265 citations · 3.3k across the 91 of their papers we have counts for
94 papers
Measuring radii of merging neutron stars with interface-mode asteroseismology informed by nuclear theory and experiment
Duncan Neill, William G. Newton, Jeremy W. Holt +3
The structure and dynamics of neutron stars can be used to probe the physics of extreme matter at nuclear densities and beyond. Nucleonic matter up to ~2-3 times nuclear saturation…
Impact of soft versus hard equations of state on hybrid stars
H. Güven, K. Bozkurt, E. Khan +1
The nuclear stiffness as a dominant contribution of nuclear symmetry energy is analyzed on the properties of compact stars considering constraints from nuclear physics and astrophy…
Dense Matter in Neutron Stars with eXTP
Ang Li, Anna L. Watts, Guobao Zhang +82
In this White Paper, we present the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission to constrain the equation of state of dense matter in neutron stars, explo…
Relativistic mean-field predictions for dense matter equation of state and application to neutron stars
Luca Passarella, Jerome Margueron, Giuseppe Pagliara
Relativistic mean-field models (RMF) based on the exchange of , , and mesons including non-linear nucleon- couplings and density-dependent coupling, are considered…
Effects of dilute neutron matter on the neutron star crust equation of state
Guilherme Grams, Jerome Margueron
We develop a compressible liquid-drop model to describe the crust of neutron stars for which the role of the nuclear clusters, the neutron gas, and the electrons are clearly identi…
What can we learn about the unstable equation-of-state branch from neutron-star mergers?
Maximiliano Ujevic, Rahul Somasundaram, Tim Dietrich +2
The Equation of State (EOS) of dense strongly-interacting matter can be probed by astrophysical observations of neutron stars (NS), such as X-ray detections of pulsars or the measu…