Abstract
The group of rigid motions is considered to guide the search for a natural system of space-time coordinates in General Relativity. This search leads us to a natural extension of the space-times that support Painlevé–Gullstrand synchronization. As an interesting example, here we describe a system of rigid coordinates for the cross mode of gravitational linear plane waves.
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Notes
Throughout the paper we will use the following notation: Latin indices \(i,j,k=1,2,3\); \(dx\,dy=\frac{1}{2}(dx\otimes dy+dy\otimes dx)\); \(T_{(i}Q_{j)}=\frac{1}{2}(T_{i}Q_{j}+T_{j}Q_{i})\); \(\delta _{ij}\) is the three-dimensional identity; \(f_{,i}=\frac{\partial f}{\partial x^{i}}\), where \(x^{i}\) are the space coordinates; \(f_{,\lambda }=\frac{\partial f}{\partial \lambda }\); \(\bar{d}\) is the restriction of the differential to \(d\lambda =0\), i.e. \(\bar{d} f(x,\lambda )= \frac{\partial f}{\partial x^{i}} dx^i\).
In this section we will use a prime, \(f'\), to indicate the derivation of a function with respect to its argument.
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Acknowledgements
We thank the reviewer for his/her interesting comments that has lead us to improve the paper. Support for this work to AM was provided by FIS2015-65140-P (MINECO/FEDER).
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Jaén, X., Molina, A. Rigid covariance as a natural extension of Painlevé–Gullstrand space-times: gravitational waves. Gen Relativ Gravit 49, 108 (2017). https://doi.org/10.1007/s10714-017-2272-1
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DOI: https://doi.org/10.1007/s10714-017-2272-1