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nucl-th2024
How neutron star properties disfavor a nuclear chiral density wave
Orestis Papadopoulos, Andreas Schmitt
Cold and dense matter may break rotational symmetry spontaneously and thus form an anisotropic phase in the interior of neutron stars. We consider the concrete example of an anisot…
hep-ph2024
Thermal pion condensation: holography meets lattice QCD
Nicolas Kovensky, Andreas Schmitt
The holographic Witten-Sakai-Sugimoto model is often employed to describe strongly-coupled baryonic and isospin-asymmetric matter, for example in the context of neutron stars. Here…