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Thermal Evolution of Rotating Neutron Stars
Rodrigo Negreiros, Stefan Schramm, Fridolin Weber
In this work we consider the thermal evolution of rigidly rotating neutron stars. In order to perform such study we first calculate the structure of rotating objects, which is cons…
Impact of Rotation on the Structure and Composition of Neutron Stars
Fridolin Weber, Milva Orsaria, Rodrigo Negreiros
Depending on mass and rotational frequency, gravity compresses the matter in the core regions of neutron stars to densities that are several times higher than the density of ordina…
Proton superconductivity and the masses of neutron stars
Rodrigo Negreiros, Stefan Schramm, Fridolin Weber
The unexpected temperature evolution of the neutron star in the Cassiopeia A supernova remnant (Cas A, for short) has renewed tremendous interest in the cooling mechanisms of neutr…