2009

Null Geodesic Congruences, Asymptotically Flat Space-Times and Their Physical Interpretation

Adamo, T. M., Newman, E. T., Kozameh, C. N.

Understand

Shear-free or asymptotically shear-free null geodesic congruences possess a large number of fascinating geometric properties and to be closely related, in the context of general relativity, to a variety of physically significant affects.

  • It is the purpose of this paper to develop these issues and find applications in GR.
  • The applications center around the problem of extracting interior physical properties of an asymptotically flat space-time directly from the asymptotic gravitational (and Maxwell) field itself in analogy with the determination of total charge by an integral over the Maxwell field at infinity or the identification of the interior mass (and its loss) by (Bondi's) integrals of the Weyl tensor, also at infinity.
  • More specifically we will see that the asymptotically shear-free congruences lead us to an asymptotic definition of the center-of-mass and its equations of motion.

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