Classical N-body Problem

The Classical N-Body Problem is a mathematical framework in classical mechanics that models the deterministic motion of a finite number of celestial bodies interacting pairwise through Newtonian gravitational forces, distinguished from other dynamical systems by its reliance solely on inverse-square law interactions and exact solutions to the equations of motion for predicting long-term trajectories.

198

Publications

21.4K

Citations

300

Authors

192

Institutions

Publications per year

2017–2026

8

Authors

300

  1. DG
    Donald G. Saari

    Northwestern University, United States

    4 publications · 136 citations

    4

    h-index

  2. AC
    Alain Chenciner

    Institut de Mécanique Céleste et de Calcul des Éphémérides, France

    3 publications · 58 citations

    3

    h-index

  3. ST
    Susanna Terracini

    University of Milano-Bicocca, Italy

    3 publications · 93 citations

    3

    h-index

  4. FM
    Flavio Mercati

    Sapienza University of Rome, Italy

    3 publications · 200 citations

    3

    h-index

  5. HP
    Harry Pollard

    Purdue University West Lafayette, United States

    3 publications · 186 citations

    3

    h-index

1–5 of 300

Venues

  1. Physics Letters B

    12 publications · 1.6K citations

    13

    h-index

  2. Nuclear Physics B

    12 publications · 2.3K citations

    12

    h-index

  3. Celestial Mechanics and Dynamical Astronomy

    9 publications · 421 citations

    9

    h-index

  4. Journal of Mathematical Physics

    6 publications · 201 citations

    6

    h-index

  5. Archive for Rational Mechanics and Analysis

    5 publications · 163 citations

    5

    h-index

1–5