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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 - )
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? 

Copyright © Cathryn Carson 2003