activity
19932005
most citedConstraints on the dense matter EOS from the measurements of PSR J0737-3039A moment of inertia and PSR J0751+1807 mass

78 citations · 199 across the 6 of their papers we have counts for

collaborators

12 papers

astro-ph200578 cited

Constraints on the dense matter EOS from the measurements of PSR J0737-3039A moment of inertia and PSR J0751+1807 mass

M. Bejger, T. Bulik, P. Haensel

The moment of inertia of the pulsar A in the neutron star binary J0737-3039 will soon be measurable through detailed measurements of the periastron advance. We present the calculat…

astro-ph200556 cited

Phase transitions in rotating neutron stars cores: back bending, stability, corequakes and pulsar timing

J. L. Zdunik, M. Bejger, P. Haensel +1

The back-bending phenomenon for compact stars is studied by means of analytical equations of state, for both constant-pressure phase transitions and the transitions through the mix…

astro-ph200529 cited

Non-equilibrium beta processes in superfluid neutron star cores

L. Villain, P. Haensel

The influence of nucleons superfluidity on the beta relaxation time of degenerate neutron star cores, composed of neutrons, protons and electrons, is investigated. We numerically c…

astro-ph20058 cited

Spin-up of the hyperon-softened accreting neutron stars

J. L. Zdunik, P. Haensel, M. Bejger

We study the spin-up of the accreting neutron stars with a realistic hyperon-softened equation of state. Using precise 2-D calculations we study the evolutionary tracks of accretin…

astro-ph200414 cited

Surface gravity of neutron stars and strange stars

M. Bejger, P. Haensel

The upper bound on the value of the surface gravity, g_s, for neutron stars with equations of state respecting v_sound <= c, is derived. This bound is inversely proportional to the…

astro-ph2000

Protoneutron stars and neutron stars

D. Gondek-Rosinska, P. Haensel, J. L. Zdunik

We find constraints on minimum and maximum mass of ordinary neutron stars imposed by their early evolution (protoneutron star stage). We calculate models of protoneutron stars usin…