Antimatter Galaxies". Space.com. Retrieved 2009-09-02.
  12. A Costly Quest for the Dark Heart of the Cosmos (New York Times, November 16, 2010)
  13. Dorfan, D. E; Eades, J.; Lederman, L. M.; Lee, W.; Ting, C. C. (June 1965). "Observation of Antideuterons". Phys. Rev. Lett. 14 (24): 1003–1006. Bibcode:1965PhRvL..14.1003D. doi:10.1103/PhysRevLett.14.1003.Dorfan, D. E.; Eades, J.; Lederman, L. M.; Lee, W.; Ting, C. C. (1965). "Observation of Antideuterons". Phys. Rev. Lett. 14 (24): 1003–1006. Bibcode:1965PhRvL..14.1003D. doi:10.1103/PhysRevLett.14.1003.
  14. Asbury, J. G.; Bertram, W. K.; Becker, U.; Joos, P.; Rohde, M.; Smith, A. J. S.; Friedlander, S.; Jordan, C.; Ting, C. C. (1967). "Validity of Quantum Electrodynamics at Small Distances" (PDF). Physical Review Letters. 18 (2): 65–70. Bibcode:1967PhRvL..18...65A. doi:10.1103/PhysRevLett.18.65. ISSN 0031-9007.
  15. Asbury, J. G.; Becker, U.; Bertram, William K.; Joos, P.; Rohde, M.; Smith, A. J. S.; Jordan, C. L.; Ting, Samuel C. C. (1967). "Leptonic Decays of Vector Mesons: The Branching Ratio of the Electron-Positron Decay Mode of the Rho Meson" (PDF). Physical Review Letters. 19 (15): 869–872. Bibcode:1967PhRvL..19..869A. doi:10.1103/PhysRevLett.19.869. ISSN 0031-9007.
  16. Asbury, J. G.; Bertram, William K.; Becker, U.; Joos, P.; Rohde, M.; Smith, A. J. S.; Friedlander, S.; Jordan, C. L.; Ting, Samuel C. C. (1967). "Photoproduction of Wide-Angle Electron-Positron Pairs at High Energies". Physical Review. 161 (5): 1344–1355. Bibcode:1967PhRv..161.1344A. doi:10.1103/PhysRev.161.1344. ISSN 0031-899X.
  17. Alvensleben, H.; et al. (1968). "Validity of Quantum Electrodynamics at Extremely Small Distances". Physical Review Letters. 21 (21): 1501–1503. Bibcode:1968PhRvL..21.1501A. doi:10.1103/PhysRevLett.21.1501. ISSN 0031-9007.
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  19. Barber, D.; et al. (1979). "Discovery of Three-Jet Events and a Test of Quantum Chromodynamics at PETRA". Physical Review Letters. 43 (12): 830–833. Bibcode:1979PhRvL..43..830B. doi:10.1103/PhysRevLett.43.830. ISSN 0031-9007.
  20. Barber, D.P.; et al. (1979). "Tests of quantum chromodynamics and a direct measurement of the strong coupling constant αs at √s=30 GeV". Physics Letters B. 89 (1): 139–144. Bibcode:1979PhLB...89..139B. doi:10.1016/0370-2693(79)90092-3. ISSN 0370-2693.
  21. Barber, D.P.; et al. (1980). "Unique solution for the weak neutral current coupling constants in purely leptonic interactions". Physics Letters B. 95 (1): 149–153. Bibcode:1980PhLB...95..149B. doi:10.1016/0370-2693(80)90420-7. ISSN 0370-2693.
  22. Adeva, B.; et al. (1990). "Measurement of Z0 decays to hadrons, and a precise determination of the number of neutrino species". Physics Letters B. 237 (1): 136–146. Bibcode:1990PhLB..237..136A. doi:10.1016/0370-2693(90)90476-M. hdl:2027.42/28683. ISSN 0370-2693.
  23. Ahlen, S.; et al. (1994). "An antimatter spectrometer in space". Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 350 (1–2): 351–367. Bibcode:1994NIMPA.350..351A. doi:10.1016/0168-9002(94)91184-3. ISSN 0168-9002.
  24. Aguilar; et al. (2002). "The Alpha Magnetic Spectrometer (AMS) on the International Space Station: Part I – results from the test flight on the space shuttle". Physics Reports. 366 (6): 331–405. Bibcode:2002PhR...366..331A. doi:10.1016/S0370-1573(02)00013-3. ISSN 0370-1573.
  25. Aguilar, M.; et al. (AMS Collaboration) (2013). "First Result from the Alpha Magnetic Spectrometer on the International Space Station: Precision Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5–350 GeV". Physical Review Letters. 110 (14): 141102. Bibcode:2013PhRvL.110n1102A. doi:10.1103/PhysRevLett.110.141102. ISSN 0031-9007. PMID 25166975.
  26. Accardo, L.; et al. (AMS Collaboration) (2014). "High Statistics Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5–500 GeV with the Alpha Magnetic Spectrometer on the International Space Station". Physical Review Letters. 113 (12): 121101. Bibcode:2014PhRvL.113l1101A. doi:10.1103/PhysRevLett.113.121101. ISSN 0031-9007. PMID 25279616.
  27. Aguilar, M.; et al. (AMS Collaboration) (2014). "Electron and Positron Fluxes in Primary Cosmic Rays Measured with the Alpha Magnetic Spectrometer on the International Space Station". Physical Review Letters. 113 (12): 121102. Bibcode:2014PhRvL.113l1102A. doi:10.1103/PhysRevLett.113.121102. hdl:1721.1/90426. ISSN 0031-9007. PMID 25279617. S2CID 2585508.
  28. Aguilar, M.; et al. (AMS Collaboration) (2014). "Precision Measurement of the (e++e−) Flux in Primary Cosmic Rays from 0.5 GeV to 1 TeV with the Alpha Magnetic Spectrometer on the International Space Station". Physical Review Letters. 113 (22): 221102. Bibcode:2014PhRvL.113v1102A. doi:10.1103/PhysRevLett.113.221102. ISSN 0031-9007. PMID 25494065.
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