The signature of the metric tensor g at the point P of the D-dimensional smooth (connected Hausdorff C ∞) manifold is the number of positive eigenvalues of the matrix (g ab ) at P, minus the number of negative ones[1]. A metric whose signature is (D − 2) is called a metric of Lorentzian signature or simply a Lorentz metric . The canonical form is
If the metric on has a Lorentzian signature then each nonzero vector X with coordinates X a at point P can be divided into three classes according to whether the scalar product g mn X m X n is negative, zero, or positive. Correspondingly the vector X is said to be timelike, null, or spacelike at P[2].
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Bibliography
S. W. Hawking and G. F. R. Ellis, The large scale structure of spacetime, Cambridge University Press 1973
W. Rindler Introduction to special relativity, Oxford, Clarendon Press 1982.
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Duplij, S. et al. (2004). Lorentzian Signature. In: Duplij, S., Siegel, W., Bagger, J. (eds) Concise Encyclopedia of Supersymmetry. Springer, Dordrecht. https://doi.org/10.1007/1-4020-4522-0_308
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DOI: https://doi.org/10.1007/1-4020-4522-0_308
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