TL;DR
This paper introduces a fast C++ library with interfaces for efficiently computing thermal functions crucial in finite-temperature quantum field theory and early Universe phase transitions.
Contribution
A new, optimized C++ implementation of thermal functions with Mathematica and Python interfaces for scientific applications.
Findings
Significantly faster computation of thermal functions.
Accurate results suitable for cosmological phase transition studies.
Easy integration into existing scientific workflows.
Abstract
We provide a small C++ library with Mathematica and Python interfaces for computing thermal functions, defined which appear in finite-temperature quantum field theory and play a role in phase-transitions in the early Universe, including baryogenesis, electroweak symmetry breaking and the Higgs mechanism.
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