Corpus ID: 220665540

Pulsar Timing Signatures of Circumbinary Asteroid Belts

@inproceedings{Jennings2020PulsarTS,
  title={Pulsar Timing Signatures of Circumbinary Asteroid Belts},
  author={R. Jennings and J. Cordes and S. Chatterjee},
  year={2020}
}
  • R. Jennings, J. Cordes, S. Chatterjee
  • Published 2020
  • Physics
  • The gravitational pull of a large number of asteroids perturbs a pulsar’s motion to a degree that is detectable through precision timing of millisecond pulsars. The result is a low-frequency, correlated noise process, similar in form to the red timing noise known to affect canonical pulsars, or to the signal expected from a stochastic gravitational-wave background. Motivated by the observed fact that many millisecond pulsars are in binary systems, we describe the ways in which the presence of a… CONTINUE READING

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    References

    Publications referenced by this paper.
    SHOWING 1-3 OF 3 REFERENCES
    Solar System Dynamics
    2031
    VizieR Online Data Catalog
    1642
    Solar system dynamics Nagler
    • 1999