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Holographic Neutron Stars
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We construct in the context of the AdS/CFT correspondence degenerate composite operators in the conformal field theory that are holographically dual to degenerate stars in anti de Sitter space. We calculate the effect of the gravitational back-reaction using the Tolman-Oppenheimer-Volkoff equations, and determine the "Chandrasekhar limit" beyond which the star undergoes gravitational collapse towards a black hole.
Forward citations
Cited by 2 Pith papers
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Bouncing singularities and thermal correlators on line defects
Retarded correlators of displacement operators on line defects in holographic thermal CFTs exhibit bouncing singularities that match between interior-sensitive WKB and boundary-only OPE analyses.
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A smooth road to bumpy horizons: shaping black holes with non-linear sigma models, from supergravity to higher dimensions
Potential-free non-linear sigma models in General Relativity support static 'bumpy-horizon' black holes, with the horizon conformal factor determined by an inhomogeneous Liouville equation sourced by arbitrary holomor...
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