Dirac equation, curved space time

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SUMMARY

The discussion focuses on the derivation of the Dirac equation in curved spacetime, specifically addressing the commutation relation involving the spin connection, \(\Gamma_{\mu}(x)\), and the gamma matrices, \(\gamma^{\nu}(x)\). Participants clarify that the gamma matrices are position-dependent and obey the relation \(\gamma^{\mu}\gamma^{\nu} + \gamma^{\nu}\gamma^{\mu} = 2 g^{\mu\nu}\). The covariant derivative of the gamma matrices includes correction terms from both the Christoffel symbols and the spin connection, which are essential for maintaining covariance in curved spacetime. The discussion references equations from a specific paper, highlighting the importance of understanding the commutation relations and the properties of the spin connection.

PREREQUISITES
  • Understanding of the Dirac equation and its application in quantum mechanics.
  • Familiarity with curved spacetime concepts and general relativity.
  • Knowledge of gamma matrices and their properties in quantum field theory.
  • Basic understanding of covariant derivatives and Christoffel symbols.
NEXT STEPS
  • Study the derivation of the Dirac equation in curved spacetime as presented in the referenced paper.
  • Explore the properties and applications of spin connections in general relativity.
  • Learn about the role of vierbeins in connecting local and global frames in curved spacetime.
  • Investigate the implications of local Lorentz transformations on gauge fields in quantum field theory.
USEFUL FOR

This discussion is beneficial for theoretical physicists, particularly those specializing in quantum field theory and general relativity, as well as graduate students seeking to deepen their understanding of the Dirac equation in curved spacetime.

pleasehelpmeno
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Hi when trying to derive this equation, i am stuck on:
[\Gamma_{\mu}(x),\gamma^{\nu}(x)]=\frac{\partial \gamma^{\nu}(x)}{\partial x^{\mu}} + \Gamma^{\nu}_{\mu p}\gamma^{p}.

This [\Gamma_{\mu}(x) term is the spin connection, if this is an ordinary commutator:
a) is it a fermionic so + commutator
b) how can one solve to find the Gamma term whilst cancelling away the
c) can anyone give a qualitative description of what the spin connection is?
thanks
 
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In curved space the gamma matrices are position-dependent, since they obey γμγν + γνγμ = 2 gμν. But we can and do take them to be covariantly constant.

A gamma matrix is a hybrid quantity, having one vector index, and two matrix indices referred to a tetrad basis. The covariant derivative contains a correction term for each index - a Christoffel symbol for the vector index and a spin connection (Ricci rotation coefficient) for each tetrad index.

The equation you wrote is the statement that the covariant derivative vanishes. You can take a look at this paper for more details.
 
Eqs. (8) and (9) in the paper I referred you to shows how to solve for Γμ.
 
thx,

am i right in thinking \bar{S_{ab}} is always equal to zero when b =0 because all my answers involved \bar{S_{a0}} terms?
 
sorry i should explain more,

I assumed that t^{a}_{b} is only non zero if a = b (from 0 to 3). and the same for t_{ab}.

If this is correct then all my answers for w_{abj} contain either a =0 and b=1,2,3 or vice versa meaning that when multiplied with S_{ab} then will surely go to zero if s^{0b} = 0.
Are any of these assumptions incorrect?
 
Sorry for the thread necro, but could someone please provide more details regarding eqn (8) in that reference, specifically why the commutator of the spin connection with the curved space gamma matrix is defined that way.
 
FunkyDwarf said:
Sorry for the thread necro, but could someone please provide more details regarding eqn (8) in that reference, specifically why the commutator of the spin connection with the curved space gamma matrix is defined that way.

Bill_K said:
A gamma matrix is a hybrid quantity, having one vector index, and two matrix indices referred to a tetrad basis. The covariant derivative contains a correction term for each index - a Christoffel symbol for the vector index and a spin connection (Ricci rotation coefficient) for each tetrad index.

The equation you wrote is the statement that the covariant derivative vanishes.

The covariant derivative of gamma contains a correction term for each index: a Christoffel symbol for the vector index, and a spin connection for each of the two spinor indices.

∂γν/∂xμ + Γνμρ γρ + Γμ γν - γν Γμ

Eq.(8) says that this quantity vanishes (we choose to define our γ's that way) and then the terms are rearranged slightly to make them look like a commutator.
 
It can be regarded as the gauge field generated by local Lorenz transformations. Although we find it is not independent of the metric and must be equal to combinations of vierbeins and their derivatives.

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