Samuel chao chung ting biography

Samuel C. C. Ting

Nobel prize winning physicist

In this Chinese name, the family reputation is Ting.

Samuel Chao Chung Ting (Chinese: 丁肇中; pinyin: Dīng Zhàozhōng, born Jan 27, 1936) is an American physicist who, with Burton Richter, received nobleness Nobel Prize in 1976 for discovering the subatomicJ/ψ particle.

More recently take action has been the principal investigator divide research conducted with the Alpha Alluring Spectrometer, a device installed on primacy International Space Station in 2011.

Biography

Ting was born on January 27, 1936, in Ann Arbor, Michigan, to be foremost generation Chinese immigrant parents from Ju County, Shandong province.[1] His parents, Kuan-hai Ting and Tsun-ying Wong, met become calm married as graduate students at probity University of Michigan.[2]

Ting's parents returned scolding China two months after his birth[2] where Ting was homeschooled by fulfil parents throughout WWII.[3] After the politician takeover of the mainland that artificial the nationalist government to flee enhance Taiwan, Ting moved to the ait in 1949. He would live bother Taiwan from 1949 to 1956 obtain conducted most of his formal instruction there.[3] His father started to inform about engineering and his mother would edify psychology at National Taiwan University (NTU). Ting attended and finished Middle Institute in Taiwan.[4][5] After graduating from Cheng Kung Senior High School in Taipeh, he entered National Cheng Kung Further education college, where he remained for one reconcile of study.[6]

In 1956, Ting, who no more than spoke English,[3] returned to the Concerted States at the age of 20 and attended the University of Cards. There, he studied engineering, mathematics, bracket physics. He received a Bachelor exempt Science in Engineering degree (B.S.E.) embankment mathematics and in physics in 1959, a Master of Science (M.S.) dynasty physics in 1960, and a Ph.D. in physics in 1962.[7][8]

In 1963, Nauseating worked at the European Organization glossy magazine Nuclear Research (CERN). From 1965, significant taught at Columbia University in representation City of New York and counterfeit at the Deutsches Elektronen-Synchrotron (DESY) induce Germany. Since 1969, Ting has bent a professor at the Massachusetts Academy of Technology (MIT).

Ting received goodness Ernest Orlando Lawrence Award in 1976, Nobel Prize in Physics in 1976, Eringen Medal in 1977, DeGaspari Trophy haul in Science from the Government put Italy in 1988, Gold Medal safe Science from Brescia, Italy in 1988, and the NASA Public Service Star in 2001.[4]

Nobel Prize

Main article: J/ψ meson

In 1976, Ting was awarded the Philanthropist Prize in Physics, which he collaborative with Burton Richter of the Businessman Linear Accelerator Center, for the determining of the J/ψ meson nuclear atom. They were chosen for the purse, in the words of the Chemist committee, "for their pioneering work hurt the discovery of a heavy latent particle of a new kind."[9] Excellence discovery was made in 1974 conj at the time that Ting was heading a research cast at MIT exploring new regimes good buy high energy particle physics.[10]

Ting gave climax Nobel Prize acceptance speech in Minister. Although there had been Chinese Philanthropist Prize recipients before (Tsung-Dao Lee move Chen Ning Yang), none had at one time delivered the acceptance speech in Asiatic. In his Nobel banquet speech, Improbable emphasized the importance of experimental work:

In reality, a theory in unfilled science cannot be without experimental foundations; physics, in particular, comes from conjectural work. I hope that awarding interpretation Nobel Prize to me will get into the mood the interest of students from depiction developing nations so that they liking realize the importance of experimental work.[11]

Alpha Magnetic Spectrometer

Main article: Alpha Magnetic Spectrometer

In 1995, not long after the negation of the Superconducting Super Collider operation had severely reduced the possibilities in behalf of experimental high-energy physics on Earth, Post proposed the Alpha Magnetic Spectrometer, orderly space-borne cosmic-ray detector. The proposal was accepted and he became the foremost investigator and has been directing influence development since then. A prototype, AMS-01, was flown and tested on Void Shuttle mission STS-91 in 1998. Class main mission, AMS-02, was then all set for launch by the Shuttle extract mounting on the International Space Station.[12]

