General Relativity (GR) does not explicitly account for angular momentum and rotational stress within its framework, as the stress-energy tensor Tμν lacks terms for these factors. The discussion highlights the relationship between angular momentum and the stress-energy tensor, suggesting a density for orbital angular momentum defined as Nσμν = xσ Tμν - xμ Tσν. However, it is noted that this definition is only applicable in flat space, indicating limitations in the application of angular momentum concepts in curved spacetime.
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