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Samuel C. C. Ting

From Wikipedia, the free encyclopedia
Nobel prize winning physicist
In thisChinese name, thefamily name isTing.

Samuel C. C. Ting
丁肇中
Ting in 1977
Born (1936-01-27)January 27, 1936 (age 90)
EducationNational Cheng Kung University
University of Michigan (BS,BS,MS,PhD)
Known forDiscovery of theJ/ψ particle
Founder of theAlpha Magnetic Spectrometer experiment
AwardsErnest Orlando Lawrence Award (1975)
Nobel Prize for Physics (1976)
Eringen Medal (1977)
De Gasperi Award (1988)
Gold Medal for Science fromBrescia (1988)
NASA Public Service Medal (2001)
Scientific career
FieldsParticle physics
InstitutionsColumbia University
Massachusetts Institute of Technology
ThesisAn Investigation of Pion-Proton Interactions at High Energies (1962)
Doctoral advisorLawrence W. Jones
Martin Lewis Perl
Chinese name
Chinese丁肇中
Transcriptions
Standard Mandarin
Hanyu PinyinDīng Zhàozhōng
Wade–GilesTing¹ Chao⁴-chung¹
WebsiteSamuel Ting

Chao Chung Ting (Chinese:丁肇中;pinyin:Dīng Zhàozhōng, born January 27, 1936), also known by his English nameSamuel, is a Taiwanese-Americanparticle physicist who was awarded theNobel Prize in Physics in 1976 withBurton Richter for discovering thesubatomicJ/ψ particle. He is the Thomas Dudley Cabot Professor of Physics at theMassachusetts Institute of Technology (MIT).

Early life and education

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Ting was born on January 27, 1936, at theUniversity of Michigan Hospital inAnn Arbor, Michigan, to first generation immigrant parents fromRizao city,Shandong peninsula, China.[1] His parents, Kuan-hai Ting andTsun-ying Wong, met and married as graduate students at theUniversity of Michigan.[2] When Ting was born, his parents had just earned their master's degrees from the University of Michigan and his father, a civil engineer, had received a professorship to teach at theChina University of Mining and Technology.[3]

Ting's parents returned to China two months after his birth where Ting washomeschooled by his parents..[2][4] After the Kuomintang's defeat, Ting moved to Taiwan with his family from 1949 to 1956 and conducted most of his formal schooling there.[4] His mother taught psychology as a professor atNational Taiwan University (NTU).[5][6]

Ting attended and finished middle school in Taiwan.[5][6] After graduating fromTaipei Municipal Chien Kuo High School, he attained a perfect score onthe college entrance examinations and enteredNational Cheng Kung University in September 1955 to studymechanical engineering.[7] As an undergraduate, he completed one semester at the university with high grades in mathematics and science.[8][9]

In 1956, Ting, who barely spoke English,[4] returned to the United States at the age of 20 and won a scholarship to attend theUniversity of Michigan, where a family friend, G. G. Brown (dean of theCollege of Engineering), invited him to enroll.[6] He studied engineering,mathematics, andphysics there, completing his bachelor's degrees, master's degree, and doctorate in only six years.[5] He earned twoBachelor of Science (B.S.) degrees in engineering, mathematics, and physics in 1959, aMaster of Science (M.S.) in physics in 1960, and hisPh.D. in physics in 1962.[10][11] As a graduate student, he befriendedHomer Neal.[5] His doctoral studies were funded by a grant by theUnited States Atomic Energy Commission.[12]

Career

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In 1963, Ting worked at theEuropean Organization for Nuclear Research (CERN). From 1965, he taught atColumbia University in the City of New York and worked at theDeutsches Elektronen-Synchrotron (DESY) inGermany. Since 1969, Ting has been a professor at theMassachusetts Institute of Technology (MIT).

