Post-accretion Core Evolution
Post-Accretion Core Evolution is a theoretical framework in planetary science that describes the ongoing physical and chemical differentiation processes within a planet's metallic core following the cessation of primary accretion, distinguishing it from earlier stages of core formation by focusing on solidification, convection, and compositional changes driven by cooling and inner core nucleation.
52
Publications
6.3K
Citations
216
Authors
149
Institutions
Publications per year
2017–2026
19
Parents
52
1–5 of 52
216
4
h-index
4
h-index
4
h-index
3
h-index
2
h-index
1–5 of 216
149
University of Münster
Münster, Germany
5 h-index
12 publications
4.5K citations
University of Cambridge
Cambridge, United Kingdom
5 h-index
8 publications
256 citations

Centre National de la Recherche Scientifique
Paris, France
5 h-index
9 publications
879 citations
University of California, Santa Cruz
Santa Cruz, United States
5 h-index
8 publications
1.5K citations
University of California, Berkeley
Berkeley, United States
4 h-index
8 publications
2.2K citations
Planetary Science Institute
Tucson, United States
4 h-index
4 publications
636 citations
California Institute of Technology
Pasadena, United States
4 h-index
4 publications
647 citations
University of Bern
Bern, Switzerland
4 h-index
7 publications
557 citations
1–8 of 149
ApJ · 8 publications · 1.1K citations
8
h-index
6 publications · 329 citations
6
h-index
5 publications · 941 citations
5
h-index
4 publications · 577 citations
4
h-index
3 publications · 122 citations
3
h-index
1–5