326 citations · 1.5k across the 22 of their papers we have counts for
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astro-ph2007★ 3 cited
Neutron star crust beyond the Wigner-Seitz approximation
N. Chamel
For more than three decades, the inner crust of neutron stars, formed of a solid lattice of nuclear clusters coexisting with a gas of electrons and neutrons, has been traditionally…
astro-ph2006★ 16 cited
A microscopic equation of state for protoneutron stars
G. F. Burgio, M. Baldo, O. E. Nicotra +1
We study the structure of protoneutron stars within the finite temperature Brueckner-Bethe-Goldstone many-body theory. If nucleons, hyperons, and leptons are present in the stellar…
astro-ph2001★ 100 cited
Maximum mass of neutron stars with a quark core
G. F. Burgio, M. Baldo, P. K. Sahu +2
Massive neutron stars (NS) are expected to possess a quark core. While the hadronic side of the NS equation of state (EOS) can be considered well established, the quark side is qui…