Ting received theErnest Orlando Lawrence Award in 1976,Nobel Prize in Physics in 1976,Eringen Medal in 1977, DeGaspari Award in Science from theGovernment of Italy in 1988, Gold Medal for Science fromBrescia, Italy in 1988, and theNASA Public Service Medal in 2001.[5]

Nobel Prize

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Main article:J/ψ meson

In 1976, Ting was awarded theNobel Prize in Physics, which he shared withBurton Richter of theStanford Linear Accelerator Center, for the discovery of theJ/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."[13] The discovery was made in 1974 when Ting was heading a research team at MIT exploring new regimes ofhigh energy particle physics.[14]

Ting gave his Nobel Prize acceptance speech inMandarin. Although there had been Chinese Nobel Prize recipients before (Tsung-Dao Lee andChen Ning Yang), none had previously delivered the acceptance speech inChinese. 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.[15]

Alpha Magnetic Spectrometer

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Main article:Alpha Magnetic Spectrometer
Ting in the Space Station Processing Facility, 2000

In 1995, not long after the cancellation of theSuperconducting Super Collider project had severely reduced the possibilities for experimental high-energy physics on Earth, Ting proposed theAlpha Magnetic Spectrometer, a space-bornecosmic-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 onSpace Shuttle missionSTS-91 in 1998. The main mission,AMS-02, was then planned for launch by the Shuttle and mounting on theInternational Space Station.[16]

This project is a massive $2 billion undertaking involving 500 scientists from 56 institutions and 16 countries.[17] After the 2003Space Shuttle Columbia disaster,NASA announced that the Shuttle was to be retired by 2010 and thatAMS-02 was not on the manifest of any of the remaining Shuttle flights. Dr. Ting was forced to (successfully) lobby theUnited 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.[18]AMS-02 was successfully launched on Shuttle missionSTS-134 on May 16, 2011, and was installed on theInternational Space Station on May 19, 2011.[19][20]

Research

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Honors and awards

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Major Awards

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Member or Foreign Member of Scientific Academies

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Doctor Honoris Causa degrees

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Personal life

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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.[6]

Ting is the eldest son of his family. He has one brother, Ting Chao-hua (丁肇華) and one sister, Ting Chao-min (丁肇民). In an interview withChina Central Television, he explained that the combination of his siblings' and his name is the first three characters of "中華民國" (Republic of China). His parents named them after the country to commemorate their grandfather, who was amartyr in theXinhai Revolution.[51]

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.[6]

