Dirac equation in curvilinear coordinates

paweld
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I wonder how Dirac equation transform under change of coordinates (in flat spacetime).
Should I simply express partial derivaties of one coordinates in another or it is
necessary to transform Dirac matrices as well?
 
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There's a good review paper

Brill & Wheeler, Rev Mod Phys 29 (1957) 465

and many others subsequently, one off the top of my head is

Chamseddine, hep-th/0511074 (2005)


I'm a bit rusty on the details but I recall the Dirac matrices have to change so that the anticommutator relation
<br /> \gamma^\mu \gamma^\nu + \gamma^\nu \gamma^\mu = 2 g^{\mu\nu}<br />
remains true. There is some sort of spinor connection which is a spinor analog of the covariant derivative.



Dave
 
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