Is There a Universal Mass Function?
Bruno Binggeli, Tatjana Hascher

TL;DR
This paper investigates the possibility of a universal mass function across all astronomical objects, from asteroids to galaxy clusters, revealing a surprisingly continuous distribution over 36 orders of magnitude.
Contribution
It demonstrates that various object classes' mass functions can be combined into a single, nearly universal power-law distribution spanning a vast mass range.
Findings
Mass functions of different objects follow a power law with slope -2.
CDM halos exhibit a similar universal slope across scales.
Planets and small bodies have a flatter mass distribution.
Abstract
Following an old idea of Fritz Zwicky, we make an attempt to establish a universal mass function for astronomical objects on all scales. The object classes considered are: solar system planets and small bodies, exoplanets, brown dwarfs, stars and stellar remnants, open and globular clusters, molecular clouds, galaxies, groups and clusters of galaxies. For comparison we also include CDM halos taken from numerical simulations. We show that the mass functions of individual object classes, when properly normalized, can indeed be concatenated to build a surprisingly continuous mass function of the universe, from approximately M = 10^(-20)Msun (sub-kilometer size asteroids) up to M = 10^(16)Msun (rich clusters of galaxies), covering 36 orders of magnitude in mass. Most individual mass functions roughly follow a power law of the form phi(M) propto M^(-2). A notable exception are planets and…
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