108 citations · 242 across the 8 of their papers we have counts for
8 papers
Could the low braking index pulsar PSR J1734-3333 evolve into a magnetar?
Z. -F. Gao, D. -L. Song, Y. -L. Liu +3
The low braking-index pulsar PSR J17343333 could be born with superhigh internal magnetic fields G, and undergo a supercritical accretion soon af…
The Effects of Superhigh Magnetic Fields on Equations of States of Neutron Stars
Z. F. Gao, N. Wang, Y. Xu +2
By introducing Dirac ?-function in superhigh magnetic field, we deduce a general formula for pressure of degenerate and relativistic electrons, Pe, which is suitable for superhigh…
Constraining the Braking Indices of Magnetars
Z. F. Gao, X. D. Li, N. Wang +3
Due to the lack of long term pulsed emission in quiescence and the strong timing noise, it is impossible to directly measure the braking index of a magnetar. Based on the estim…
Evolution of superhigh magnetic fields of magnetars
Z. F. Gao, N. Wang, J. P. Yuan +3
In this paper, we consider the effect of Landau levels on the decay of superhigh magnetic fields of magnetars. Applying anisotropic neutron superfluid theory yield a seco…
Magnetic field decay of magnetars in supernova remnants
Z. F. Gao, Q. H. Peng, N. Wang +1
In this paper, we modify our previous research carefully, and derive a new expression of electron energy density in superhigh magnetic fields. Based on our improved model, we re-co…
The surface and inner temperatures of magnetars
Z. F. Gao, N. Wang, Q. H. Peng
Assuming that the timescale of the magnetic field decay is approximately equal to that of the stellar cooling via neutrino emission, we obtain a one-to-one relationship between the…
The effects of intense magnetic fields on Landau levels in a neutron star
Z. F. Gao, N. Wang, D. L. Song +2
In this paper, an approximate method of calculating the Fermi energy of electrons () in a high-intensity magnetic field, based on the analysis of the distribution of a ne…
A very large glitch in PSR B2334+61
J. P. Yuan, R. N. Manchester, N. Wang +3
Seven years of pulse time-of-arrival measurements have been collected from observations of the young pulsar PSR B2334+61 using the Nanshan radio telescope of Urumqi Observatory. A…