Abstract
In the paper (Khugaev et al. in Phys Rev D94:064065. arXiv: 1603.07118, 2016), we have shown that for perfect fluid spheres the pressure isotropy equation for Buchdahl–Vaidya–Tikekar metric ansatz continues to have the same Gauss form in higher dimensions, and hence higher dimensional solutions could be obtained by redefining the space geometry characterizing Vaidya–Tikekar parameter K. In this paper we extend this analysis to pure Lovelock gravity; i.e. a \((2N+2)\)-dimensional solution with a given \(K_{2N+2}\) can be taken over to higher n-dimensional pure Lovelock solution with \(K_n=(K_{2N+2}-n+2N+2)/(n-2N-1)\) where N is degree of Lovelock action. This ansatz includes the uniform density Schwarzshild and the Finch–Skea models, and it is interesting that the two define the two ends of compactness, the former being the densest and while the latter rarest. All other models with this ansatz lie in between these two limiting distributions.
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Notes
Gravitational potential for Einstein goes as \(1/r^{n-3}\) while for pure Lovelock as \(1/r^{(n-2N-1)/N}\).
This is because the two define the extremity limits and hence they both have to be exclusive.
It has recently been generalized [23] for pure Lovelock gravity.
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Acknowledgements
AK and AM gratefully acknowledge IUCAA for the invitation and warm hospitality which facilitated this collaboration. Partial support for this work to AK was provided by Uzbekistan Foundation for Fundamental Research project F2-FA-F-116. Partial support for this work to AM was provided by FIS2015-65140-P (MINECO/FEDER). ND thanks Albert Einstein Institute, Golm and the University of Barcelona for visits that facilitated finalization of the manuscript.
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Molina, A., Dadhich, N. & Khugaev, A. Buchdahl–Vaidya–Tikekar model for stellar interior in pure Lovelock gravity. Gen Relativ Gravit 49, 96 (2017). https://doi.org/10.1007/s10714-017-2259-y
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DOI: https://doi.org/10.1007/s10714-017-2259-y