Genetic Algorithms and Supernovae Type Ia Analysis
C. Bogdanos, Savvas Nesseris

TL;DR
This paper demonstrates that genetic algorithms can effectively analyze supernovae type Ia data to derive model-independent insights into dark energy evolution, offering a complementary approach to existing methods.
Contribution
It introduces genetic algorithms as a novel, non-parametric technique for analyzing supernovae data to constrain dark energy properties without model bias.
Findings
Genetic algorithms produce results consistent with established methods.
They offer a model-independent approach to supernovae data analysis.
Genetic algorithms can reduce bias from premature model assumptions.
Abstract
We introduce genetic algorithms as a means to analyze supernovae type Ia data and extract model-independent constraints on the evolution of the Dark Energy equation of state. Specifically, we will give a brief introduction to the genetic algorithms along with some simple examples to illustrate their advantages and finally we will apply them to the supernovae type Ia data. We find that genetic algorithms can lead to results in line with already established parametric and non-parametric reconstruction methods and could be used as a complementary way of treating SnIa data. As a non-parametric method, genetic algorithms provide a model-independent way to analyze data and can minimize bias due to premature choice of a dark energy model.
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