The Physical Origin of the Stellar Initial Mass Function
Patrick Hennebelle, Michael Y. Grudi\'c

TL;DR
This paper reviews the physical processes and theories behind the stellar initial mass function (IMF), emphasizing gravity, turbulence, and dust physics as key factors in its origin and apparent universality.
Contribution
It synthesizes current understanding and numerical simulations to explain the physical origins of the IMF, highlighting the roles of gravity, turbulence, and dust physics.
Findings
Gravity and turbulence shape the high-mass IMF slope.
Multiple regimes of the IMF are possible depending on Mach number and density.
Protostellar jets influence the IMF by injecting momentum and unbinding gas.
Abstract
Stars are amongst the most fundamental structures of our Universe. They comprise most of the baryonic and luminous mass of galaxies, synthethise heavy elements, and injec\ t mass, momentum, and energy into the interstellar medium. They are also home to the planets. Since stellar properties are primarily decided by their mass, the so-called \ stellar initial mass function (IMF) is critical to the structuring of our Universe. We review the various physical processes, and theories which have been put forward as well as the numerical simulations which have been carried out to explain the origin of the stellar initial mass function. Key messages from this review are: (1) Gravity and turbulence most likely determine the power-law, high-mass part of the IMF. (2) Depending of the Mach number and the density distribution, several regimes are possible, including , -0.8, -1…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Stellar, planetary, and galactic studies · Gamma-ray bursts and supernovae
