Javascript must be enabled to continue!
Using Spectator Matter for Centrality Determination in Nucleus-Nucleus Collisions
View through CrossRef
One of the common methods to measure the centrality of nucleus-nucleus collision events consists of detecting forward spectator neutrons. Because of non-monotonic dependence of neutron numbers on centrality, other characteristics of spectator matter in 197Au–197Au collisions at NICA must be considered to improve the centrality determination. The numbers of spectator deuterons and α-particles and the forward–backward asymmetry of the numbers of free spectator nucleons were calculated with the Abrasion–Ablation Monte Carlo for Colliders (AAMCC) model as functions of event centrality. It was shown that the number of charged fragments per spectator nucleon decreases monotonically with an increase of the impact parameter, and thus can be used to estimate the collision centrality. The conditional probabilities that a given event with specific spectator characteristics belongs to a certain centrality class were calculated by means of AAMCC. Such probabilities can be used as an input to Bayesian or other machine-learning approaches to centrality determination in 197Au–197Au collisions.
Title: Using Spectator Matter for Centrality Determination in Nucleus-Nucleus Collisions
Description:
One of the common methods to measure the centrality of nucleus-nucleus collision events consists of detecting forward spectator neutrons.
Because of non-monotonic dependence of neutron numbers on centrality, other characteristics of spectator matter in 197Au–197Au collisions at NICA must be considered to improve the centrality determination.
The numbers of spectator deuterons and α-particles and the forward–backward asymmetry of the numbers of free spectator nucleons were calculated with the Abrasion–Ablation Monte Carlo for Colliders (AAMCC) model as functions of event centrality.
It was shown that the number of charged fragments per spectator nucleon decreases monotonically with an increase of the impact parameter, and thus can be used to estimate the collision centrality.
The conditional probabilities that a given event with specific spectator characteristics belongs to a certain centrality class were calculated by means of AAMCC.
Such probabilities can be used as an input to Bayesian or other machine-learning approaches to centrality determination in 197Au–197Au collisions.
Related Results
Nature Transformed: English Landscape Gardens and <i>Theatrum Mundi</i>
Nature Transformed: English Landscape Gardens and <i>Theatrum Mundi</i>
IntroductionThe European will to modify the natural world emerged through English landscape design during the eighteenth century. Released from the neo-classical aesthetic dichotom...
Probing Short-Range Nucleon–Nucleon Correlations by Detecting Spectator Neutrons in Collider Experiments
Probing Short-Range Nucleon–Nucleon Correlations by Detecting Spectator Neutrons in Collider Experiments
We investigate whether short-range nucleon–nucleon correlations (NN-SRC) and cluster configurations in nuclei can be explored by studying spectator neutrons produced in high-energy...
Pre-Equilibrium Clustering in Production of Spectator Fragments in Collisions of Relativistic Nuclei
Pre-Equilibrium Clustering in Production of Spectator Fragments in Collisions of Relativistic Nuclei
An algorithm of pre-equilibrium clustering of spectator matter based on the construction of the minimum spanning tree (MST) is presented. The algorithm was implemented in the Abras...
Peeling away surface neutrons from 209Bi in asymmetric collisions
Peeling away surface neutrons from 209Bi in asymmetric collisions
The emission of spectator neutrons and protons in ultracentral collisions of Bi with the same (Bi) or lighter (W, Cu) target nuclei has been simulated using the Abrasion-Ablation M...
Outcome of Collisions in the Early Outer Solar System
Outcome of Collisions in the Early Outer Solar System
AbstractThe processes leading to the formation of planetary systems leave behind a significant mass of small bodies - up to 35 Earth masses depending on the model [1] - orbiting at...
W±-boson production in p–Pb collisions at $$ \sqrt{s_{\textrm{NN}}} $$ = 8.16 TeV and Pb–Pb collisions at $$ \sqrt{s_{\textrm{NN}}} $$ = 5.02 TeV
W±-boson production in p–Pb collisions at $$ \sqrt{s_{\textrm{NN}}} $$ = 8.16 TeV and Pb–Pb collisions at $$ \sqrt{s_{\textrm{NN}}} $$ = 5.02 TeV
Abstract
The production of the W± bosons measured in p–Pb collisions at a centre-of-mass energy per nucleon–nucleon collision $$ \sqrt{s_{\textrm{NN}}} $$
...
Study of $$\langle {p}_{\text{T}}\rangle $$ and its higher moments, and extraction of the speed of sound in Pb-Pb collisions with ALICE
Study of $$\langle {p}_{\text{T}}\rangle $$ and its higher moments, and extraction of the speed of sound in Pb-Pb collisions with ALICE
A
bstract
Ultrarelativistic heavy-ion collisions produce a state of hot and dense strongly interacting...
Cell Nucleus
Cell Nucleus
Abstract
The cell nucleus is a double membrane‐bound organelle that contains the genetic information of the cell packaged in the form of chromat...

