A&A 441, 207-211 (2005)
Spin-up of the hyperon-softened accreting neutron starsJ. L. Zdunik, P. Haensel and M. Bejger
N. Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18, 00-716 Warszawa, Poland
(Received 7 February 2005 / Accepted 25 April 2005)
We study the spin-up of the accreting neutron stars with a realistic hyperon-softened equation of state. Using precise 2D calculations we study the evolutionary tracks of accreting neutron stars in the angular-momentum - frequency planes. In contrast to the case of spinning-down solitary radio-pulsars, where a strong back-bending behavior has been observed, we do not see back-bending phenomena in the accretion-powered spinning-up case. We conclude that in the case of accretion-driven spin-up the back-bending is strongly suppressed by the mass-increase effect accompanying the angular-momentum increase.
Key words: dense matter -- equation of state -- stars: neutron -- stars: binaries: general
© ESO 2005