Non-equilibrium photons from the bottom-up thermalization scenario

In this work, I calculate the p⊥ resolved spectra for the three stages of the bottom-up scenario, which are comparable to the thermal contribution, particularly at higher values of the saturation scale Q2. Analytical solutions are obtained by including a parametrization of scaling solutions from far...

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1. Verfasser: García-Montero, Oscar (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: [August 2022]
In: Annals of physics
Year: 2022, Jahrgang: 443, Pages: 1-23
DOI:10.1016/j.aop.2022.168984
Online-Zugang:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1016/j.aop.2022.168984
Verlag, lizenzpflichtig, Volltext: https://www.sciencedirect.com/science/article/pii/S0003491622001403
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Verfasserangaben:Oscar Garcia-Montero (Institut für Theoretische Physik, Universität Heidelberg)

MARC

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520 |a In this work, I calculate the p⊥ resolved spectra for the three stages of the bottom-up scenario, which are comparable to the thermal contribution, particularly at higher values of the saturation scale Q2. Analytical solutions are obtained by including a parametrization of scaling solutions from far-from-equilibrium classical statistical lattice simulations into a small angle kinetic rate. Furthermore, a theoretically motivated ansatz is used to account for near-collinear enhancement of the low-p⊥ radiation. The system is phenomenologically constrained using the charged hadron multiplicities from LHC and RHIC as in previous parametric estimates and fair agreement with the data available for photons was found. I find that for this realistic set of parameters, the contribution from the pre-equilibrium dominates the excess photons. 
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