Abstract
This paper explores structure scalars of cylindrically symmetric spacetime in Brans-Dicke gravity. We construct twelve scalar factors using orthogonal splitting of the Reimann tensor and study their distinct dynamical interpretations. These structure scalars are used to derive a set of governing equations of the evolving system. It is concluded that cylindrical systems are necessarily inhomogeneous. Finally, we show that all possible static inhomogeneous cylindrical solutions can be obtained through structure scalars.
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Appendix
Appendix
The non-zero components of BD equations are
and the wave equation is
The non-zero components of the Weyl tensor in Eqs. (8) and (9) are
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Sharif, M., Manzoor, R. Structure scalars and cylindrical systems in Brans-Dicke gravity. Astrophys Space Sci 359, 17 (2015). https://doi.org/10.1007/s10509-015-2440-2
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DOI: https://doi.org/10.1007/s10509-015-2440-2