activity
20162022
most citedStrong correlations of neutron star radii with the slopes of nuclear matter incompressibility and symmetry energy at saturation

94 citations · 517 across the 16 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

14 papers · 1 filter

astro-ph.HE2022★ 10 cited

Partially accreted crusts of neutron stars

Lami Suleiman, Julian-Leszek Zdunik, Pawel Haensel +1

Neutron stars in low-mass binary systems are subject to accretion. The common assumption in studying the properties of the neutron star crust is the fully accreted crust approximat…

astro-ph.HE2021★ 43 cited

Influence of the crust on the neutron star macrophysical quantities and universal relations

Lami Suleiman, Morgane Fortin, Julian Leszek Zdunik +1

Measurements of neutron-star macrophysical properties thanks to multimessenger observations offer the possibility to constrain the properties of nuclear matter. Indeed cold and den…

astro-ph.HE2020

Magnetic fields in late-stage proto-neutron stars

S. K. Lander, P. Haensel, B. Haskell +2

We explore the thermal and magnetic-field structure of a late-stage proto-neutron star. We find the dominant contribution to the entropy in different regions of the star, from whic…

astro-ph.HE2019★ 31 cited

Bulk viscosity in neutron stars with hyperon cores

D. D. Ofengeim, M. E. Gusakov, P. Haensel +1

It is well-known that r-mode oscillations of rotating neutron stars may be unstable with respect to the gravitational wave emission. It is highly unlikely to observe a neutron star…

astro-ph.HE2018

Hyperonic stars and the symmetry energy

Constança Providência, Morgan Fortin, Helena Pais +1

In the present study we analyse the effect of the density dependence of the symmetry energy on the hyperonic content of neutron stars within a relativistic mean field description o…

astro-ph.HE2018

Fundamental physics and the absence of sub-millisecond pulsars

B. Haskell, J. L. Zdunik, M. Fortin +3

Observations of the spin distribution of rapidly rotating neutron stars show evidence for a lack of stars spinning at frequencies larger than Hz, well below the pred…