Cosmic Strings and the Origin of Globular Clusters
Alistair Barton, Robert H. Brandenberger, Ling Lin (McGill, University)

TL;DR
This paper proposes that cosmic string loops could be the initial seeds for globular clusters, explaining their properties and distribution within galaxies by matching theoretical predictions with observed data.
Contribution
It introduces a novel hypothesis linking cosmic strings to globular cluster formation and derives predictions consistent with observed globular cluster distributions.
Findings
Cosmic string tension fixed by matching mass distribution peaks.
Predicted number density of globular clusters aligns with observations.
Explains why globular clusters are old, dense, and located in galactic halos.
Abstract
We hypothesize that cosmic string loops are the seeds about which globular clusters accrete. Fixing the cosmic string tension by demanding that the peak in the distribution of masses of objects accreting onto string loops agrees with the peak in the observed mass distribution of globular clusters in our Milky Way galaxy, we then compute the expected number density and mass function of globular clusters, and compare with observations. Our hypothesis naturally explains why globular clusters are the oldest and most dense objects in a galaxy, and why they are found in the halo of the galaxy.
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