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Dirac equation in curved spacetime

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In mathematical physics, the Dirac equation in curved spacetime generalizes the original Dirac equation to curved space.

It can be written by using vierbein fields and the gravitational spin connection. The vierbein defines a local rest frame, allowing the constant Gamma matrices to act at each spacetime point. In this way, Dirac's equation takes the following form in curved spacetime:[1]

Here eaμ is the vierbein and Dμ is the covariant derivative for fermionic fields, defined as follows

where σab is the commutator of Gamma matrices:

and ωμab are the spin connection components.

The modified Klein–Gordon equation obtained by squaring the operator in the Dirac equation, first found by Erwin Schrödinger as cited by Pollock [2] is given by

where is the Ricci scalar, and is the field strength of .

Note that here Latin indices denote the "Lorentzian" vierbein labels while Greek indices denote manifold coordinate indices.

See also

References

  1. ^ Lawrie, Ian D. A Unified Grand Tour of Theoretical Physics.
  2. ^ Pollock, M.D. (2010), On the Dirac equation in curved space-time