2012
DOI: 10.1007/jhep09(2012)030
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Notes on emergent gravity

Abstract: Emergent gravity is aimed at constructing a Riemannian geometry from U(1) gauge fields on a noncommutative spacetime. But this construction can be inverted to find corresponding U(1) gauge fields on a (generalized) Poisson manifold given a Riemannian metric (M, g). We examine this bottom-up approach with the LeBrun metric which is the most general scalar-flat Kähler metric with a U(1) isometry and contains the Gibbons-Hawking metric, the real heaven as well as the multi-blown up Burns metric which is a scalar-… Show more

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Cited by 16 publications
(24 citation statements)
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“…We are also trying to find out interesting 1+1 dimensional or 2+1 dimensional DH type systems that can be solved using inverse scattering transform and can be studied to uncover several widely known aspects of integrability. Another testing ground could be various scalar flat Kähler metrics namely the LeBrun metric with U (1) isometry that contains Gibbons-Hawking, Real heaven and Burns metric as special limits and were used to test the bottomup approach of emergent gravity [49]. Using monodromy evolving deformation [50] on Plebanski type self dual Einstein equations which are actually the EOM obtained from the 2-dim chiral U (N ) model in the large N limit and studying integrability might clarify some important issues for the test of emergent gravity [51].…”
Section: Discussionmentioning
confidence: 99%
“…We are also trying to find out interesting 1+1 dimensional or 2+1 dimensional DH type systems that can be solved using inverse scattering transform and can be studied to uncover several widely known aspects of integrability. Another testing ground could be various scalar flat Kähler metrics namely the LeBrun metric with U (1) isometry that contains Gibbons-Hawking, Real heaven and Burns metric as special limits and were used to test the bottomup approach of emergent gravity [49]. Using monodromy evolving deformation [50] on Plebanski type self dual Einstein equations which are actually the EOM obtained from the 2-dim chiral U (N ) model in the large N limit and studying integrability might clarify some important issues for the test of emergent gravity [51].…”
Section: Discussionmentioning
confidence: 99%
“…However, it seems to be difficult to write down Eq. (4.43) as a local form in terms of symplectic U(1) gauge fields [42]. Now we are ready to discuss how the cosmological constant problem can be resolved in emergent gravity.…”
Section: Matrix Model and Quantum Gravitymentioning
confidence: 99%
“…Recently works in emergent gravity [39] aim at constructing a Riemannian geometry from U (1) gauge fields on a noncommutative spacetime. This construction is invertible to find corresponding U (1) gauge fields on a (generalized) Poisson manifold given a metric (M, g).…”
Section: Hyperkähler Structure and The Ky Tensorsmentioning
confidence: 99%