Three-body Problem Stability

Three-Body Problem Stability is a theoretical construct in celestial mechanics that characterizes the qualitative persistence of bounded orbital configurations among three gravitationally interacting bodies, distinguishing it from general dynamical stability by addressing the inherent chaos and lack of general analytical solutions in three-body systems.

377

Publications

15.2K

Citations

484

Authors

265

Institutions

Publications per year

2017–2026

44

Authors

484

  1. JS
    Jagadish Singh

    Ahmadu Bello University, Nigeria

    29 publications · 887 citations

    20

    h-index

  2. BI
    B. Ishwar

    Babasaheb Bhimrao Ambedkar Bihar University, India

    9 publications · 288 citations

    9

    h-index

  3. EI
    Elbaz I. Abouelmagd

    National Research Institute of Astronomy and Geophysics, Egypt

    8 publications · 515 citations

    8

    h-index

  4. EA
    E. A. Perdios

    University of Patras, Greece

    8 publications · 216 citations

    8

    h-index

  5. JL
    Jaume Llibre

    Universitat Autònoma de Barcelona, Spain

    7 publications · 230 citations

    7

    h-index

1–5 of 484

Venues

  1. Celestial Mechanics and Dynamical Astronomy

    81 publications · 3.3K citations

    31

    h-index

  2. Astrophysics and Space Science

    44 publications · 1.4K citations

    23

    h-index

  3. 14

    h-index

  4. The Astronomical Journal

    AJ · 16 publications · 740 citations

    12

    h-index

  5. Journal of Differential Equations

    12 publications · 611 citations

    11

    h-index

1–5