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Pseudo-complex General Relativity and Neutron Stars

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Nuclear Physics: Present and Future

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Abstract

The basic concepts of the pseudo-complex General Relativity (pc-GR) are presented. The pc-GR is finally applied to neutron stars. We discuss the TOV equations for the matter and the dark energy. It is shown that already with a simple coupling of the matter with the dark energy, neutron stars with six solar masses can be generated without difficulty.

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Acknowledgments

P.O.H. acknowledges financial support from DGAPA and CONACyT, and also from FIAS and GSI.

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Correspondence to Peter O. Hess .

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Hess, P.O., Rodríguez, I., Greiner, W. (2015). Pseudo-complex General Relativity and Neutron Stars. In: Greiner, W. (eds) Nuclear Physics: Present and Future. FIAS Interdisciplinary Science Series. Springer, Cham. https://doi.org/10.1007/978-3-319-10199-6_24

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