EOS Manual
Li Zeng, Stein B. Jacobsen, Dimitar D. Sasselov, and Michail I. Petaev

TL;DR
This paper provides a detailed methodology for deriving exoplanet mass-radius relations from equations of state, aiding understanding of their compositions and formation scenarios.
Contribution
It offers a comprehensive step-by-step guide to implement EOS in internal structure models of exoplanets, emphasizing the physics and chemistry involved.
Findings
Method for converting EOS into mass-radius relations
Insights into planetary composition and structure
Framework applicable to various planetary materials
Abstract
The exoplanet field now abounds with new discoveries of planets and planetary systems. It is of great interest for the scientific community to understand the compositions and internal structures of these new planets outside our own solar system, and then infer their formation scenarios. In particular, the proper implementation of the equation-of-states of various matters into the calculation of internal structure is crucial. Thus, we have come up with this write-up that provides the detailed steps to turn an equation-of-state (EOS) into a mass-radius relation of exoplanets, and highlight the physics and chemistry involved in these calculations. It must be visualized!
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Taxonomy
TopicsStellar, planetary, and galactic studies