Selected publications

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See also

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References

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  1. ^"Samuel Ting".Physics Today. 2016.doi:10.1063/PT.5.031142.Archived from the original on February 6, 2023. RetrievedMay 27, 2020.
  2. ^abNg, Franklin (1995).The Asian American encyclopedia. Marshall Cavendish. pp. 1, 490.ISBN 978-1-85435-684-0.
  3. ^Wang, Zhao & Park 2013, p. 1113.
  4. ^abcBoebel, Chris (September 6, 2011)."MIT 150: Samuel C.C. Ting".InfiniteMIT.Massachusetts Institute of Technology.Archived from the original on April 18, 2021. RetrievedMarch 1, 2021.
  5. ^abcdeMoyers, Bill (2003)."Personal Journeys: Samuel C.C. Ting". The Chinese Experience.PBS.Archived from the original on June 12, 2018. RetrievedJune 2, 2014.
  6. ^abcde"Samuel C.C. Ting - Biographical".Nobel prizes and laureates.Nobel Foundation. 1976.Archived from the original on July 30, 2014. RetrievedJune 3, 2014.
  7. ^"The winners of the National Cheng Kung University Alumni Outstanding Achievement Award: Ting Zhaozhong, Huang Zhigang, Xiong Keping, and Si Hualing" (in Chinese (Taiwan)).National Cheng Kung University. August 14, 2019. RetrievedSeptember 25, 2025.
  8. ^"Culture, science and education".Taiwan Today. December 1, 1976. RetrievedNovember 25, 2024.
  9. ^Hong, Rongzhi; Shi, Wennan."Studying in Taiwan, Samuel Ting had a strong bond with National Cheng Kung University".China Times. RetrievedSeptember 25, 2025 – viaNational Cheng Kung University.
  10. ^"Samuel C.C. Ting » MIT Physics".MIT Physics.Archived from the original on February 2, 2023. RetrievedFebruary 2, 2023.
  11. ^McAlpine, Kate (February 28, 2018)."Q&A with Samuel Ting".Engineering Research News, University of Michigan College of Engineering.Archived from the original on February 2, 2023. RetrievedFebruary 2, 2023.
  12. ^Linda Nobel Laureate
  13. ^"The Nobel Prize in Physics 1976". nobelprize.org.Archived from the original on August 26, 2009. RetrievedOctober 9, 2009.
  14. ^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.
  15. ^"Samuel C.C.Ting - Banquet Speech".Nobelprize.org. Nobel Media AB 2013. December 10, 1976.Archived from the original on July 30, 2014. RetrievedJune 1, 2014.
  16. ^"Alpha Magnetic Spectrometer - 02 (AMS-02)". NASA. August 21, 2009. Archived fromthe original on August 16, 2009. RetrievedSeptember 3, 2009.
  17. ^William Harwood (May 19, 2011)."Endeavour astronauts install $2 billion cosmic ray detector". cbsnews.com.Archived from the original on March 7, 2021. RetrievedApril 18, 2019.
  18. ^"NASA Presents: AMS - The Fight for Flight".IMDb.Archived from the original on October 24, 2017. RetrievedApril 18, 2019.
  19. ^Jeremy Hsu (September 2, 2009)."Space Station Experiment to Hunt Antimatter Galaxies". Space.com.Archived from the original on October 6, 2009. RetrievedSeptember 2, 2009.
  20. ^Overbye, Dennis (November 17, 2010)."A Costly Quest for the Dark Heart of the Cosmos (New York Times, November 16, 2010)".The New York Times.Archived from the original on April 4, 2017. RetrievedFebruary 25, 2017.
  21. ^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.
  22. ^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.S2CID 120873954.Archived(PDF) from the original on June 12, 2020. RetrievedSeptember 27, 2020.
  23. ^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.S2CID 198471242.Archived(PDF) from the original on September 24, 2019. RetrievedSeptember 24, 2019.
  24. ^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.S2CID 121002799.Archived from the original on June 17, 2020. RetrievedSeptember 27, 2020.
  25. ^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.Archived from the original on February 22, 2020. RetrievedSeptember 27, 2020.
  26. ^Aubert, J. J.; et al. (1974)."Experimental Observation of a Heavy ParticleJ".Phys. Rev. Lett.33 (23):1404–1406.Bibcode:1974PhRvL..33.1404A.doi:10.1103/PhysRevLett.33.1404.
  27. ^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.S2CID 13903005.
  28. ^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.
  29. ^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.
  30. ^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.
  31. ^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.
  32. ^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.hdl:2078.1/72661.ISSN 0370-1573.S2CID 122726107.
  33. ^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.hdl:1721.1/81241.ISSN 0031-9007.PMID 25166975.
  34. ^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.hdl:1721.1/90505.ISSN 0031-9007.PMID 25279616.
  35. ^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.
  36. ^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.hdl:11365/981933.ISSN 0031-9007.PMID 25494065.
