activity
19952026
most citedNeutron star radii and crusts: uncertainties and unified equations of state

335 citations · 2.5k across the 69 of their papers we have counts for

collaborators

71 papers

astro-ph.HE2026

Modelling mountains on accreting magnetized neutron stars

T. Brusco, B. Haskell, M. Razzano +2

Continuous gravitational waves from accreting neutron stars in Low Mass X-ray Binaries are one of the main targets for current and next generation ground based detectors. In order…

astro-ph.HE2025

Dynamical tides in neutron stars with first-order phase transitions: the role of the discontinuity mode

Jonas P. Pereira, Lucas Tonetto, Michał Bejger +2

During the late stages of a binary neutron star inspiral, dynamical tides induced in each star by its companion become significant and should be included in complete gravitational-…

astro-ph.HE2024★ 1 cited

Layers of electron captures in the crust of accreting neutron stars

Lami Suleiman, Julian-Leszek Zdunik, Pawel Haensel

The accumulation of accreted matter onto the neutron star surface triggers exothermic reactions in the crust. The heat released as a result influences the luminosity exhibited by t…

astro-ph.HE2022

Internal Heating in Magnetars: Role of Electron Captures

Nicolas Chamel, Anthea Francesca Fantina, Lami Suleiman +2

The role of electron captures by nuclei in the shallow heating of magnetars is further investigated using both nuclear measurements and the theoretical atomic mass table HFB-27. St…

astro-ph.HE2022★ 7 cited

Crustal failure as a tool to probe hybrid stars

Jonas P. Pereira, Michał Bejger, Paweł Haensel +1

It is currently unknown if neutron stars (NSs) are composed of nucleons only or are hybrid stars, i.e., in addition to nucleonic crusts and outer cores, they also possess quark cor…

astro-ph.HE2022

Evidence for 3XMM J185246.6+003317 as a massive magnetar with a low magnetic field

Rafael C. R. de Lima, Jonas P. Pereira, Jaziel G. Coelho +10

3XMM J185246.6+003317 is a transient magnetar located in the vicinity of the supernova remnant Kes\,79. So far, observations have only set upper limits to its surface magnetic fiel…