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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?