Francis Halzen

Francis Louis Halzen (born 23 March 1944 in Tienen, Belgium) is a Belgian-American particle physicist. He is the Hilldale and Gregory Breit Distinguished Professor at the University of Wisconsin-Madison and Director of its Institute for Elementary Particle Physics. Halzen is the Principal Investigator of the IceCube Neutrino Observatory at the Amundsen-Scott South Pole Station in Antarctica, the world's largest neutrino detector which has been operational since 2010.

Francis Halzen
Born23 March 1944
EducationUniversity of Louvain
Known forIceCube Neutrino Observatory
TitleHilldale and Gregory Breit Distinguished Professor
AwardsAcademia Europaea Member (2018)
Balzan Price for Astroparticle Physics (2015)
European Physical Society Prize for Astroparticle Physics and Cosmology (2015)
Smithsonian American Ingenuity Award (2014)
Physics World Breakthrough of the Year Award (2013)
American Physical Society Fellow (1995)
Scientific career
FieldsParticle physics, Neutrino physics
InstitutionsUniversity of Wisconsin-Madison
Websitehttps://icecube.wisc.edu/~halzen/

Background

Halzen was born and raised in Belgium. He graduated from the University of Louvain (UCLouvain) with a MSc Physics degree in 1966, a PhD in 1969, then his Agrégé de l'Enseignement Supérieur in 1972. Between 1969-1971 he worked as a scientific associate at CERN. Since 1972 he has been a professor at the University of Wisconsin-Madison and the Principal Investigator on the AMANDA and IceCube projects.[1][2]

Halzen is been a leading scientist in the development of cosmic ray physics and astroparticle physics since the 1970s. In addition to particle physics he published many early papers on cosmic ray anomalies and quark matter, and on relations between particle physics and cosmic rays, on particles from supernovae and on muon production in atmospheric gamma-ray showers.[3] He has served on various advisory committees, including those for the SNO, Telescope Array and Auger-upgrade experiments, the Max Planck Institutes in Heidelberg and Munich, the ICRR at the University of Tokyo, the US Particle Physics Prioritization Panel and the ApPEC particle astrophysics advisory panel in Europe.[4]

With Alan Martin he is the co-author of Quarks and Leptons, a standard text.[5]

AMANDA

Halzen first learned about attempts by Russian scientists to detect neutrinos in Antarctica, using radio antennas at their Antarctic research station to search for electric sparks resulting from cosmic neutrinos colliding with the ice.[6] After determining these interactions would be too weak to register, in 1987 he started working on the AMANDA project, which proposed burying an array of light sensors deep in the Antarctic ice which is clear, dark, stable, sterile and free of background light. This pilot experiment proved successful, however their results were marred by interference from cosmic rays as well as air bubbles in the ice. This convinced him that a much larger and deeper array would be needed, and in 2005 the AMANDA project became part of its successor project, the IceCube Neutrino Observatory.

IceCube

Halzen argued for a much larger detector, and was able to secure funding from both European and American sources. In 2005 his team started construction of the IceCube project, designed to be 100 times bigger than AMANDA, with a total size of 1 km3 and buried up to a mile and a half deep. After six years of construction, IceCube became operational in 2010.

The most important result from the IceCube was the clear break-through observation of high-energy neutrinos (about 100 times more energetic than the particles accelerated today in the world’s most powerful machine, the LHC at CERN) in 2013, from as yet not identified sources outside the Galaxy. This discovery has stimulated the planning and development of even larger neutrino telescopes, both at the South Pole and deep under the ocean.[3]


Awards

gollark: Which apparently gets much worse than a factor-of-two slowdown in practice.
gollark: Specifically, they share one radio between communicating with clients (fronthaul) and communicating with the router thing (backhaul).
gollark: Most of the available repeater things are rather bad because of contention issues.
gollark: So what is this "repeater" doing?
gollark: So now there's a cable involved?

References

  1. "Francis Halzen Full CV" (PDF). IceCube/University of Wisconsin. Retrieved 19 February 2020.
  2. "Academy of Europe: Halzen Francis". Academia Europaea. Retrieved 19 February 2020.
  3. "2015 Balzan Prize for Astroparticle Physics including neutrino and gamma-ray observation". International Balzan Prize Foundation. October 2015. Retrieved November 11, 2018.
  4. "Francis Halzen: Biographical and Bibliographical Information". International Balzan Prize Foundation. October 2015. Retrieved 19 February 2020.
  5. "Alan Martin". Fellows Directory. Royal Society. Retrieved 4 December 2018.
  6. Jayawardhana, Ray (10 December 2013). Neutrino Hunters: The Thrilling Chase for a Ghostly Particle to Unlock the Secrets of the Universe. Scientific American. ISBN 0374220638.
  7. Hamish Johnston (December 13, 2013). "Cosmic neutrinos named Physics World 2013 Breakthrough of the Year". Physics World. Retrieved November 11, 2018.
  8. "The 2015 EPS HEPP Prizes are announced". European Physical Society. April 14, 2015. Retrieved November 11, 2018.
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