335 citations · 2.5k across the 69 of their papers we have counts for
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Neutron star radii and crusts: uncertainties and unified equations of state
M. Fortin, C. Providencia, A. R. Raduta +4
The uncertainties in neutron star (NS) radii and crust properties due to our limited knowledge of the equation of state (EOS) are quantitatively analysed. We first demonstrate the…
Progenitor neutron stars of the lightest and heaviest millisecond pulsars
M. Fortin, M. Bejger, P. Haensel +1
The recent mass measurements of two binary millisecond pulsars, PSR J1614-2230 and PSR J0751+1807 with a mass M=1.97+/-0.04 Msun and M= 1.26 +/- 0.14 Msun, respectively, indicate a…
Neutron stars with hyperon cores: stellar radii and EOS near nuclear density
M. Fortin, J. L. Zdunik, P. Haensel +1
The existence of 2 Msun pulsars puts very strong constraints on the equation of state (EOS) of neutron stars (NSs) with hyperon cores, which can be satisfied only by special models…
Maximum mass of neutron stars and strange neutron-star cores
J. L. Zdunik, P. Haensel
Recent measurement of mass of PSR J1614-2230 rules out most of existing models of equation of state (EOS) of dense matter with high-density softening due to hyperonization, based o…
Formation of millisecond pulsars - NS initial mass and EOS constraints
M. Bejger, M. Fortin, P. Haensel +1
Recent measurement of a high millisecond pulsar mass (PSR J1614-2230, 1.97+-0.04 Msun) compared with the low mass of PSR J0751+1807 (1.26+-0.14 Msun) indicates a large span of mass…
Hyperons in neutron-star cores and two-solar-mass pulsar
I. Bednarek, P. Haensel, J. L. Zdunik +2
Recent measurement of mass of PSR J1614-2230 rules out most of existing models of equation of state (EOS) of dense matter with high-density softening due to hyperonization or a pha…