2018
DOI: 10.1090/tran/7658
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Geodesic-Einstein metrics and nonlinear stabilities

Abstract: In this paper, we introduce notions of nonlinear stabilities for a relative ample line bundle over a holomorphic fibration and define the notion of a geodesic-Einstein metric on this line bundle, which generalize the classical stabilities and Hermitian-Einstein metrics of holomorphic vector bundles. We introduce a Donaldson type functional and show that this functional attains its absolute minimum at geodesic-Einstein metrics, and we also discuss the relations between the existence of geodesic-Einstein metrics… Show more

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Cited by 7 publications
(8 citation statements)
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“…[24, page 82]). Combining with [19,Theorem 0.3], it shows that the existence of geodesic-Einstein metrics is equivalent to the existence of Hermitian-Einstein metrics, which is also equivalent to polystability of the holomorphic vector bundle by the Donaldson-Uhlenbeck-Yau Theorem. In the sense of this, we may identify a Hermitian-Einstein vector bundle E with a projective bundle pair (P (E), O P (E) (1)) of which admits a geodesic-Einstein metric.…”
Section: Introductionmentioning
confidence: 88%
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“…[24, page 82]). Combining with [19,Theorem 0.3], it shows that the existence of geodesic-Einstein metrics is equivalent to the existence of Hermitian-Einstein metrics, which is also equivalent to polystability of the holomorphic vector bundle by the Donaldson-Uhlenbeck-Yau Theorem. In the sense of this, we may identify a Hermitian-Einstein vector bundle E with a projective bundle pair (P (E), O P (E) (1)) of which admits a geodesic-Einstein metric.…”
Section: Introductionmentioning
confidence: 88%
“…In this section, we will recall some basic definitions and facts on geodesic-Einstein metrics of a relative ample line bundle over holomorphic fibration, and also recall Berndtsson's curvature formula of direct image bundles. For more details one may refer to [3,4,5,19,37].…”
Section: Preliminariesmentioning
confidence: 99%
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“…Remark 2: The Poisson-Kähler condition is in general stronger than the geodesic-Einstein condition in [21,44]. It is known that (see [4,41]) every relative Kähler fibration is Poisson-Kähler locally in the following sense: for every t ∈ B, there exists a small open neighborhood U of t such that the fibration from p −1 (U) to U possesses a Poisson-Kähler structure.…”
Section: Introductionmentioning
confidence: 99%