We study the shear dynamics of higher dimensional
Friedmann-Lema\^{i}tre-Robertson-Walker (FLRW) cosmology by considering a
non-perfect fluid which exerts different pressure in the normal and extra
dimensions. We generalise the definition of shear tensor for higher dimensional
space-time and prove it to be consistent with the evolution equation for shear
tensor obtained from the Ricci identities. The evolution of shear tensor is
investigated numerically. The role of extra dimensions and other parameters
involved in shear dynamics is discussed in detail. We find that with increase
in anisotropy parameter, time of decay of shear increases while with increase
in number of extra dimensions, shear tends to decay early.Comment: 8 pages, 3 figures, comments welcom