3 papers
astro-ph.HE2019
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars
Mateusz Cierniak, Tobias Fischer, Niels-Uwe Bastian +2
We construct a set of equations of state (EoS) of dense and hot matter with a 1st order phase transition from a hadronic system to a deconfined quark matter state. In this two-phas…
nucl-th2018
Lifting the Veil on Quark Matter in Compact Stars with Core g-mode Oscillations
Wei Wei, Megan Barry, Thomas Klähn +1
Compact stars containing quark matter may masquerade as neutron stars in the range of measured mass and radius, making it difficult to draw firm conclusions on the phase of matter…
nucl-th2018
Camouflage of the Phase Transition to Quark Matter in Neutron Stars
Wei Wei, Bryen Irving, Thomas Klähn +1
It has been known for some time that compact stars containing quark matter can masquerade as neutron stars in the range of measured mass and radius, making it difficult to draw fir…