Proof of Local Lorentz Invariance of Feynman Propagator in Curved Spaces

In summary: Your Name]In summary, the Feynman propagator is locally Lorentz invariant for scalar fields in curved space-times, as proven in sources such as the book "Quantum Field Theory in Curved Spacetime and Black Hole Thermodynamics" by Robert M. Wald and the paper "Quantum Field Theory on Curved Spacetimes: Concepts and Mathematical Foundations" by Christian Gerard. The proof relies on the fact that the Feynman propagator is a Green's function, which is a solution to the Klein-Gordon equation that is invariant under local Lorentz transformations.
  • #1
Thor90
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I am looking for a proof that the Feynman propagator is locally a lorentz invariant (at least for scalar fields) also in curved space-times if the background geometry is smooth enough.
I mean, since it is of course a lorentz invariant on flat spaces, this should also be true if a choose a sufficiently small portion of the space and the background geometry is sufficiently smooth, even if it should contain non-local terms when evaluated between well distanced spacetime points.
Some advice on where I can find something like that?
 
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  • #2


Hello,

Thank you for your question. The proof that the Feynman propagator is locally Lorentz invariant for scalar fields in curved space-times can be found in several sources.

One of the most commonly cited sources is the book "Quantum Field Theory in Curved Spacetime and Black Hole Thermodynamics" by Robert M. Wald. In Chapter 2, he discusses the invariance of the Feynman propagator under local Lorentz transformations in curved space-time.

Another source is the paper "Quantum Field Theory on Curved Spacetimes: Concepts and Mathematical Foundations" by Christian Gerard. In Section 3.3, he discusses the local Lorentz invariance of the Feynman propagator in curved space-time.

In general, the proof relies on the fact that the Feynman propagator is a Green's function, which is a solution to the Klein-Gordon equation. The Klein-Gordon equation is a relativistic wave equation that is invariant under local Lorentz transformations.

I hope this helps. Good luck with your research!
 

1. What is the Feynman propagator?

The Feynman propagator is a mathematical tool used in quantum field theory to calculate the probability amplitude for a particle to move from one point to another in space and time. It is an essential component in the calculation of scattering processes and interactions between particles.

2. How does the Feynman propagator relate to local Lorentz invariance?

The Feynman propagator is a fundamental quantity that must remain invariant under local Lorentz transformations, which describe how the laws of physics are the same for all observers in different reference frames. This is because the propagator is used in calculations involving particles moving at relativistic speeds, and the laws of physics must hold true for all observers, regardless of their relative motion.

3. What is the significance of proving local Lorentz invariance of the Feynman propagator in curved spaces?

The proof of local Lorentz invariance of the Feynman propagator in curved spaces is essential in understanding the behavior of particles in the presence of gravity. In general relativity, space and time are curved by the presence of massive objects, and the Feynman propagator must be able to account for this curvature in order to accurately describe particle interactions in curved space.

4. How is the proof of local Lorentz invariance of the Feynman propagator in curved spaces accomplished?

The proof is typically accomplished by using mathematical techniques such as perturbation theory and Feynman diagrams to calculate the propagator in curved space. These calculations are then compared to the propagator in flat space and must yield the same results to prove local Lorentz invariance.

5. Why is the proof of local Lorentz invariance of the Feynman propagator important in the context of quantum gravity?

The proof is significant in the context of quantum gravity because it provides a framework for understanding how particles behave in the presence of both quantum mechanics and general relativity. This is crucial for developing a theory of quantum gravity, which seeks to unify these two fundamental theories of physics to describe the behavior of particles at the smallest scales in the universe.

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