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Qu'est-ce (qui) est quadruple summation - définition
SHORTHAND NOTATION FOR TENSOR OPERATIONS
Einstein summation convention; Einstein summation notation; Einstein summation; Einstein convention; Einstein's summation convention; Summation convention; Einstein rule; Einstein Summation convention
Duple and quadruple metre
MUSICAL METRE
2/4 time; Duple metre; Duple time; Binary measure; Quadruple meter; Quadruple time; Binary meter; Duple meter; Four-beat; Duple and quadruple meter; Quadruple-time; Binary metre
Duple metre (or Am. duple meter, also known as duple time) is a musical metre characterized by a primary division of 2 beats to the bar, usually indicated by 2 and multiples (simple) or 6 and multiples (compound) in the upper figure of the time signature, with (cut time), , and (at a fast tempo) being the most common examples.
Einstein notation
In mathematics, especially in applications of linear algebra to physics, Einstein notation (also known as the Einstein summation convention or Einstein summation notation) is a notational convention that implies summation over a set of indexed terms in a formula, thus achieving brevity. As part of mathematics it is a notational subset of Ricci calculus; however, it is often used in physics applications that do not distinguish between tangent and cotangent spaces.
Rowing at the 2008 Summer Olympics – Women's quadruple sculls
ROWING EVENT
Rowing at the 2008 Summer Olympics - Women's quadruple sculls
Women's quadruple sculls competition at the 2008 Summer Olympics in Beijing was held between August 10 and 17, at the Shunyi Olympic Rowing-Canoeing Park.
Wikipédia
Einstein notation
In mathematics, especially the usage of linear algebra in mathematical physics, Einstein notation (also known as the Einstein summation convention or Einstein summation notation) is a notational convention that implies summation over a set of indexed terms in a formula, thus achieving brevity. As part of mathematics it is a notational subset of Ricci calculus; however, it is often used in physics applications that do not distinguish between tangent and cotangent spaces. It was introduced to physics by Albert Einstein in 1916.
