Binary Pulsar Dynamics

Binary Pulsar Dynamics is a theoretical framework within the post-Newtonian approximation that models the orbital evolution and relativistic interactions of compact binary systems containing at least one pulsar, distinguishing itself by incorporating high-order gravitational radiation effects and spin-orbit couplings to predict observable timing anomalies.

597

Publications

43.7K

Citations

1.1K

Authors

528

Institutions

Publications per year

2017–2026

113

Authors

1.1K

  1. JH
    J. H. Taylor

    Princeton University, United States

    24 publications · 4.5K citations

    22

    h-index

  2. IH
    I. H. Stairs

    University of British Columbia, Canada

    20 publications · 3.7K citations

    19

    h-index

  3. AG
    A. G. Lyne

    University of Manchester, United Kingdom

    18 publications · 1.4K citations

    18

    h-index

  4. RN
    R. N. Manchester

    Commonwealth Scientific and Industrial Research Organisation, Australia

    18 publications · 1.4K citations

    18

    h-index

  5. VM
    V. M. Kaspi

    McGill University, Canada

    17 publications · 2.9K citations

    16

    h-index

1–5 of 1.1K

Venues

  1. The Astrophysical Journal

    ApJ · 150 publications · 9.9K citations

    58

    h-index

  2. Nature

    63 publications · 9.3K citations

    42

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    76 publications · 3.7K citations

    36

    h-index

  4. 22

    h-index

  5. Physical Review Letters

    PRL · 18 publications · 2.4K citations

    17

    h-index

1–5