A Coverage Study of the CMSSM Based on ATLAS Sensitivity Using Fast Neural Networks Techniques
arXiv:1011.4306 · doi:10.1007/JHEP03(2011)012
Abstract
We assess the coverage properties of confidence and credible intervals on the CMSSM parameter space inferred from a Bayesian posterior and the profile likelihood based on an ATLAS sensitivity study. In order to make those calculations feasible, we introduce a new method based on neural networks to approximate the mapping between CMSSM parameters and weak-scale particle masses. Our method reduces the computational effort needed to sample the CMSSM parameter space by a factor of ~ 10^4 with respect to conventional techniques. We find that both the Bayesian posterior and the profile likelihood intervals can significantly over-cover and identify the origin of this effect to physical boundaries in the parameter space. Finally, we point out that the effects intrinsic to the statistical procedure are conflated with simplifications to the likelihood functions from the experiments themselves.
Further checks about accuracy of neural network approximation, fixed typos, added refs. Main results unchanged. Matches version accepted by JHEP
References in corpus (14)
- Bayes in the sky: Bayesian inference and model selection in cosmology
- The RooStats Project
- Indirect Dark Matter Detection from Dwarf Satellites: Joint Expectations from Astrophysics and Supersymmetry
- Implications for the Constrained MSSM from a new prediction for b to s gamma
- Natural Priors, CMSSM Fits and LHC Weather Forecasts
- Bayesian Selection of sign(mu) within mSUGRA in Global Fits Including WMAP5 Results
- Measuring Supersymmetry
- Fast cosmological parameter estimation using neural networks
- Identification of Dark Matter particles with LHC and direct detection data
- The Dark Side of mSUGRA
- On prospects for dark matter indirect detection in the Constrained MSSM
- Prospects for dark matter detection with IceCube in the context of the CMSSM
- Global Fits of the Large Volume String Scenario to WMAP5 and Other Indirect Constraints Using Markov Chain Monte Carlo
- Panglossian Prospects for Detecting Neutralino Dark Matter in Light of Natural Priors