231 citations · 908 across the 28 of their papers we have counts for
7 papers · 1 filter
Can magnetic fields stabilize or destabilize twin stars?
R. O. Gomes, V. Dexheimer, S. Han +1
Sharp phase transitions described by stiff equations of state allow for the existence of a third family of stable compact stars (besides white dwarfs and neutron stars), twin stars…
What do we learn about vector interactions from GW170817?
Veronica Dexheimer, Rosana de Oliveira Gomes, Stefan Schramm +1
We analyze the role played by vector-isovector meson interaction in dense matter present in the interior of neutron stars in the light of new measurements made during the double ne…
QCD at high density: Equation of state for nuclear collisions and neutron stars
Anton Motornenko, Volodymyr Vovchenko, Jan Steinheimer +2
A unified chiral mean field approach is presented for QCD thermodynamics in a wide range of temperatures and densities. The model simultaneously gives a satisfactory description of…
Effects of a non-zero strangeness-chemical potential in strong interaction models
Ayon Mukherjee, Abhijit Bhattacharyya, Stefan Schramm
The effect of a non-zero strangeness chemical potential on the strong interaction phase diagram has been studied within the framework of the SU(3) quark-hadron chiral parity-double…
Signatures of quark-hadron phase transitions in general-relativistic neutron-star mergers
Elias R. Most, L. Jens Papenfort, Veronica Dexheimer +4
Merging binaries of neutron stars are not only strong sources of gravitational waves, but also have the potential of revealing states of matter at densities and temperatures not ac…
Constraining strangeness in dense matter with GW170817
R. O. Gomes, Prasanta Char, S. Schramm
Particles with strangeness content are predicted to populate dense matter, modifying the equation of state of matter inside neutron stars as well as their structure and evolution.…