695 citations · 6.4k across the 119 of their papers we have counts for
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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…
Constraint on the internal structure of a neutron star from Vela pulsar glitches
N. Chamel
Pulsars are spinning extremely rapidly with periods as short as about milliseconds and delays of a few milliseconds per year at most, thus providing the most accurate clocks…
Landau quantization and neutron emissions by nuclei in the crust of a magnetar
N. Chamel, Y. D. Mutafchieva, Zh. K. Stoyanov +2
Magnetars are neutron stars endowed with surface magnetic fields of the order of ~G, and with presumably much stronger fields in their interior. As a result of Lan…
Global numerical simulations of the rise of vortex-mediated pulsar glitches in full general relativity
Aurélien Sourie, Nicolas Chamel, Jérôme Novak +1
In this paper, we study in detail the role of general relativity on the global dynamics of giant pulsar glitches as exemplified by Vela. For this purpose, we carry out numerical si…
Giant Pulsar Glitches and the Inertia of Neutron-Star Crusts
T. Delsate, N. Chamel, N. Gürlebeck +3
Giant pulsar frequency glitches as detected in the emblematic Vela pulsar have long been thought to be the manifestation of a neutron superfluid permeating the inner crust of a neu…