Rotational Disruption of Astrophysical Dust and Ice: Theory and Applications
Thiem Hoang

TL;DR
This paper reviews new mechanisms of dust destruction in space, specifically rotational disruption caused by radiative torques and mechanical torques, which impact dust properties and observations across various astrophysical environments.
Contribution
It introduces and discusses the novel dust destruction mechanisms of radiative torque disruption (RATD) and mechanical torque disruption (METD), expanding understanding of dust evolution in space.
Findings
RATD effectively disrupts dust grains in diverse radiation fields.
METD causes dust destruction through grain motion relative to gas.
These mechanisms influence dust size distribution and observational signatures.
Abstract
Dust is an essential component of the interstellar medium (ISM) and plays an important role in many different astrophysical processes and phenomena. Traditionally, dust grains are known to be destroyed by thermal sublimation, Coulomb explosions, sputtering, and shattering. The first two mechanisms arise from the interaction of dust with intense radiation fields and high-energy photons (extreme UV), which work in a limited astrophysical environment. The present review is focused on a new destruction mechanism present in the {\it dust-radiation interaction} that is effective in a wide range of radiation fields and has ubiquitous applications in astrophysics. We first describe this new mechanism of grain destruction, namely rotational disruption induced by Radiative Torques (RATs) or RAdiative Torque Disruption (RATD). We then discuss rotational disruption of nanoparticles by mechanical…
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