Planet masses and radii from physical principles

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Planetary Systems: Formation

Scientific paper

Masses and radii are the primary observables to characterize exoplanets
today. A self-consistent theoretical approach is presented that allows
to calculate mass- and radius-distributions of exoplanet populations
from basic physical principles and avoids the usual parametrisation of a
multitude of processes.

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