Foretellings of Ragnar\"ok: World-engulfing Asymptotic Giants and the Inheritance of White Dwarfs
Alexander James Mustill, Eva Villaver

TL;DR
This paper models the evolution of planets during the AGB phase of stars, revealing how tidal forces and stellar mass loss influence planetary survival and orbital expansion, with implications for planets around White Dwarfs.
Contribution
It provides the first detailed study of planetary evolution during each thermal pulse on the AGB, considering tidal forces, mass loss, and eccentricity effects.
Findings
Jovian planets within ~3-5 AU can be engulfed by the star.
Lower-mass planets within 1.5-3 AU may survive due to orbital expansion.
Planets are unlikely to be found within ~1.5 AU of White Dwarfs from 1M_Sol progenitors.
Abstract
The search for planets around White Dwarf stars, and evidence for dynamical instability around them in the form of atmospheric pollution and circumstellar discs, raises questions about the nature of planetary systems that can survive the vicissitudes of the Asymptotic Giant Branch (AGB). We study the competing effects, on planets at several AU from the star, of strong tidal forces arising from the star's large convective envelope, and of the planets' orbital expansion due to stellar mass loss. We, for the first time, study the evolution of planets while following each thermal pulse on the AGB. For Jovian planets, tidal forces are strong, and can pull into the envelope planets initially at ~3 AU for a 1M_Sol star and ~5 AU for a 5M_Sol star. Lower-mass planets feel weaker tidal forces, and Terrestrial planets initially within 1.5-3 AU enter the stellar envelope. Thus, low-mass planets…
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