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Observational Constraints on Quark Matter in neutron stars

Chinese Journal of Astronomy and Astrophysics 2007年第5期7卷 675-684页

作者： Na-Na Pan Xiao-Ping Zheng Institute of Astrophysics Huazhong Normal University Wuhan 430079

We study the observational constraints of mass and redshift on the properties of the equation of state （EOS） for quark matter in compact stars based on the quasi-particle description. We discuss two scenarios; strange stars and hybrid stars. We construct the equations of state utilizing an extended MIT bag model taking the medium effect into account for quark matter and the relativistic mean field theory for hadron matter. We show that quark matter may exist in strange stars and in the interior of neutron stars. The bag constant is a key parameter that affects strongly the mass of strange stars. The medium effect can lead to the stiffer hybrid-star EOS approaching the pure hadronic EOS, due to the reduction of quark matter, and hence the existence of heavy hybrid stars. We find that a middle range coupling constant may be the best choice for the hybrid stars being compatible with the observational constraints.

关键词： dense matter -- gravitation -- stars neutron -- stars rotation -- stars oscillations

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Toward an Understanding of the Periastron Puzzle of PSR B1259-63

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Chinese Journal of Astronomy and Astrophysics 2006年第5期6卷 572-578页

作者： Ren-Xin Xu Department of Astronomy School of Physics Peking University Beijing 100871

Efforts are made to understand the timing behaviors （e.g., the jumps in the projected pulsar semimajor axis at the periastron passages） observed in the 13-year monitoring of PSR B1259-63. Planet-like objects are suggested to orbit around the Be star, which may gravitationally perturb the （probably low mass） pulsar when it passes through periastron. An accretion disk should exist outside the pulsar＇s light cylinder, which creates a spindown torque on the pulsar due to the propeller effect. The observed negative braking index and the discrepant timing residuals close to periastron could be related to the existence of a disk with a varying accretion rate. A speculation is presented that the accretion rate may increase on a long timescale in order to explain the negative braking index.

关键词： pulsars individual PSR B1259-63 -- binaries general -- stars neutron -- stars early-type

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Temporal variations and spectral properties of the Be/X-ray pulsar GRO J1008–57 studied by INTEGRAL

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Research in Astronomy and Astrophysics 2014年第5期14卷 565-580页

作者： Wei Wang National Astronomical Observatories Chinese Academy of Sciences

The spin period variations and hard X-ray spectral properties of the Be/Xray pulsar GRO J1008-57 are studied with INTEGRAL observations during two out- bursts in 2004 June and 2009 March. The pulsation periods of -93.66 s in 2004 and - 93.73 s in 2009 are determined. Pulse profiles of GRO J1008-57 during out- bursts are strongly energy dependent with a double-peaked profile from 3-7 keV and a single-peaked profile in hard X-rays above 7 keV. Combined with previous measure- ments, we find that GRO J1008-57 has undergone a spin-down trend from 1993 - 2009 with a rate of - 4.1 × 10^-5 s d^-1, and could have changed into a spin-up trend after 2009. We find a relatively soft spectrum in the early phase of the 2009 outburst with cutoff energy ~ 13keV. Above a hard X-ray flux of - 10^-9 erg cm^-2 s^-1, the spectra of GRO J1008-57 during outbursts need an enhanced hydrogen absorption with column density ~ 6 x 1022 cm-2. The observed dip-like pulse profile of GRO J1008-57 in soft X-ray bands could be caused by this intrinsic absorption. Around the outburst peaks, a possible cyclotron resonance scattering feature at - 74 keV is detected in the spectra of GRO J1008-57 which is consistent with the feature that was reported in MAXI/GSC observations, making the source a neutron star with the highest known magnetic field （- 6.6 × 10^12 G） among accreting X-ray pulsars. This marginal feature is supported by the present detections in GRO J1008-57 following the correlation between the fundamental line energies and cutoff energies in accret- ing X-ray pulsars. Finally we discovered two modulation periods at - 124.38 d and 248.78d using RXTE/ASM light curves of GRO J1008-57. Two flare peaks ap- pearing in the folded light curve had different spectral properties. The normal outburst lasting 0,1 of an orbital phase had a hard spectrum and could not be significantly de- tected below 3 keV. The second flare lasting ten days showed a very soft spectrum without significant detections above

关键词： stars individual (GRO J1008-57) -- stars neutron -- stars magneticfields -- binaries close -- X-rays binaries

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