Integrable Flows for Starlike Curves in Centroaffine Space

We construct integrable hierarchies of flows for curves in centroaffine R³ through a natural pre-symplectic structure on the space of closed unparametrized starlike curves. We show that the induced evolution equations for the differential invariants are closely connected with the Boussinesq hierarch...

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Бібліографічні деталі
Дата:2013
Автори: Calini, A., Ivey, T., Beffa, G.M.
Формат: Стаття
Мова:English
Опубліковано: Інститут математики НАН України 2013
Назва видання:Symmetry, Integrability and Geometry: Methods and Applications
Онлайн доступ:http://dspace.nbuv.gov.ua/handle/123456789/149224
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:Integrable Flows for Starlike Curves in Centroaffine Space / A. Calini, T. Ivey, G.M. Beffa // Symmetry, Integrability and Geometry: Methods and Applications. — 2013. — Т. 9. — Бібліогр.: 30 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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spelling irk-123456789-1492242019-02-20T01:26:45Z Integrable Flows for Starlike Curves in Centroaffine Space Calini, A. Ivey, T. Beffa, G.M. We construct integrable hierarchies of flows for curves in centroaffine R³ through a natural pre-symplectic structure on the space of closed unparametrized starlike curves. We show that the induced evolution equations for the differential invariants are closely connected with the Boussinesq hierarchy, and prove that the restricted hierarchy of flows on curves that project to conics in RP² induces the Kaup-Kuperschmidt hierarchy at the curvature level. 2013 Article Integrable Flows for Starlike Curves in Centroaffine Space / A. Calini, T. Ivey, G.M. Beffa // Symmetry, Integrability and Geometry: Methods and Applications. — 2013. — Т. 9. — Бібліогр.: 30 назв. — англ. 1815-0659 2010 Mathematics Subject Classification: 37K10; 53A20; 53C44 DOI: http://dx.doi.org/10.3842/SIGMA.2013.022 http://dspace.nbuv.gov.ua/handle/123456789/149224 en Symmetry, Integrability and Geometry: Methods and Applications Інститут математики НАН України
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
description We construct integrable hierarchies of flows for curves in centroaffine R³ through a natural pre-symplectic structure on the space of closed unparametrized starlike curves. We show that the induced evolution equations for the differential invariants are closely connected with the Boussinesq hierarchy, and prove that the restricted hierarchy of flows on curves that project to conics in RP² induces the Kaup-Kuperschmidt hierarchy at the curvature level.
format Article
author Calini, A.
Ivey, T.
Beffa, G.M.
spellingShingle Calini, A.
Ivey, T.
Beffa, G.M.
Integrable Flows for Starlike Curves in Centroaffine Space
Symmetry, Integrability and Geometry: Methods and Applications
author_facet Calini, A.
Ivey, T.
Beffa, G.M.
author_sort Calini, A.
title Integrable Flows for Starlike Curves in Centroaffine Space
title_short Integrable Flows for Starlike Curves in Centroaffine Space
title_full Integrable Flows for Starlike Curves in Centroaffine Space
title_fullStr Integrable Flows for Starlike Curves in Centroaffine Space
title_full_unstemmed Integrable Flows for Starlike Curves in Centroaffine Space
title_sort integrable flows for starlike curves in centroaffine space
publisher Інститут математики НАН України
publishDate 2013
url http://dspace.nbuv.gov.ua/handle/123456789/149224
citation_txt Integrable Flows for Starlike Curves in Centroaffine Space / A. Calini, T. Ivey, G.M. Beffa // Symmetry, Integrability and Geometry: Methods and Applications. — 2013. — Т. 9. — Бібліогр.: 30 назв. — англ.
series Symmetry, Integrability and Geometry: Methods and Applications
work_keys_str_mv AT calinia integrableflowsforstarlikecurvesincentroaffinespace
AT iveyt integrableflowsforstarlikecurvesincentroaffinespace
AT beffagm integrableflowsforstarlikecurvesincentroaffinespace
first_indexed 2023-05-20T17:32:16Z
last_indexed 2023-05-20T17:32:16Z
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