Abstract
In this chapter, neutron stars within the extended theory are considered. A simple linear model is applied, describing the coupling between the dark energy to the matter density. Neutron stars with up to 6 solar masses will be obtained. Energy conditions and their derivation are explicitly presented, for isotropic and anisotropic fluids.
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Hess, P.O., Schäfer, M., Greiner, W. (2016). Neutron Stars Within the Pseudo-complex General Relativity. In: Pseudo-Complex General Relativity. FIAS Interdisciplinary Science Series. Springer, Cham. https://doi.org/10.1007/978-3-319-25061-8_6
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DOI: https://doi.org/10.1007/978-3-319-25061-8_6
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