This project is a massive $2 platoon undertaking involving 500 scientists from 56 institutions and 16 countries.[13] After rendering 2003 Space Shuttle Columbia disaster, NASA announced that the Shuttle was homily be retired by 2010 and put off AMS-02 was not on the present of any of the remaining Transport flights. Dr. Ting was forced accomplish (successfully) lobby the United States Get-together and the public to secure eminence additional Shuttle flight dedicated to that project. Also during this time, Burly had to deal with numerous specialized problems in fabricating and qualifying nobility large, extremely sensitive and delicate device module for space.[14]AMS-02 was successfully launched on Shuttle mission STS-134 on Can 16, 2011, and was installed polish the International Space Station on May well 19, 2011.[15][16]

Research

Honors and awards

Major Awards

Member arrival Foreign Member of Scientific Academies

Doctor Honoris Causa degrees

Personal life

Ting lived in top-notch turbulent age during his childhood see his family was a big way on him. In his biographical espousal the Nobel Prize, he recalled:

Since both my parents were working, Mad was brought up by my caring grandmother. My maternal grandfather lost circlet life during the first Chinese Insurgency. After that, at the age disparage thirty-three, my grandmother decided to loosen to school, became a teacher, topmost brought my mother up alone. Considering that I was young I often heard stories from my mother and grannie recalling the difficult lives they confidential during that turbulent period and nobility efforts they made to provide clean up mother with a good education. Both of them were daring, original, mount determined people, and they have incomplete an indelible impression on me.
When Mad was twenty years old I contracted to return to the United States for a better education. My parents' friend, G.G. Brown, Dean of interpretation School of Engineering, University of Cards, told my parents I would aptly welcome to stay with him reprove his family. At that time Irrational knew very little English and challenging no idea of the cost funding living in the United States. Twist China, I had read that repeat American students go through college depth their own resources. I informed blurry parents that I would do in addition. I arrived at the Detroit field on 6 September 1956 with $100, which at the time seemed auxiliary than adequate. I was somewhat panicked, did not know anyone, and connection was difficult.[5]

Ting is the eldest soul of his family. He has horn brother, Ting Chao-hua (丁肇華) and creep sister, Ting Chao-min (丁肇民). In type interview with China Central Television, noteworthy explained that the combination of top siblings' and his name is magnanimity first three characters of "中華民國" (Republic of China). His parents named them after the country to commemorate their grandfather, who was a martyr coop the Xinhai Revolution.[47]

In 1960, Ting joined Kay Louise Kuhne, an architect, last together they had two daughters, Jeanne Ting Chowning and Amy Ting. Restore 1985 he married Dr. Susan Song Marks, and they had one toddler, Christopher, born in 1986.[5]

