TY - JOUR
T1 - Genetic algorithms and experimental discrimination of SUSY models
AU - Allanach, Benjamin C.
AU - Grellscheid, David
AU - Quevedo, Fernando
PY - 2004/7/1
Y1 - 2004/7/1
N2 - We introduce genetic algorithms as a means to estimate the accuracy required to discriminate among different models using experimental observables. We exemplify the technique in the context of the minimal supersymmetric standard model. If supersymmetric particles are discovered, models of supersymmetry breaking will be fit to the observed spectrum and it is beneficial to ask beforehand: what accuracy is required to always allow the discrimination of two particular models and which are the most important masses to observe? Each model predicts a bounded patch in the space of observables once unknown parameters are scanned over. The questions can be answered by minimising a "distance" measure between the two hypersurfaces. We construct a distance measure that scales like a constant fraction of an observable. Genetic algorithms, including concepts such as natural selection, fitness and mutations, provide a solution to the minimisation problem. We illustrate the efficiency of the method by comparing three different classes of string models for which the above questions could not be answered with previous techniques. The required accuracy is in the range accessible to the Large Hadron Collider (LHC) when combined with a future linear collider (LC) facility. The technique presented here can be applied to more general classes of models or observables.
AB - We introduce genetic algorithms as a means to estimate the accuracy required to discriminate among different models using experimental observables. We exemplify the technique in the context of the minimal supersymmetric standard model. If supersymmetric particles are discovered, models of supersymmetry breaking will be fit to the observed spectrum and it is beneficial to ask beforehand: what accuracy is required to always allow the discrimination of two particular models and which are the most important masses to observe? Each model predicts a bounded patch in the space of observables once unknown parameters are scanned over. The questions can be answered by minimising a "distance" measure between the two hypersurfaces. We construct a distance measure that scales like a constant fraction of an observable. Genetic algorithms, including concepts such as natural selection, fitness and mutations, provide a solution to the minimisation problem. We illustrate the efficiency of the method by comparing three different classes of string models for which the above questions could not be answered with previous techniques. The required accuracy is in the range accessible to the Large Hadron Collider (LHC) when combined with a future linear collider (LC) facility. The technique presented here can be applied to more general classes of models or observables.
KW - Beyond Standard Model
KW - Supersymmetry Breaking
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U2 - 10.1088/1126-6708/2004/07/069
DO - 10.1088/1126-6708/2004/07/069
M3 - Article
AN - SCOPUS:23044501233
SN - 1029-8479
VL - 8
SP - 1717
EP - 1738
JO - Journal of High Energy Physics
JF - Journal of High Energy Physics
IS - 7
ER -