The Jeans Mass as a Fundamental Measure of Self-Gravitating Disc Fragmentation and Initial Fragment Mass
Duncan Forgan, Ken Rice

TL;DR
This paper introduces a method to estimate the initial masses of fragments in self-gravitating protostellar discs using the local Jeans mass, providing insights into the typical masses and fragmentation conditions.
Contribution
It presents a novel approach to predict initial fragment masses in self-gravitating discs based on the local Jeans mass, linking it to various fragmentation criteria.
Findings
Minimum fragment mass around 3 Jupiter masses.
Most common fragment masses between 10 and 20 Jupiter masses.
The Jeans mass-based criterion recovers previous fragmentation conditions.
Abstract
As a formation route for objects such as giant planets and low-mass stars in protostellar discs (as well as stars in AGN discs), theories of self-gravitating disc fragmentation need to be able to predict the initial masses of fragments. We describe a means by which the local Jeans mass inside the spiral structure of a self-gravitating disc can be estimated. If such a self-gravitating disc satisfies the criteria for disc fragmentation, this estimate provides a lower limit for the initial mass of any fragments formed. We apply this approach to a series of self-gravitating protostellar disc models, to map out the typical masses of fragments produced by this formation mode. We find a minimum fragment mass of around 3 Jupiter masses, which is insensitive to the stellar mass, and that - within the parameter space surveyed - fragments with masses between 10 and 20 Jupiter masses are the most…
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