2018
DOI: 10.1112/plms.12114
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On integrability in Grassmann geometries: integrable systems associated with fourfolds in Gr(3,5)

Abstract: Let Gr(d, n) be the Grassmannian of d-dimensional linear subspaces of an n-dimensional vector space V n . A submanifold X ⊂ Gr(d, n) gives rise to a differential system Σ(X) that governs d-dimensional submanifolds of V n whose Gaussian image is contained in X. Systems of the form Σ(X) appear in numerous applications in continuum mechanics, theory of integrable systems, general relativity and differential geometry. They include such well-known examples as the dispersionless Kadomtsev-Petviashvili equation, the … Show more

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Cited by 15 publications
(26 citation statements)
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“…This point of view has been developed in [24,57] leading to remarkable connections with integrable GL(2, R) geometry. Integrability aspects of dispersionless systems related to Grassmann geometries were recently studied in [15,16].…”
Section: Dispersionless Hirota Type Equationsmentioning
confidence: 99%
See 1 more Smart Citation
“…This point of view has been developed in [24,57] leading to remarkable connections with integrable GL(2, R) geometry. Integrability aspects of dispersionless systems related to Grassmann geometries were recently studied in [15,16].…”
Section: Dispersionless Hirota Type Equationsmentioning
confidence: 99%
“…One can verify that dω = 0. Equations (15) and (17) constitute an involutive differential system for f which characterises Monge-Ampère equations. It remains to point out that equations (17) can be obtained from the consistency of equations (15) alone, without invoking (16).…”
Section: Monge-ampère Equations In Higher Dimensions: the Defining Rementioning
confidence: 99%
“…Einstein-Weyl geometries in 3 dimensions play an important role because of its relationship with the geometry of third order ODEs (see [20] and [21]), twistor theory (see [12] and [15]) and integrable systems (see [1], [2], [4] and [11]). Let (M 3 , [g]) be a smooth conformal manifold equipped with a conformal class of metrics [g] of (pseudo)-Riemannian signature.…”
Section: Three Dimensional Einstein-weyl Geometriesmentioning
confidence: 99%
“…Let M 3 be a three dimensional smooth manifold equipped with a Lorentzian metric. A near-horizon metric on M 3 is a Lorentzian metric of the form (1) g N H = 2dν dr + rh(x)dx + r 2 2 F (x)dν + dxdx, where x, ν and r are local coordinates and h(x), F (x) are arbitrary functions of x. Near-horizon geometries in higher dimensions are studied in relation to the existence of extremal black holes [5], [14], [16], [17], [18]. The near-horizon metric (1) is derived as follows.…”
Section: Introductionmentioning
confidence: 99%
“…, x d ). In paper [5] we have initiated the study of integrability of first-order systems of the form F (u 1 , . .…”
Section: Introductionmentioning
confidence: 99%