868 citations · 2.7k across the 67 of their papers we have counts for
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Neutron star properties in the Thomas-Fermi model
Klaus Strobel, Fridolin Weber, Manfred K. Weigel +1
The modern nucleon-nucleon interaction of Myers and Swiatecki, adjusted to the properties of finite nuclei, the parameters of the mass formula, and the behavior of the optical pote…
Signal for the Quark-Hadron Phase Transition in Rotating Hybrid Stars
Fridolin Weber, Norman K. Glendenning, Shouyong Pei
For the past 20 years it had been thought that the coexistence phase of the confined hadronic and quark matter phases, assumed to be a first order transition, was strictly excluded…
Differences in the Cooling Behavior of Strange Quark Matter Stars and Neutron Stars
Christoph Schaab, Bernd Hermann, Fridolin Weber +1
The general statement that hypothetical strange (quark matter) stars cool more rapidly than neutron stars is investigated in greater detail. It is found that the direct Urca proces…