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Electron Captures and Stability of White Dwarfs
N. Chamel, L. Perot, A. F. Fantina +4
Electron captures by atomic nuclei in dense matter are among the most important processes governing the late evolution of stars, limiting in particular the stability of white dwarf…
On the maximum mass of magnetised white dwarfs
D. Chatterjee, A. F. Fantina, N. Chamel +2
We develop a detailed and self-consistent numerical model for extremely-magnetised white dwarfs, which have been proposed as progenitors of overluminous Type Ia supernovae. This mo…
Probing the neutron star interior and the Equation of State of cold dense matter with the SKA
Anna Watts, Renxin Xu, Cristobal Espinoza +15
With an average density higher than the nuclear density, neutron stars (NS) provide a unique test-ground for nuclear physics, quantum chromodynamics (QCD), and nuclear superfluidit…
CompOSE - CompStar Online Supernovae Equations of State
S. Typel, M. Oertel, T. Klaehn
This paper is the manual of the CompOSE service, see http://compose.obspm.fr, an equation of state (EoS) database for use in nuclear physics and in astrophysical applications, e.g.…