Two-dimensional Bayesian Approach for Centrality Determination in Nucleus-Nucleus Collisions
D. Idrisov, F. Guber, N. Karpushkin, P. Parfenov
TL;DR
This work tackles centrality determination in nucleus-nucleus collisions by introducing a two-dimensional Bayesian framework based on the observables $(N_{ ext{hits}}, E_{ ext{spec}})$. A two-dimensional Gamma distribution, decorrelated through a rotation, models the joint fluctuations at fixed $b$, with moments tied to centrality via polynomial fits in the centrality variable $c_b$ and calibrated for experimental effects using factors $oldsymbol{ ext{alpha}}$ and $oldsymbol{ extbeta}$ and an efficiency $oldsymbol{ extepsilon}$. The Bayes posterior $P(b|E_{ ext{spec}},N_{ ext{hits}})$ is computed to reconstruct impact-parameter distributions, and centrality classes are obtained via constrained clustering; applied to simulated Xe+CsI collisions at $3.8$ AGeV, the method reproduces model $b$ distributions within about 2% and reduces autocorrelation in proton multiplicity analyses. An appendix develops a two-parameter Glauber-type description of multiplicity fluctuations, separating volume and particle-production fluctuations and enabling parameter reduction when comparing data to simulations. Overall, the approach provides a robust, low-bias centrality estimator suitable for low-multiplicity heavy-ion systems and sets the stage for expanding the observable set in BM@N.
Abstract
The determination of centrality in nucleus-nucleus collisions is a crucial task as it enables the estimation of the impact parameter and hence allows for the comparison of experimental results with data from theoretical models and other experiments. In this work, we present a two-dimensional approach for centrality determination based on a Bayesian framework. The observables used were the number of track hits and the deposited energy of spectators in the forward hadronic calorimeter. A distribution is proposed to describe the fluctuations of these two observables at a fixed impact parameter value, which provides a significantly superior description of the observable distributions in both central and peripheral regions. The effectiveness of the proposed method was verified for the BM@N experiment using simulated data for Xe+CsI collisions at a beam energy of 3.8 AGeV.
