Einstein manifold

Results: 30



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11Nonlocal gravity, Schwinger-Keldysh technique, dark energy and all that A. O. Barvinskya ∗ a  Theory Department, Lebedev Physics Institute

Nonlocal gravity, Schwinger-Keldysh technique, dark energy and all that A. O. Barvinskya ∗ a Theory Department, Lebedev Physics Institute

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Source URL: quarks.inr.ac.ru

Language: English - Date: 2014-08-28 10:24:16
12ESI  The Erwin Schr¨ odinger International Institute for Mathematical Physics

ESI The Erwin Schr¨ odinger International Institute for Mathematical Physics

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Source URL: www.esi.ac.at

Language: English - Date: 2014-07-14 08:15:33
13ESI  The Erwin Schr¨ odinger International Institute for Mathematical Physics

ESI The Erwin Schr¨ odinger International Institute for Mathematical Physics

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Source URL: www.esi.ac.at

Language: English - Date: 2014-07-14 08:15:33
14¨ THE ETA INVARIANT IN THE DOUBLY KAHLERIAN CONFORMALLY COMPACT EINSTEIN CASE GIDEON MASCHLER Abstract. On a 3-manifold bounding a compact 4-manifold, let a conformal structure be induced from a complete Einstein metric

¨ THE ETA INVARIANT IN THE DOUBLY KAHLERIAN CONFORMALLY COMPACT EINSTEIN CASE GIDEON MASCHLER Abstract. On a 3-manifold bounding a compact 4-manifold, let a conformal structure be induced from a complete Einstein metric

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Source URL: mathcs.clarku.edu

Language: English - Date: 2014-08-12 14:55:57
15Conformally K¨ahler base metrics for Einstein warped products Gideon Maschler1, Department of Mathematics and Computer Science, Clark University, Worcester, MA 01610, U.S.A. Abstract A Riemannian metric 𝑔 with Ricci

Conformally K¨ahler base metrics for Einstein warped products Gideon Maschler1, Department of Mathematics and Computer Science, Clark University, Worcester, MA 01610, U.S.A. Abstract A Riemannian metric 𝑔 with Ricci

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Source URL: mathcs.clarku.edu

Language: English - Date: 2014-08-12 14:55:57
16Week 8 (due May[removed]a) Let M be a K¨ahler manifold with K¨ahler metric gi¯j . Show that the only nonvanishing components of the Riemann tensor are Ri¯jk¯l = −R¯jik¯l = −Ri¯jk¯l = R¯ji¯lk . Show that mi

Week 8 (due May[removed]a) Let M be a K¨ahler manifold with K¨ahler metric gi¯j . Show that the only nonvanishing components of the Riemann tensor are Ri¯jk¯l = −R¯jik¯l = −Ri¯jk¯l = R¯ji¯lk . Show that mi

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Source URL: www.theory.caltech.edu

Language: English - Date: 2009-05-21 13:17:42
17¨ REMARKS ON SOME NON-LINEAR HEAT FLOWS IN KAHLER GEOMETRY Donovan C. McFeron

¨ REMARKS ON SOME NON-LINEAR HEAT FLOWS IN KAHLER GEOMETRY Donovan C. McFeron

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Source URL: www.math.columbia.edu

Language: English - Date: 2009-06-15 15:10:20
18On the Mean Curvature Flow of Graphs of Symplectomorphisms of K¨ahler-Einstein Manifolds; Application to Complex Projective Spaces Ivana Medoˇs

On the Mean Curvature Flow of Graphs of Symplectomorphisms of K¨ahler-Einstein Manifolds; Application to Complex Projective Spaces Ivana Medoˇs

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Source URL: www.math.columbia.edu

Language: English - Date: 2009-09-01 13:55:39
19Department of Mathematics University of North Carolina at Chapel Hill The 2014 Alfred Brauer Lectures SIMON DONALDSON Simons Centre

Department of Mathematics University of North Carolina at Chapel Hill The 2014 Alfred Brauer Lectures SIMON DONALDSON Simons Centre

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Source URL: math.unc.edu

Language: English - Date: 2014-03-03 10:19:30
20Microsoft PowerPoint - AALBORGTALK-FINAL

Microsoft PowerPoint - AALBORGTALK-FINAL

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Source URL: www.physics.rutgers.edu

Language: English - Date: 2012-08-07 16:30:25