Secular Stability is a theoretical construct in orbital dynamics denoting the long-term resistance of orbital configurations to cumulative perturbations over astronomical timescales, distinguished from short-term oscillatory stability by its focus on gradual, non-periodic evolution of orbital elements.
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Secular instability of rotating Newtonian stars
John L. Friedman, B. F. Schutz · The Astrophysical Journal · 1978 · 567 citations · Full text
Natural Sciences, Astronomy, Physics +16
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The University of Tokyo
Tokyo, Japan
6 h-index
8 publications
240 citations
Centre National de la Recherche Scientifique
Paris, France
4 h-index
6 publications
111 citations
Max Planck Institute for Gravitational Physics
Potsdam, Germany
3 h-index
4 publications
764 citations
California Institute of Technology
Pasadena, United States
2 h-index
2 publications
114 citations
University of Oregon
Eugene, United States
2 h-index
2 publications
47 citations
Université Grenoble Alpes
Saint-Martin-d'Hères, France
2 h-index
2 publications
29 citations
University of the Witwatersrand
Johannesburg, South Africa
2 h-index
4 publications
58 citations
Indiana University Bloomington
Bloomington, United States
2 h-index
4 publications
117 citations
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- The Astrophysical Journal
ApJ · 25 publications · 1.6K citations
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- Monthly Notices of the Royal Astronomical Society
7 publications · 222 citations
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- Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields
3 publications · 281 citations
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- Astrophysics and Space Science
3 publications · 42 citations
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- Physical Review Letters
PRL · 3 publications · 547 citations
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