Need flat spacetime to define mass and spin?

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SUMMARY

The discussion centers on the necessity of a flat background metric for defining mass and spin in the context of General Relativity (GR). According to Wald, mass and spin are linked to the Casimir operators of the restricted Poincaré group, which governs the symmetries of flat spacetime. In the linear approximation of GR, a flat metric is present, allowing for the definition of these properties, but this is not the case in the full theory where curvature complicates the framework.

PREREQUISITES
  • Understanding of General Relativity (GR)
  • Familiarity with the Poincaré group and its symmetries
  • Knowledge of Casimir operators in quantum field theory
  • Basic concepts of metric tensors and spacetime curvature
NEXT STEPS
  • Study the implications of flat spacetime in General Relativity
  • Explore the role of Casimir operators in quantum field theory
  • Investigate the differences between linear and full theories of GR
  • Learn about the isometry groups of various spacetime geometries
USEFUL FOR

The discussion is beneficial for theoretical physicists, researchers in quantum field theory, and students of General Relativity seeking to understand the relationship between spacetime geometry and physical properties like mass and spin.

copernicus1
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In his book on GR, Wald writes "the notion of the mass and spin of a field requires the presence of a flat background metric...which one has in the linear approximation but not in the full theory..."

Why do we need a flat background metric to define a field's mass and spin?
 
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Mass and spin are essentially the 2 Casimirs of the (restricted) Poincare' group, which is the isometry group of a flat space-time.
 

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