On the Spiral Structures in Heavy-Ion Collisions
A. Rustamov, J. N. Rustamov

TL;DR
This paper explores the potential presence of spiral structures in heavy-ion collisions, suggesting they could serve as indicators of phase transitions shortly after the Big Bang, drawing parallels with galactic spiral patterns.
Contribution
It introduces a novel hypothesis that spiral structures may form in heavy-ion collisions, linking cosmic galactic patterns to subatomic phenomena through self-similarity.
Findings
Spiral structures could be signatures of phase transitions in heavy-ion collisions.
Galactic spiral patterns and collision structures may share underlying self-similar dynamics.
Proposes a new way to interpret signals from early universe conditions.
Abstract
It is well established that many galaxies, like our Milky Way, exhibit spiral patterns. The entire galactic disc rotates about the galactic centre with different speeds; higher closer to the centre, lower at greater distances - that is, galactic discs do not rotate like a solid compact disc. The spiral arms are the part of the galactic disc where many young stars are being born. Since young stars are also brightest, we can see the spiral structure of other galaxies from afar. Typically spiral galaxies are copiously observed at redshifts z ~ 1. The recently observed grand-design galaxy Q2343-BX442 at z=2.18, however, implies uncertain origin of its spiral structure. Indeed such "old" galaxies usually look rather clumpy because of their dynamically hot discs. In this report, based on self-similarity, we argue that spiral structures may also appear in heavy-ion collisions as messengers of…
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Taxonomy
TopicsHigh-Energy Particle Collisions Research
