Periastron Precession

Periastron Precession is a relativistic orbital phenomenon in post-Newtonian gravity that describes the gradual advance of the point of closest approach in a binary system’s orbit due to the curvature of spacetime caused by the masses’ gravitational interaction.

154

Publications

7.6K

Citations

330

Authors

267

Institutions

Publications per year

2017–2026

52

Variants

Periastron Advance

Authors

330

  1. AB
    Abdelmalek Bouzenada

    Université Larbi Tébessi, Algeria

    5 publications · 107 citations

    5

    h-index

  2. LI
    Lorenzo Iorio

    Ministry of Education, Universities and Research, Italy

    4 publications · 86 citations

    4

    h-index

  3. AG
    A. Gopakumar

    Tata Institute of Fundamental Research, India

    4 publications · 277 citations

    4

    h-index

  4. JW
    J. W. Moffat

    University of Toronto, Canada

    4 publications · 106 citations

    4

    h-index

  5. AD
    Allah Ditta

    Zhejiang Normal University, China

    4 publications · 92 citations

    4

    h-index

1–5 of 330

Venues

  1. The Astrophysical Journal

    ApJ · 21 publications · 1.4K citations

    19

    h-index

  2. 14

    h-index

  3. 12

    h-index

  4. The European Physical Journal C

    9 publications · 272 citations

    9

    h-index

  5. Astronomy and Astrophysics

    7 publications · 956 citations

    7

    h-index

1–5