Higher-order Gravity Coefficients

Higher-Order Gravity Coefficients is a mathematical construct in planetary gravity modeling that represents the deviation of a celestial body's gravitational field from spherical symmetry, distinguished by its derivation from terms beyond the second degree in the spherical harmonic expansion of the gravitational potential.

21

Publications

746

Citations

29

Authors

27

Institutions

Publications per year

2017–2026

4

Variants

Higher-degree Gravity Coefficients

Authors

29

  1. SC
    Salvatore Capozzıello

    Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Italy

    3 publications · 207 citations

    3

    h-index

  2. JD
    John D. Barrow

    University of Cambridge, United Kingdom

    2 publications · 60 citations

    2

    h-index

  3. MD
    Mariafelicia De Laurentis

    Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Italy

    2 publications · 186 citations

    2

    h-index

  4. SC
    Spiros Cotsakis

    University of the Aegean, Greece

    2 publications · 60 citations

    2

    h-index

  5. RJ
    R. J. Anderle

    Naval Surface Warfare Center, United States

    1 publications · 17 citations

    1

    h-index

1–5 of 29

Venues

  1. General Relativity and Gravitation

    4 publications · 138 citations

    4

    h-index

  2. Physics Letters B

    3 publications · 78 citations

    3

    h-index

  3. Astroparticle Physics

    2 publications · 186 citations

    2

    h-index

  4. Physical review. D/Physical review. D.

    PRD · 1 publications · 42 citations

    1

    h-index

  5. Periodica Polytechnica Civil Engineering

    1 publications · 16 citations

    1

    h-index

1–5