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History 181B: Modern Physics
Class 40 (4/30/03)
Renormalization
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| Outline |
Facing the infinities? Renormalized QED (continued)
War work and postwar theory
Schwinger and Tomonaga (recap)
Feynman
Disassembling
the diagrams
Reassembling
them: Perturbation theory
Thinking
out of daily experience
Los Alamos
and modularity
Assembling a full-fledged renormalized QED
A conservative response to calls for radical change
Rethinking quantum field theory
Renormalization: QED and beyond
Renormalizability as a criterion for theories
New particles, new forces
The data flood
Strategies in the face of multiplicity
The rise and fall (and rise again) of QFT |
| Names
and terms |
| Primary |
Secondary |
quantum electrodynamics (QED)
Sin-itiro Tomonaga (1906-1979), NP 1965
Julian Schwinger (1918-1994), NP 1965
Richard Feynman (1918-1988), NP 1965
propagator, vertex
perturbation theory
fine structure constant alpha = e² / h-bar c
Freeman Dyson (1923 - )
S matrix
4 forces: EM, weak, strong, gravity |
path-integral formulation
coupling constant
Fermi-field theory = 4-fermion interaction
Geoffrey Chew (1924 - ) |
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| Assignment |
Freeman J. Dyson, "Tomonaga, Schwinger, and
Feynman Awarded Nobel Prize for Physics," Science 150 (1965): 588-589.
What made Dyson consider QED so successful?
How were theory and experiment related in this episode?
Who were the radicals over which Dyson's conservatives
triumphed?
Extra: If the problems discussed here are
so complicated and messy, and three different physicists tackled it in
very different ways, how could people see that they were ultimately doing
the same thing? |
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Copyright © Cathryn Carson 2003 |