arXiv (OAI Expanded)
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Intrinsic pressure anisotropy in spherical Proca stars
general-relativity-and-quantum-cosmologyhigh-energy-astrophysical-phenomenahigh-energy-physics-phenomenologyhigh-energy-physics-theory
Pressure anisotropy in relativistic stars is commonly prescribed through a phenomenological closure, obscuring its microscopic origin and relation to stress-energy conservation. Here it is derived directly from the minimally coupled Einstein-complex-Proca theory. For spherical Proca stars, the princ
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