In physics, the gyration tensor is a tensor that describes the second moments of position of a collection of particles
S m n = d e f 1 N ∑ i = 1 N r m ( i ) r n ( i ) {\displaystyle S_{mn}\ {\stackrel {\mathrm {def} }{=}}\ {\frac {1}{N}}\sum _{i=1}^{N}r_{m}^{(i)}r_{n}^{(i)}}
where r m ( i ) {\displaystyle r_{m}^{(i)}} is the m t h {\displaystyle \mathrm {m^{th}} } Cartesian coordinate of the position vector r ( i ) {\displaystyle \mathbf {r} ^{(i)}} of the
i t h {\displaystyle \mathrm {i^{th}} } particle. The origin of the coordinate system has been chosen such that
∑ i = 1 N r ( i ) = 0 {\displaystyle \sum _{i=1}^{N}\mathbf {r} ^{(i)}=0}
i.e. in the system of the center of mass r C M {\displaystyle r_{CM}} . Where
r C M = 1 N ∑ i = 1 N r ( i ) {\displaystyle r_{CM}={\frac {1}{N}}\sum _{i=1}^{N}\mathbf {r} ^{(i)}}
Another definition, which is mathematically identical but gives an alternative calculation method, is:
S m n = d e f 1 2 N 2 ∑ i = 1 N ∑ j = 1 N ( r m ( i ) − r m ( j ) ) ( r n ( i ) − r n ( j ) ) {\displaystyle S_{mn}\ {\stackrel {\mathrm {def} }{=}}\ {\frac {1}{2N^{2}}}\sum _{i=1}^{N}\sum _{j=1}^{N}(r_{m}^{(i)}-r_{m}^{(j)})(r_{n}^{(i)}-r_{n}^{(j)})}
Therefore, the x-y component of the gyration tensor for particles in Cartesian coordinates would be:
S x y = 1 2 N 2 ∑ i = 1 N ∑ j = 1 N ( x i − x j ) ( y i − y j ) {\displaystyle S_{xy}={\frac {1}{2N^{2}}}\sum _{i=1}^{N}\sum _{j=1}^{N}(x_{i}-x_{j})(y_{i}-y_{j})}
In the continuum limit,
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