  37. ^Aguilar, M.; et al. (AMS Collaboration) (2015)."Precision Measurement of the Proton Flux in Primary Cosmic Rays from Rigidity 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station".Physical Review Letters.114 (17) 171103.Bibcode:2015PhRvL.114q1103A.doi:10.1103/PhysRevLett.114.171103.hdl:10400.26/26836.ISSN 0031-9007.PMID 25978222.
  38. ^Aguilar, M.; et al. (AMS Collaboration) (2015)."Precision Measurement of the Helium Flux in Primary Cosmic Rays of Rigidities 1.9 GV to 3 TV with the Alpha Magnetic Spectrometer on the International Space Station".Physical Review Letters.115 (21) 211101.Bibcode:2015PhRvL.115u1101A.doi:10.1103/PhysRevLett.115.211101.hdl:10400.26/26975.ISSN 0031-9007.PMID 26636836.
  39. ^Aguilar, M.; et al. (AMS Collaboration) (2016)."Antiproton Flux, Antiproton-to-Proton Flux Ratio, and Properties of Elementary Particle Fluxes in Primary Cosmic Rays Measured with the Alpha Magnetic Spectrometer on the International Space Station".Physical Review Letters.117 (9) 091103.Bibcode:2016PhRvL.117i1103A.doi:10.1103/PhysRevLett.117.091103.hdl:1721.1/109505.ISSN 0031-9007.PMID 27610839.
  40. ^Aguilar, M.; et al. (AMS Collaboration) (2016)."Precision Measurement of the Boron to Carbon Flux Ratio in Cosmic Rays from 1.9 GV to 2.6 TV with the Alpha Magnetic Spectrometer on the International Space Station".Physical Review Letters.117 (23) 231102.Bibcode:2016PhRvL.117w1102A.doi:10.1103/PhysRevLett.117.231102.hdl:1721.1/106916.ISSN 0031-9007.PMID 27982618.
  41. ^Aguilar, M.; et al. (AMS Collaboration) (2017)."Observation of the Identical Rigidity Dependence of He, C, and O Cosmic Rays at High Rigidities by the Alpha Magnetic Spectrometer on the International Space Station".Physical Review Letters.119 (25) 251101.Bibcode:2017PhRvL.119y1101A.doi:10.1103/PhysRevLett.119.251101.hdl:10400.26/27534.ISSN 0031-9007.PMID 29303302.
  42. ^Aguilar, M.; et al. (AMS Collaboration) (2018)."Observation of New Properties of Secondary Cosmic Rays Lithium, Beryllium, and Boron by the Alpha Magnetic Spectrometer on the International Space Station".Physical Review Letters.120 (2) 021101.Bibcode:2018PhRvL.120b1101A.doi:10.1103/PhysRevLett.120.021101.hdl:10400.26/27558.ISSN 0031-9007.PMID 29376729.
  43. ^Aguilar, M.; et al. (AMS Collaboration) (2018)."Observation of Fine Time Structures in the Cosmic Proton and Helium Fluxes with the Alpha Magnetic Spectrometer on the International Space Station".Physical Review Letters.121 (5) 051101.Bibcode:2018PhRvL.121e1101A.doi:10.1103/PhysRevLett.121.051101.hdl:11511/28440.ISSN 0031-9007.PMID 30118264.
  44. ^Aguilar, M.; et al. (AMS Collaboration) (2018)."Observation of Complex Time Structures in the Cosmic-Ray Electron and Positron Fluxes with the Alpha Magnetic Spectrometer on the International Space Station".Physical Review Letters.121 (5) 051102.Bibcode:2018PhRvL.121e1102A.doi:10.1103/PhysRevLett.121.051102.hdl:10400.26/27696.ISSN 0031-9007.PMID 30118287.
  45. ^Aguilar, M.; et al. (AMS Collaboration) (2018)."Precision Measurement of Cosmic-Ray Nitrogen and its Primary and Secondary Components with the Alpha Magnetic Spectrometer on the International Space Station".Physical Review Letters.121 (5) 051103.Bibcode:2018PhRvL.121e1103A.doi:10.1103/PhysRevLett.121.051103.hdl:10400.26/27698.ISSN 0031-9007.PMID 30118280.
  46. ^Aguilar, M.; et al. (AMS Collaboration) (2019)."Towards Understanding the Origin of Cosmic-Ray Positrons".Physical Review Letters.122 (4) 041102.Bibcode:2019PhRvL.122d1102A.doi:10.1103/PhysRevLett.122.041102.hdl:11572/226282.ISSN 0031-9007.PMID 30768313.
  47. ^Aguilar, M.; et al. (AMS Collaboration) (2019)."Towards Understanding the Origin of Cosmic-Ray Electrons".Physical Review Letters.122 (10) 101101.Bibcode:2019PhRvL.122j1101A.doi:10.1103/PhysRevLett.122.101101.hdl:11572/230954.ISSN 0031-9007.PMID 30932626.
  48. ^Aguilar, M.; et al. (AMS Collaboration) (2019)."Properties of Cosmic Helium Isotopes Measured by the Alpha Magnetic Spectrometer".Physical Review Letters.123 (18) 181102.Bibcode:2019PhRvL.123r1102A.doi:10.1103/PhysRevLett.123.181102.hdl:1721.1/133438.ISSN 0031-9007.PMID 31763896.
  49. ^Aguilar, M.; et al. (AMS Collaboration) (2020)."Properties of Neon, Magnesium, and Silicon Primary Cosmic Rays Results from the Alpha Magnetic Spectrometer".Physical Review Letters.124 (21) 211102.Bibcode:2020PhRvL.124u1102A.doi:10.1103/PhysRevLett.124.211102.hdl:1721.1/133557.2.ISSN 0031-9007.PMID 32530660.
  50. ^"Golden Plate Awardees of the American Academy of Achievement".www.achievement.org.American Academy of Achievement.Archived from the original on December 15, 2016. RetrievedMay 22, 2020.
  51. ^"丁肇中(下)".《大家》 (in Simplified Chinese). Renmin Ribao. Archived fromthe original on March 21, 2016. RetrievedJanuary 27, 2013.

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