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16 de may. de 2024 · Henri Poincaré (born April 29, 1854, Nancy, France—died July 17, 1912, Paris) was a French mathematician, one of the greatest mathematicians and mathematical physicists at the end of 19th century. He made a series of profound innovations in geometry, the theory of differential equations, electromagnetism, topology, and the ...
- Michael Freedman
Freedman was awarded the Fields Medal at the International...
- Oscar II
Oscar II was the king of Sweden from 1872 to 1907 and of...
- Poincaré Conjecture
The conjecture was made in 1904 by the French mathematician...
- Michael Freedman
Hace 2 días · Summary. Poincaré made many contributions to different fields of pure and applied mathematics such as: celestial mechanics, fluid mechanics, optics, electricity, telegraphy, capillarity, elasticity, thermodynamics, potential theory, quantum theory, theory of relativity and physical cosmology .
Hace 5 días · La Conjetura de Poincaré es una famosa hipótesis en el campo de la topología, formulada por el matemático Henri Poincaré en 1904. Trata sobre la naturaleza de las esferas tridimensionales. La conjetura establece que cualquier variedad tridimensional cerrada, simplemente conexa, es homeomorfa a una esfera tridimensional. Topología.
12 de may. de 2024 · 6. 13 views 2 hours ago SEVILLA. 🤯 ¿Conocías al pensador francés Henri Poincaré? 😱 Te presento aquí a este curioso personaje, polímata francés de principios del siglo XX, que destacó en la...
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- Alejandro Colete Moya
3 de may. de 2024 · 2 Henri Poincaré : une biographie au(x) quotidien(s), Editions Ellipses, Paris 2012.; 10 Henri Poincaré étant d'un naturel très discret, il n'est pas surprenant qu'on ne retrouve aucune trace particulière dans la presse de l'époque de sa vie à Lozère, à l'exception d'un entrefilet paru dans le journal Le Temps du 15 avril 1909, et relevé malicieusement par notre confrère et ...
Hace 2 días · An early proponent of chaos theory was Henri Poincaré. In the 1880s, while studying the three-body problem, he found that there can be orbits that are nonperiodic, and yet not forever increasing nor approaching a fixed point.
