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Lecture 28.

Handouts:

Midsemester Grade Summary.

Today we showed that the Dirac Lagrangian is Lorentz-invariant, and rewrote both it and the Dirac equation in a manifestly Lorentz-covariant form.

We recalled how tex2html_wrap_inline20 transforms under rotations and boosts in the Weyl basis, with the only two bilinear products invariant under both being tex2html_wrap_inline22 and tex2html_wrap_inline24 . We then showed that the mass term tex2html_wrap_inline26 gave the sum of precisely those two Lorentz-invariant terms.

We defined the Dirac adjoint tex2html_wrap_inline28 as a dual to tex2html_wrap_inline30 ; that is, we defined tex2html_wrap_inline32 so that the product tex2html_wrap_inline34 always gives a scalar. This is just as we defined 4-covectors to absorb the matrix tex2html_wrap_inline36 necessary to obtain Lorentz-invariant inner products between 4-vectors.

This feature of transforming exactly opposite to the the way that tex2html_wrap_inline38 transforms is so useful that we rewrite our Lagrangian to involve only tex2html_wrap_inline40 and tex2html_wrap_inline42 . We then considered the gradient term in the Lagrangian, and rewrote it as tex2html_wrap_inline44 , where tex2html_wrap_inline46 We then showed that the bilinear tex2html_wrap_inline48 transforms under Lorentz transformations as a spacetime 4-vector: that the Lorentz transformation matrices acting on tex2html_wrap_inline50 and tex2html_wrap_inline52 in spin space induce an effective Lorentz transformation of the spacetime indices tex2html_wrap_inline54 of tex2html_wrap_inline56 . Thus the gradient term in the Lagrangian, tex2html_wrap_inline58 , transforms as a Lorentz scalar, with tex2html_wrap_inline60 transforming in the opposite direction as tex2html_wrap_inline62 in spacetime.

Finally we introduced the Feynman slash notation, writing the Dirac equation in its compact, manifestly Lorentz-covariant form tex2html_wrap_inline64 .

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Katherine Benson
Fri Mar 29 16:49:49 EST 1996