Constraints on Nonluminous Matter From Higher Order Pulsar Period Derivatives

Details Constraints on Nonluminous Matter From Higher Order Pulsar Period Derivatives Constraints on Nonluminous Matter From Higher Order Pulsar Period Derivatives

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009apj...694l..95e&link_type=abstract

The Astrophysical Journal Letters, Volume 694, Issue 2, pp. L95-L97 (2009).

Astronomy and Astrophysics

Astronomy

1

Pulsars: General

Scientific paper

Pulsar timing can detect the discreteness of the mass distribution in the Galaxy. The jerk imposed on millisecond pulsars by their nearest neighbors, and on the Sun by its nearest neighbor, may be detectable presently or within a decade. The method can detect planets in the outer solar system out to distances of several thousand AU, with the sensitivity rapidly increasing with time.

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