Lindblad Torque
Lindblad Torque is a gravitational resonance-driven force arising from the interaction between a migrating planetary body and a surrounding protoplanetary disk, distinguished by its excitation of spiral density waves at orbital resonances that transfer angular momentum and drive orbital evolution.
34
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5K
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43
Authors
51
Institutions
Publications per year
2017–2026
9
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34
Density waves in the solar nebula: Diffential Lindblad torque
William R. Ward · Icarus · 1986 · 361 citations
Disk Surface Density Transitions as Protoplanet Traps
F. Masset, Alessandro Morbidelli, A. Crida et al. · The Astrophysical Journal · 2006 · 359 citations · Full text
Natural Sciences, Astronomy, Physics +14
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Universidad Nacional Autónoma de México
Mexico City, Mexico
6 h-index
7 publications
924 citations
University of California, Santa Cruz
Santa Cruz, United States
5 h-index
7 publications
1.4K citations

Centre National de la Recherche Scientifique
Paris, France
5 h-index
12 publications
1.4K citations
University of Cambridge
Cambridge, United Kingdom
5 h-index
6 publications
571 citations
Queen Mary University of London
London, United Kingdom
4 h-index
8 publications
633 citations
Service de Physique de l'État Condensé
Gif-sur-Yvette, France
3 h-index
3 publications
592 citations

Southwest Research Institute
San Antonio, United States
3 h-index
4 publications
2.2K citations
University of California, Berkeley
Berkeley, United States
3 h-index
5 publications
322 citations
1–8 of 51
11 publications · 1.5K citations
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ApJ · 9 publications · 2.3K citations
9
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4 publications · 258 citations
4
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AJ · 2 publications · 47 citations
2
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Repository · 1 publications · 83 citations
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