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Gravitational vacuum polarization
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The energy conditions of classical Einstein gravity fail once quantum effects are introduced. These quantum violations of the energy conditions are not subtle high-energy Planck scale effects. Rather the quantum violations of the energy conditions already occur in semiclassical quantum gravity and are first-order O(\hbar) effects. Quantum violations of the energy conditions are widespread, albeit small.
Forward citations
Cited by 2 Pith papers
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Imprints of quantum vacuum fluctuations on the gravitational field of a spherical mass
Under stated assumptions on the quantum vacuum energy density, static spherically symmetric semiclassical spacetimes generically replace Killing horizons with wormhole throats.
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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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