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end{aligned} (2.11) Furthermore, the scalar curvature ρ for a submanifold M of an almost contact manifold M̃ is given by begin{aligned} rho=sum_{1leq ineq jleq n}K e_{i} wedge e_{j}), end{aligned} (2.12) where (K e_{i}wedge e_{j})) is the sectional curvature of plane section spanned by (e_{i}) and (e_{j}).
where K ( e i ∧ e j ) is the sectional curvature of the plane section spanned by e i and e j at x ∈ M. Let Π k be a k-plane section of T x M, and let { e 1, …, e k } be any orthonormal basis of Π k.
where K ( e i ∧ e j ) and K ¯ ( e i ∧ e j ) denote the sectional curvature of the plane section spanned by e i and e j at x in the submanifold M and in the ambient manifold M ¯, respectively.
Then the mean curvature vector H is given by H = ∑ r = n + 1 n + p ( 1 n ∑ i = 1 n h i i r ) e r, and the squared norm of h over dimension n is denoted by C and is called the Casorati curvature of the submanifold M. Therefore we have C = 1 n ∑ r = n + 1 n + p ∑ i, j = 1 n ( h i j r ) 2. Let K ( e i ∧ e j ), 1 ≤ i < j ≤ n, denote the sectional curvature of the plane section spanned by e i and e j.
Then we denote by g the metric tensor induced on M. Let (K pi)) be the sectional curvature of M associated with a plane section (pisubset T_{p}M), (pin M).
We denote by K the sectional curvature of M associated with a plane section π ⊂ T p M, p ∈ M. If { e 1, …, e n } is an orthonormal basis of the tangent space T p M, the scalar curvature τ at p is defined by τ ( p ) = ∑ 1 ≤ i < j ≤ n K ( e i ∧ e j ).
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