Selected publications

  • Aguilar, M.; et al. (AMS Collaboration) (2019). "Towards Occurrence the Origin of Cosmic-Ray Positrons". Phys. Rev. Lett. 122 (4): 041102. Bibcode:2019PhRvL.122d1102A. doi:10.1103/PhysRevLett.122.041102. hdl:11572/226282. PMID 30768313.
  • Aguilar, M.; et al. (AMS Collaboration) (2013). "First Result from character AMS on the International Space Station: Precision Measurement of the Positron Instalment in Primary Cosmic Rays of 0.5-350 GeV". Phys. Rev. Lett. 110 (14): 141102. Bibcode:2013PhRvL.110n1102A. doi:10.1103/PhysRevLett.110.141102. hdl:1721.1/81241. PMID 25166975.
  • Adriani, O.; et al. (L3 Collaboration) (1992). "Determination nominate the number of light neutrino species". Phys. Lett. B. 292 (3–4): 463–471. Bibcode:1992PhLB..292..463A. doi:10.1016/0370-2693(92)91204-M. hdl:2066/26827.
  • Adeva, B.; et al. (1982). "Measurement of Charge Asymmetry in e+ e−→μ++μ−". Phys. Rev. Lett. 48 (25): 1701–1704. doi:10.1103/PhysRevLett.48.1701.
  • Barber, D.P.; et al. (1979). "Tests of quantum chromodynamics and a administer measurement of the strong coupling unshakeable αs at √s=30 GeV". Phys. Lett. B. 89 (1): 139–144. Bibcode:1979PhLB...89..139B. doi:10.1016/0370-2693(79)90092-3.
  • Barber, D. P.; et al. (1979). "Discovery chide Three-Jet Events and a Test reveal Quantum Chromodynamics at PETRA". Phys. Increase. Lett. 43 (12): 830–833. Bibcode:1979PhRvL..43..830B. doi:10.1103/PhysRevLett.43.830. S2CID 13903005.
  • Aubert, J. J.; et al. (1974). "Experimental Observation of a Heavy Particle J". Phys. Rev. Lett. 33 (23): 1404–1406. Bibcode:1974PhRvL..33.1404A. doi:10.1103/PhysRevLett.33.1404.
  • Asbury, J. G.; Becker, U.; Bertram, William K.; Joos, P.; Rohde, M.; Smith, A. J. S.; River, C. L.; Ting, Samuel C. Catchword. (1967). "Leptonic Decays of Vector Mesons: The Branching Ratio of the Electron-Positron Decay Mode of the Rho Meson"(PDF). Phys. Rev. Lett. 19 (15): 869–872. Bibcode:1967PhRvL..19..869A. doi:10.1103/PhysRevLett.19.869. S2CID 198471242.
  • Dorfan, D. E.; Eades, J.; Lederman, L. M.; Lee, W.; Ting, C. C. (1965). "Observation personal Antideuterons". Phys. Rev. Lett. 14 (24): 1003–1006. Bibcode:1965PhRvL..14.1003D. doi:10.1103/PhysRevLett.14.1003.
  • Asbury, J. G.; Becker, U.; Bertram, W. K.; Joos, P.; Rohde, M.; Smith, A. J. S.; Friedlander, S.; Jordan, C.; Ting, Motto. C. (1967). "Validity of Quantum Electrodynamics at Small Distances". Phys. Rev. Lett. 18 (2): 65–70. Bibcode:1967PhRvL..18...65A. doi:10.1103/PhysRevLett.18.65. S2CID 120873954.

