Emergent Gravity And The Cosmological Constant Problem

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More precisely, ∂ μ \partial_{\mu} in D μ D_{\mu} must also be regarded as a background. Indeed ∂ μ \partial_{\mu} and y a / κ y^{a}/\kappa are related to each other by a ‘matrix T-duality’ hsy6 ; i ​ D μ ↔ Φ a iD_{\mu}\leftrightarrow\Phi^{a}

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