1992
DOI: 10.2307/2374768
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Complex Monge-Ampere and Symplectic Manifolds

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Cited by 262 publications
(339 citation statements)
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“…0). The positivity of D then follows from a computation in [27], but we will give the short argument here too. Let Φ = i∂∂φ where the ∂∂-operator acts on t 1 and the z-variables, the remaining t-variables being fixed.…”
Section: The Proof Of Theorem 11mentioning
confidence: 99%
See 2 more Smart Citations
“…0). The positivity of D then follows from a computation in [27], but we will give the short argument here too. Let Φ = i∂∂φ where the ∂∂-operator acts on t 1 and the z-variables, the remaining t-variables being fixed.…”
Section: The Proof Of Theorem 11mentioning
confidence: 99%
“…Now consider our space X above and let U = {|Re t| < 1} be a strip, and consider functions ψ that depend only on Re t. Then 4C(ψ) =ψ − |∂ zψ | 2 φ if we use dots to denote derivatives with respect to Re t. The link between Theorem 1.2 and the papers cited above lies in the fact that, by the results in [27], the right-hand side here is the geodesic curvature of the path in K(L) determined by ψ.…”
Section: The Space Of Kähler Metricsmentioning
confidence: 99%
See 1 more Smart Citation
“…To prove the theorem we first apply the observation of Donaldson [10], Mabuchi [19] and Semmes [24], which shows that solving the geodesic equation on H is equivalent to solving the degenerate Monge-Ampère equation…”
Section: Introductionmentioning
confidence: 99%
“…Well-known examples of such gravitational actions are the Liouville [1], Mabuchi and Aubin-Yau actions [2][3][4][5], as well as the cosmological constant action S c [g 0 , g] = µ 0 d 2 x( √ g − √ g 0 ) = µ 0 (A − A 0 ). While the Liouville action is formulated entirely in terms of g 0 and the conformal factor σ (defined as g = e 2σ g 0 ), the Mabuchi and Aubin-Yau actions crucially involve also directly the Kähler potential φ.…”
Section: Jhep11(2017)154mentioning
confidence: 99%