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Arthur Bruce McDonald, CC OOnt ONS FRS FRSC P.Eng, (born August 29, 1943) is a Canadian astrophysicist. McDonald is the director of the Sudbury Neutrino Observatory Collaboration and held the Gordon and Patricia Gray Chair in Particle Astrophysics at Queen's University in Kingston, Ontario from 2006 to 2013. He was awarded the 2015 Nobel Prize in Physics jointly with Japanese physicist Takaaki Kajita.

Arthur B. McDonald
CC OOnt ONS FRS FRSC
Arthur B. McDonald 5193-2015.jpg
Arthur B. McDonald in Stockholm in December 2015
Born Arthur Bruce McDonald
(1943-08-29) August 29, 1943 (age 74)
North Sydney, Nova Scotia
Residence Kingston, Ontario
Nationality Canadian
Alma mater
Known for Solving the solar neutrino problem
Awards
Website queensu.ca/physics/arthur-mcdonald
Scientific career
Fields Astrophysics
Institutions
Thesis Excitation energies and decay properties of T = 3/2 states in 17O, 17F and 21Na. (1970)
Doctoral advisor William Alfred Fowler

Contents

Early lifeEdit

McDonald was born on August 29, 1943,[1] in Sydney, Nova Scotia.[3] He graduated with a B.Sc. in physics in 1964 and M.Sc. in physics in 1965 from Dalhousie University in Nova Scotia.[4] He then obtained his Ph.D. in physics in 1969 from the California Institute of Technology.[5]

Academic careerEdit

McDonald worked as a Research Officer at the Chalk River Nuclear Laboratories northwest of Ottawa from 1969 to 1982. He became professor of physics at Princeton University from 1982 to 1989, leaving Princeton to join Queen's University where he became Professor from 1989 to 2013. in 2013 McDonald became Professor Emeritus of Queen's University in Kingston, Canada. He continues to be active in basic research in Neutrinos and Dark Matter at the SNOLAB underground Laboratory and as member of the Board of the Perimeter Institute for Theoretical Physics.[4][6][7]

ResearchEdit

McDonald presenting himself and his research

Physicists have been investigating whether or not neutrinos have mass. Since the late 1960s, experiments have hinted that neutrinos may have mass. Theoretical models of the Sun predict that neutrinos should be made in large numbers. Neutrino detectors on the Earth have repeatedly seen fewer than the expected number of neutrinos. Because neutrinos come in three varieties (electron, muon, and tau neutrinos), and because solar neutrino detectors have been primarily sensitive only to electron neutrinos, the preferred explanation over the years is that those "missing" neutrinos had changed, or oscillated, into a variety for which the detectors had little or no sensitivity. If a neutrino oscillates, according to the laws of quantum mechanics, then it must have a mass.[6]

In 1984, McDonald's collaborator Herb Chen at the University of California at Irvine suggested the advantages of using heavy water as a detector for solar neutrinos.[8] Unlike previous detectors, using heavy water would make the detector sensitive to two reactions, one reaction sensitive to all neutrino flavours, the other sensitive to only the electron neutrino. Thus, such a detector could measure neutrino oscillations directly. Chen, McDonald, and collaborators formed the Sudbury Neutrino Observatory (SNO) to exploit this idea in 1984.[9][10] SNO was to be a detector facility using 1000 tonnes of heavy water located 6,800 feet (2,100 m) underground in a mine outside Sudbury, Ontario. Chen died of leukemia in November 1987, however.

In August 2001, the Sudbury Neutrino Observatory, now led by McDonald, reported observations that directly suggested electron neutrinos from the Sun were oscillating into muon and tau neutrinos. McDonald is a co-recipient of the 2007 Benjamin Franklin Medal in Physics, the 2015 Nobel Prize in Physics, and the 2015 Fundamental Physics Prize for the discovery of neutrino oscillations and demonstrating that neutrinos have mass.[5][11]

Honours and awardsEdit

ReferencesEdit

  1. ^ a b c McDonald, Prof. Arthur Bruce. ukwhoswho.com. Who's Who. 2015 (online Oxford University Press ed.). A & C Black, an imprint of Bloomsbury Publishing plc.    (subscription required)
  2. ^ a b "Arthur McDonald biography". Royal Society. Retrieved 2015-10-09. 
  3. ^ "Past Winner 2003 NSERC Award of Excellence McDonald". Natural Sciences and Engineering Research Council of Canada. Retrieved 2012-09-21. 
  4. ^ a b "CV Arthur B. McDonald" (PDF). www.queensu.ca. 
  5. ^ a b c "Arthur B. McDonald". www.fi.edu. The Franklin Institute. Retrieved 6 October 2015. 
  6. ^ a b "Interview with Arthur B. McDonald". Archived from the original on 17 November 2007. Retrieved 2007-11-02. 
  7. ^ "Board of Directors". Perimeter Institute. 2012. Retrieved 2015-10-09. 
  8. ^ Chen, Herbert H. (September 1985). "Direct Approach to Resolve the Solar-Neutrino Problem". Physical Review Letters. 55 (14): 1534–1536. Bibcode:1985PhRvL..55.1534C. doi:10.1103/PhysRevLett.55.1534. 
  9. ^ Ewan, G.T.; Davidson, W.F. (2005). "Early Development of the Underground SNO Laboratory in Canada" (PDF). Physics in Canada. 61: 339–346, 347–350. Retrieved 13 December 2016. 
  10. ^ "The Nobel Prize in Physics 2015". Retrieved 2016-12-15. 
  11. ^ Spears, Tom (9 November 2015). "Neutrino Nobel winner Art McDonald nabs second big physics prize". Ottawa Citizen. Retrieved 9 November 2015. 
  12. ^ "Order of Canada citation". 
  13. ^ "Henry Marshall Tory Medal". Royal Society of Canada. Retrieved 2012-09-21. 
  14. ^ "The Nobel Prize in Physics 2015". www.nobelprize.org. 
  15. ^ "Order of Canada Appointments". The Governor General of Canada His Excellency the Right Honourable David Johnston. Governor General of Canada. Retrieved 31 December 2015. 
  16. ^ National Academy of Sciences Members and Foreign Associates Elected, News from the National Academy of Sciences, National Academy of Sciences, May 3, 2016, retrieved 2016-05-14 .
  17. ^ "Order of Nova Scotia". Retrieved 2016-12-08. 
  18. ^ "University of Toronto". Retrieved 2017-06-14. 

External linksEdit