131 citations · 233 across the 11 of their papers we have counts for
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Representing Equations of State With Strong First-Order Phase Transitions
Lee Lindblom, Steve M. Lewis, Fridolin Weber
Parametric representations of the high-density nuclear equation of state are used in constructing models for interpreting the astrophysical observations of neutron stars. This stud…
Hybrid Stars in the Framework of different NJL Models
G. A. Contrera, M. Orsaria, I. F. Ranea-Sandoval +1
We compute models for the equation of state (EoS) of the matter in the cores of hybrid stars. Hadronic matter is treated in the non-linear relativistic mean-field approximation, an…
Quark deconfinement in high-mass neutron stars
M. Orsaria, H. Rodrigues, F. Weber +1
In this paper, we explore whether or not quark deconfinement may occur in high-mass neutron stars such as J1614-2230 (1.97 \pm 0.04 M_Sun) and J0348+0432 (2.01 \pm 0.04 M_Sun). Our…