Mapping the QCD phase diagram with statistics friendly distributions
arXiv:1811.04456 · doi:10.1103/PhysRevC.100.051902
Abstract
We demonstrate that the multiplicity distribution of a system located in the vicinity of a first-order phase transition can be successfully measured in terms of its factorial cumulants with a surprisingly small number of events. This finding has direct implications for the experimental search of a QCD phase transition conjectured to be located in the high baryon density region of the QCD phase diagram.
6 pages, 3 figures; comments added
References in corpus (4)
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- The renormalization group and quark number fluctuations in the Polyakov loop extended quark-meson model at finite baryon density
- Energy Dependence of Moments of Net-Proton and Net-Charge Multiplicity Distributions at STAR
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Cited by in corpus (14)
- Mapping the Phases of Quantum Chromodynamics with Beam Energy Scan
- Proton number fluctuations in = 2.4 GeV Au+Au collisions studied with HADES
- Quartic cumulant of baryon number in the presence of QCD critical point
- Higher-Order Cumulants and Correlation Functions of Proton Multiplicity Distributions in = 3 GeV Au+Au Collisions at the RHIC STAR Experiment
- Reconstructing particle number distributions with convoluting volume fluctuations
- Factorial cumulants from global baryon number conservation
- Factorial cumulants from short-range correlations and global baryon number conservation
- The QCD phase diagram and statistics friendly distributions
- Cumulants and factorial cumulants in the 3-dimensional Ising universality class
- Cumulants from short-range correlations and baryon number conservation - next-to-leading order
- Beam Energy Dependence of Fifth and Sixth-Order Net-proton Number Fluctuations in Au+Au Collisions at RHIC
- The time evolution of light nuclei cumulants and ratios with a first-order phase transition in the UrQMD transport model
- Fixed point behavior of cumulants in the three-dimensional Ising universality class
- QCD Critical Point and Net-Proton Number Fluctuations at RHIC-STAR