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[Emeriti-faculty] Department of Physics and Astronomy Colloquium Information



Dear Physics & Astronomy Department Colleagues:

On Friday, Feb. 26th we will be having a distinguished visitor and Colloquium speaker. Chris Quigg has been head of the Theoretical Physics Division at Fermilab, Professor at the University of Chicago, Chair of DPF, and a member of many national advisory panels. He was a student of J.D. Jackson, a point of interest for those of us, almost all, who may have struggled through “Classical Electrodynamics”. Our plans for the day are a visit with the high energy physics group at STC in the morning, a meeting with our cosmology group around 12:30 in Robinson 258, and a department light lunch for everyone at 1:30 p.m. in the Knipp Library in Robinson Hall. Lunch will be followed by the Colloquium at 2:30. Please mark your calendar.

Jack , for the Colloquium Committee

Feb. 26, 2010 – Lunch, 1:30 p.m., Robinson 251
Colloquium, 2:30 p.m. – Nelson Auditorium, Anderson Hall
The Coming Revolutions in Particle Physics
Chris Quigg
Theoretical Physics Department
Fermi National Accelerator Laboratory

Abstract:

Soon, the Large Hadron Collider at CERN will advance the experimental frontier of particle physics to the heart of the Fermi scale, reaching energies around one trillion electron volts for collisions among the basic constituents of matter. We do not know what the new wave of exploration will find, but the discoveries we make and the new puzzles we encounter are certain to change the face of particle physics and echo through neighboring sciences. In this new world, we confidently expect to learn what sets electromagnetism apart from the weak interactions, with profound implications for our conception of the everyday world. We will gain a new understanding of simple and profound questions: Why are there atoms? Why chemistry? What makes stable structures possible? A pivotal step will be finding the Higgs boson and exploring its properties. But there may be much more: we have hints of other new phenomena, including some that may clarify why gravity is so much weaker than the other fundamental forces. We also have reason to believe that candidates for the dark matter of the Universe could be lurking on the Fermi scale. Beyond the Fermi scale lies the prospect of other new insights: into the different forms of matter, the unity of quarks and leptons, and the nature of spacetime. The questions in play all seem linked to one another—and to the relationship of the weak and electromagnetic interactions. Where will the revolutions end?