Abstract
A Riemannian space of embedding class two is characterised by two symmetric tensors a ij , b ij and a vector si, satisfying the equations of Gauss, Codazzi and Ricci. It is proved that the Gauss equations together with one set of Codazzi equations imply the other set of Codazzi equations and the Ricci equations, provided that the matrix of the tensor b ij (or a ij ) is nonsingular. (The class m generalisation of the result has also been suggested). The result so proved has further been utilized in finding explicitly the a ij 's and b ij 's in the case of the static spherically symmetric line element. It is further indicated that the a ij 's and b ij 's so obtained are responsible for the different types of embeddings of the spacetime considered.
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References
Thomas, T.Y. (1936). Riemannian Spaces of Class One and Their Characterization,Acta Math.,67, 169–211.
Eisenhart, L.P. (1925).Riemannian Geometry, (Princeton University Press), p. 197.
Fujitani, T., Ekeda, M. and Matsumoto, M. (1961–62). On the Embedding of the Schwarzschild Space-Time. I.,J. Math. Kyoto Univ.,1, 43–61.
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Gupta, Y.K., Goel, P. Class two analogue of T. Y. Thomas's theorem and different types of embeddings of static spherically symmetric space-times. Gen Relat Gravit 6, 499–505 (1975). https://doi.org/10.1007/BF00762454
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DOI: https://doi.org/10.1007/BF00762454