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High-Frequency Variability in Neutron-Star Low-Mass X-ray Binaries

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Timing Neutron Stars: Pulsations, Oscillations and Explosions

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 461))

Abstract

Binary systems with a neutron-star primary accreting from a companion star display variability in the X-ray band on time scales ranging from years to milliseconds. With frequencies of up to ∼1300 Hz, the kilohertz quasi-periodic oscillations (kHz QPOs) represent the fastest variability observed from any astronomical object. The sub-millisecond time scale of this variability implies that the kHz QPOs are produced in the accretion flow very close to the surface of the neutron star, providing a unique view of the dynamics of matter under the influence of some of the strongest gravitational fields in the Universe. This offers the possibility to probe some of the most extreme predictions of General Relativity, such as dragging of inertial frames and periastron precession at rates that are 16 orders of magnitude faster than those observed in the solar system and, ultimately, the existence of a minimum distance at which a stable orbit around a compact object is possible. Here we review the last 20 years of research on kHz QPOs, and we discuss the prospects for future developments in this field.

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Notes

  1. 1.

    Phase lags equal to Δϕ ± 2, with n any integer number, cannot be distinguished from a phase lag Δϕ.

  2. 2.

    As explained in Sect. 6.4, in a modified version of the sonic-point model the frequency difference between the kHz QPOs can also be equal to half the neutron-star spin frequency [87].

  3. 3.

    This is possibly also the case for the upper kHz QPO, and all other QPO signals in these sources.

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Acknowledgements

This work is part of the research programme Athena with project number 184.034.002, which is (partly) financed by the Dutch Research Council (NWO). TMB acknowledges financial contribution from the agreement ASI-INAF n.2017-14-H.0. This research has made use of data and/or software provided by the High Energy Astrophysics Science Archive Research Center (HEASARC), which is a service of the Astrophysics Science Division at NASA/GSFC. This research made use of NASA’s Astrophysics Data System.

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Méndez, M., Belloni, T.M. (2021). High-Frequency Variability in Neutron-Star Low-Mass X-ray Binaries. In: Belloni, T.M., Méndez, M., Zhang, C. (eds) Timing Neutron Stars: Pulsations, Oscillations and Explosions. Astrophysics and Space Science Library, vol 461. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-662-62110-3_6

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