On three-dimensional anti-de Sitter spacetime, the renormalized stress-energy tensor of a nonminimally coupled quantum scalar field can violate the weak and null energy conditions in both vacuum and thermal states, depending on mass, coupling, and boundary conditions.
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Re-derivation of the constant-density star in isotropic coordinates produces a transparent metric and highlights under-appreciated special cases including pressure gravitating alone and naked singularities.
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Nonminimal coupling, quantum scalar field stress-energy tensor and energy conditions on global anti-de Sitter space-time
On three-dimensional anti-de Sitter spacetime, the renormalized stress-energy tensor of a nonminimally coupled quantum scalar field can violate the weak and null energy conditions in both vacuum and thermal states, depending on mass, coupling, and boundary conditions.
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Revisiting Schwarzschild's constant density star in isotropic coordinates
Re-derivation of the constant-density star in isotropic coordinates produces a transparent metric and highlights under-appreciated special cases including pressure gravitating alone and naked singularities.
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