Spacetimes with continuous linear isotropies III: null rotations
Autor: | MacCallum, M. A. H. |
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Rok vydání: | 2021 |
Předmět: | |
Druh dokumentu: | Working Paper |
DOI: | 10.1007/s10714-021-02869-1 |
Popis: | It is shown that in many cases local null rotation invariance of the curvature and its first derivatives is sufficient to ensure there is an isometry group G with dimension at least 3 acting on (a neighbourhood of) the spacetime and containing a null rotation isotropy. Invariance of the second derivatives is additionally required to ensure this conclusion in Petrov type N Einstein spacetimes, spacetimes containing "pure radiation" (a Ricci tensor of Segre type [(11,2)]), and conformally flat spacetimes with a Ricci tensor of Segre type [1(11,1)] (a "tachyon fluid"). Comment: Formatted for submission to General Relativity and Gravitation. Parts I and II accepted there and in press |
Databáze: | arXiv |
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