It has recently been demonstrated that the dynamics of black holes at large
can be recast as a set of non gravitational membrane equations. These
membrane equations admit a simple static solution with shape $S^{D-p-2} \times
R^{p,1}$. In this note we study the equations for small fluctuations about this
solution in a limit in which amplitude and length scale of the fluctuations are
simultaneously scaled to zero as is taken to infinity. We demonstrate that
the resultant nonlinear equations, which capture the Gregory- Laflamme
instability and its end point, exactly agree with the effective dynamical
black brane' equations of Emparan Suzuki and Tanabe. Our results thus identify the black brane’ equations as a special limit of the membrane equations and so
unify these approaches to large black hole dynamics.

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