
Let M denote a Sasakian manifold and let \(\phi\) be the tensor field of type (1,1) with the property \(\phi^ 2=-I+\eta \otimes \xi\) where \(\eta\) denotes the contact form and \(\xi\) is the characteristic vector field with \(\eta (\xi)=1\). A geodesic \(\gamma\) on M is called a \(\phi\)-geodesic if \(\eta\) (\({\dot \gamma}\))\(=0\). M is locally \(\phi\)-symmetric (in the sense of Takahashi) if \(\phi^ 2(\nabla_ VR)(X,Y)Z=0\) for all vector fields V,X,Y,Z orthogonal to \(\xi\). A plane section of \(T_ pM\) is called a \(\phi\)-section if it is spanned by vectors X and \(\phi\) X orthogonal to \(\xi\). The sectional curvature of a \(\phi\)-section is called a \(\phi\)-sectional curvature. M is a Sasakian space form if M is of constant \(\phi\)-sectional curvature. In the paper the following main results are proved: M is locally \(\phi\)- symmetric iff the volume density function \(\theta_{\sigma}\) has antipodal symmetry along \(\phi\)-geodesics orthogonal to a \(\phi\)-geodesic \(\sigma\) for any \(\sigma\). M is a Sasakian space form iff the local symmetries with respect to all \(\phi\)-geodesics are volume-preserving provided that M is connected. M has constant curvature 1 iff M is harmonic with respect to each \(\phi\)-geodesic. In the case dim(M)\(\geq 5\) this condition is satisfied iff the local symmetries with respect to all \(\phi\)-geodesics are isometries. If M is a 3-dimensional Sasakian space form then any local symmetry with respect to any \(\phi\)-geodesic is an isometry.
Special Riemannian manifolds (Einstein, Sasakian, etc.), Sasakian space form, local symmetry, geodesic, Sasakian manifold
Special Riemannian manifolds (Einstein, Sasakian, etc.), Sasakian space form, local symmetry, geodesic, Sasakian manifold
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