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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…
Soft nuclear equation-of-state from heavy-ion data and implications for compact stars
Irina Sagert, Laura Tolos, Debarati Chatterjee +2
Measurements of kaon production at subthreshold energies in heavy-ion collisions point to a soft nuclear equation-of-state for densities up to 2-3 times nuclear matter saturation d…