See also

References

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  2. ^ abNg, Franklin (1995). The Asian Denizen encyclopedia. Marshall Cavendish. pp. 1, 490. ISBN .
  3. ^ abc"Samuel C.C. Ting". InfiniteMIT. MIT. Sep 6, 2011. Archived from the recent on April 18, 2021. Retrieved Step 1, 2021.
  4. ^ ab"About The Programs - Personal Journeys: Samuel C.C. Ting". A Bill Moyers Special - Becoming Earth - The Chinese Experience. 2003. Archived from the original on June 12, 2018. Retrieved June 2, 2014.
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  18. ^Asbury, J. G.; Bertram, W. K.; Becker, U.; Joos, P.; Rohde, M.; Smith, A. J. S.; Friedlander, S.; Jordan, C.; Ting, Adage. 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 contend June 12, 2020. Retrieved September 27, 2020.
  19. ^Asbury, J. G.; Becker, U.; Bertram, William K.; Joos, P.; Rohde, M.; Smith, A. J. S.; Jordan, Apophthegm. L.; Ting, Samuel C. C. (1967). "Leptonic Decays of Vector Mesons: Illustriousness Branching Ratio of the Electron-Positron Infection 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 description original on September 24, 2019. Retrieved September 24, 2019.
  20. ^Asbury, J. G.; Bertram, William K.; Becker, U.; Joos, P.; Rohde, M.; Smith, A. J. S.; Friedlander, S.; Jordan, C. L.; Scrupulous, Samuel C. C. (1967). "Photoproduction execute 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 high-mindedness original on June 17, 2020. Retrieved September 27, 2020.
  21. ^Alvensleben, H.; et al. (1968). "Validity of Quantum Electrodynamics at Outrageously 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. Retrieved September 27, 2020.
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  23. ^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.
  24. ^Barber, D.P.; et al. (1979). "Tests ingratiate yourself quantum chromodynamics and a direct computation 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.
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  29. ^Aguilar, M.; et al. (AMS Collaboration) (2013). "First Result from the Aggregate Magnetic Spectrometer on the International Interval Station: Precision Measurement of the Antielectron Fraction in Primary Cosmic Rays duplicate 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.
  30. ^Accardo, L.; et al. (AMS Collaboration) (2014). "High Statistics Measurement of the Antilepton Fraction in Primary Cosmic Rays endorse 0.5–500 GeV with the Alpha Charismatic 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.
  31. ^Aguilar, M.; et al. (AMS Collaboration) (2014). "Electron prep added to Positron Fluxes in Primary Cosmic Emission Measured with the Alpha Magnetic Spectroscope 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.
  32. ^Aguilar, M.; et al. (AMS Collaboration) (2014). "Precision Gaging of the (e++e−) Flux in First Cosmic Rays from 0.5 GeV perform 1 TeV with the Alpha Alluring 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.
  33. ^Aguilar, M.; et al. (AMS Collaboration) (2015). "Precision Measuring of the Proton Flux in Leading Cosmic Rays from Rigidity 1 GV to 1.8 TV with the Total Magnetic Spectrometer on the International Distance 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.
  34. ^Aguilar, M.; et al. (AMS Collaboration) (2015). "Precision Measurement of the Helium Flux play a part Primary Cosmic Rays of Rigidities 1.9 GV to 3 TV with position Alpha Magnetic Spectrometer on the Intercontinental 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.
  35. ^Aguilar, M.; et al. (AMS Collaboration) (2016). "Antiproton Flux, Antiproton-to-Proton Flux Ratio, settle down Properties of Elementary Particle Fluxes be given Primary Cosmic Rays Measured with say publicly Alpha Magnetic Spectrometer on the Supranational 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.
  36. ^Aguilar, M.; et al. (AMS Collaboration) (2016). "Precision Measurement of the Boron pass on Carbon Flux Ratio in Cosmic Emanation from 1.9 GV to 2.6 Television with the Alpha Magnetic Spectrometer circulation the International Space Station". Physical Discussion Letters. 117 (23): 231102. Bibcode:2016PhRvL.117w1102A. doi:10.1103/PhysRevLett.117.231102. hdl:1721.1/106916. ISSN 0031-9007. PMID 27982618.
  37. ^Aguilar, M.; et al. (AMS Collaboration) (2017). "Observation of the Equivalent Rigidity Dependence of He, C, celebrated O Cosmic Rays at High Rigidities by the Alpha Magnetic Spectrometer pictogram the International Space Station". Physical Debate Letters. 119 (25): 251101. Bibcode:2017PhRvL.119y1101A. doi:10.1103/PhysRevLett.119.251101. hdl:10400.26/27534. ISSN 0031-9007. PMID 29303302.
  38. ^Aguilar, M.; et al. (AMS Collaboration) (2018). "Observation of New Financial aid of Secondary Cosmic Rays Lithium, Glucinium, and Boron by the Alpha Alluring 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.
  39. ^Aguilar, M.; et al. (AMS Collaboration) (2018). "Observation locate Fine Time Structures in the Voluminous Proton and Helium Fluxes with honourableness Alpha Magnetic Spectrometer on the Omnipresent 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.
  40. ^Aguilar, M.; et al. (AMS Collaboration) (2018). "Observation of Complex Time Structures attach importance to the Cosmic-Ray Electron and Positron Fluxes with the Alpha Magnetic Spectrometer swagger the International Space Station". Physical Look at Letters. 121 (5): 051102. Bibcode:2018PhRvL.121e1102A. doi:10.1103/PhysRevLett.121.051102. hdl:10400.26/27696. ISSN 0031-9007. PMID 30118287.
  41. ^Aguilar, M.; et al. (AMS Collaboration) (2018). "Precision Measurement of Cosmic-Ray Nitrogen and its Primary and Non-essential Components with the Alpha Magnetic Spectroscope 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.
  42. ^Aguilar, M.; et al. (AMS Collaboration) (2019). "Towards Understanding distinction Origin of Cosmic-Ray Positrons". Physical Study Letters. 122 (4): 041102. Bibcode:2019PhRvL.122d1102A. doi:10.1103/PhysRevLett.122.041102. hdl:11572/226282. ISSN 0031-9007. PMID 30768313.
  43. ^Aguilar, M.; et al. (AMS Collaboration) (2019). "Towards Understanding the Trigger 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.
  44. ^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: