Orbit decay of 2-100 au planetary remnants around white dwarfs with no gravitational assistance from planets
Dimitri Veras, Yusuf Birader, Uwais Zaman

TL;DR
This paper proposes a new mechanism for white dwarf metal pollution that involves small bodies being radiatively dragged inward without the need for planetary perturbations, expanding understanding of debris accretion.
Contribution
It introduces a novel planet-less model for white dwarf pollution by coupling Poynting-Robertson, Yarkovsky, and YORP effects driven solely by white dwarf radiation.
Findings
Effective for dust particles up to 80 au from the white dwarf.
Can spin up and fragment large boulders into smaller debris.
Suggests a significant fraction of white dwarf pollution may occur without planetary influence.
Abstract
A widely-held assumption is that each single white dwarf containing observable rocky debris requires the presence of at least one terrestrial or giant planet to have gravitationally perturbed the progenitor of the debris into the star. However, these planets could have been previously been engulfed by the star or escaped the system, leaving behind asteroids, boulders, cobbles, pebbles, sand and dust. These remaining small bodies could then persist throughout the host star's evolution into a white dwarf at ~2-100 au scales, and then be radiatively dragged into the white dwarf without the help of a planet. Here we identify the parameter space and cooling ages for which this one metal-pollution mechanism is feasible by, for the first time, coupling Poynting-Robertson drag, the Yarkovsky effect and the YORP effect solely from rapidly dimming white dwarf radiation. We find that this…
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