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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CITATION STYLE
APA
Hess, P. O., Rodríguez, I., & Greiner, W. (2015). Pseudo-complex general relativity and neutron stars. In Nuclear Physics: Present and Future (pp. 255–264). Springer International Publishing. https://doi.org/10.1007/978-3-319-10199-6_24
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