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Driven by the loss of energy, isolated rotating neutron stars (pulsars) are gradually slowing down to lower frequencies, which increases the tremendous compression of the matter inside of them. This increase in compression changes both the global properties of rotating neutron stars as well as their hadronic core compositions. Both effects may register themselves observationally in the thermal evolution...
The baryonic properties of neutron stars within the theory of pseudo‐complex General Relativity (pc‐GR) are studied. The pc‐Tolman‐Oppenheimer‐Volkoff equations are numerically integrated in order to understand the structure of these objects. The pc‐component energy density ϵΛ has been linearly coupled to the respective baryonic quantity ϵm. Solutions have been presented for different values of the...
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