POET: A Model for (P)lanetary (O)rbital (E)volution due to (T)ides on Evolving Stars
Kaloyan Penev, Michael Zhang, Brian Jackson

TL;DR
POET is a comprehensive, publicly available tool that models the evolution of planetary orbits due to stellar tides, incorporating detailed stellar physics and angular momentum transfer, with ongoing development for more complex orbital configurations.
Contribution
It introduces the first model to fully include stellar angular momentum evolution, tidal dissipation, and stellar wind effects in planetary orbit evolution calculations.
Findings
Accurately models circular aligned planetary orbit evolution due to tides.
Accounts for stellar angular momentum transfer and wind loss.
Provides extensive documentation for community use and extension.
Abstract
We make publicly available an efficient, versatile, easy to use and extend tool for calculating the evolution of circular aligned planetary orbits due to the tidal dissipation in the host star. This is the first model to fully account for the evolution of the angular momentum of the stellar convective envelope by the tidal coupling, the transfer of angular momentum between the stellar convective and radiative zones, the effects of the stellar evolution on the tidal dissipation efficiency and stellar core and envelope spins, the loss of stellar convective zone angular momentum to a magnetically launched wind and frequency dependent tidal dissipation. This is only a first release and further development is under way to allow calculating the evolution of inclined and eccentric orbits, with the latter including the tidal dissipation in the planet and its feedback on planetary structure.…
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