A Non-radial Oscillation Mode in an Accreting Millisecond Pulsar?
arXiv:1310.5147 · doi:10.1088/0004-637X/784/1/72
Abstract
We present results of targeted searches for signatures of non-radial oscillation modes (such as r- and g-modes) in neutron stars using {\it RXTE} data from several accreting millisecond X-ray pulsars (AMXPs). We search for potentially coherent signals in the neutron star rest frame by first removing the phase delays associated with the star's binary motion and computing FFT power spectra of continuous light curves with up to time bins. We search a range of frequencies in which both r- and g-modes are theoretically expected to reside. Using data from the discovery outburst of the 435 Hz pulsar XTE J1751305 we find a single candidate, coherent oscillation with a frequency of Hz, and a fractional Fourier amplitude of . We estimate the significance of this feature at the level, slightly better than a detection. We argue that possible mode identifications include rotationally-modified g-modes associated with either a helium-rich surface layer or a density discontinuity due to electron captures on hydrogen in the accreted ocean. Alternatively, the frequency could be identified with that of an inertial mode or an r-mode modified by the presence of a solid crust, however, the r-mode amplitude required to account for the observed modulation amplitude would induce a large spin-down rate inconsistent with the observed pulse timing measurements. For the AMXPs XTE J1814338 and NGC 6440 X-2 we do not find any candidate oscillation signals, and we place upper limits on the fractional Fourier amplitude of any coherent oscillations in our frequency search range of and , respectively. We briefly discuss the prospects and sensitivity for similar searches with future, larger X-ray collecting area missions.
17 pages, 11 figures. Additional discussion of r- and inertial mode interpretations. Accepted for publication in the Astrophysical Journal
References in corpus (4)
- Detecting gravitational wave emission from the known accreting neutron stars
- Oscillations of rapidly rotating stratified neutron stars
- Timing of the Accreting Millisecond Pulsar XTE J1814-338
- Coherence of burst oscillations and accretion-powered pulsations in the accreting millisecond pulsar XTE J1814-338
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