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What is Gravitational Radiation via Spin Coefficients about?

This document presents a new approach to general relativity using a tetrad or spinor formalism. It applies this formalism to two problems in radiation theory: providing a concise proof of a theorem by Goldberg and Sachs, and describing the asymptotic behavior of the Riemann tensor and metric tensor for outgoing gravitational radiation. The formalism introduces complex linear combinations of Ricci rotation coefficients that give the spinor affine connection. This allows derivation of compact equations useful

Author

Yoni Ramirez Robles

Language

EN