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Almost flat manifold

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In mathematics, a smooth compact manifold M is called almost flat if for any ε > 0 {\displaystyle \varepsilon >0} there is a Riemannian metric g ε {\displaystyle g_{\varepsilon }} on M such that diam ( M , g ε ) 1 {\displaystyle {\mbox{diam}}(M,g_{\varepsilon })\leq 1} and g ε {\displaystyle g_{\varepsilon }} is ε {\displaystyle \varepsilon } -flat, i.e. for the sectional curvature of K g ε {\displaystyle K_{g_{\varepsilon }}} we have | K g ϵ | < ε {\displaystyle |K_{g_{\epsilon }}|<\varepsilon } .

Given n, there is a positive number ε n > 0 {\displaystyle \varepsilon _{n}>0} such that if an n-dimensional manifold admits an ε n {\displaystyle \varepsilon _{n}} -flat metric with diameter 1 {\displaystyle \leq 1} then it is almost flat. On the other hand, one can fix the bound of sectional curvature and get the diameter going to zero, so the almost-flat manifold is a special case of a collapsing manifold, which is collapsing along all directions.

According to the Gromov–Ruh theorem, M is almost flat if and only if it is infranil. In particular, it is a finite factor of a nilmanifold, which is the total space of a principal torus bundle over a principal torus bundle over a torus.

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