Recent results from the strong interactions program of NA61/SHINE

TL;DR

The NA61/SHINE experiment investigates hadron production across various collision systems and energies to explore the phase diagram of strongly interacting matter, aiming to identify the onset of deconfinement and the critical point.

Contribution

This paper presents recent experimental results from p+p, Be+Be, and Ar+Sc collisions, advancing the understanding of the phase diagram of strongly interacting matter.

Findings

Particle spectra comparison with previous NA49 results.

Progress in mapping the phase diagram of strongly interacting matter.

Evidence towards identifying the onset of deconfinement.

Abstract

The NA61/SHINE experiment studies hadron production in hadron+hadron, hadron+nucleus and nucleus+nucleus collisions. The strong interactions program has two main purposes: study the properties of the onset of deconfinement and search for the signatures of the critical point of strongly interacting matter. This aim is pursued by performing a two-dimensional scan of the phase diagram by varying the energy/momentum (13A-158A GeV/c) and the system size (p+p, Be+Be, Ar+Sc, Xe+La) of the collisions. This publication reviews recent results from p+p, Be+Be and Ar+Sc interactions. Measured particle spectra are discussed and compared to NA49 results from Pb+Pb collisions. The results illustrate the progress towards scanning the phase diagram of strongly interacting matter.

Full text

1 The NA61/SHINE facility

The layout of the NA61/SHINE detector detectorpaper is presented in Fig. 1. It consists of a large acceptance hadron spectrometer with excellent capabilities in charged particle momentum measurements and identification by a set of five Time Projection Chambers as well as Time-of-Flight detectors. The high resolution forward calorimeter, the Projectile Spectator Detector, measures energy flow around the beam direction, which in nucleus-nucleus reactions is primarily a measure of the number of spectator (non-interacted) nucleons and is thus related to the centrality of the collision. An array of beam detectors identifies beam particles and measures precisely their trajectories. Primary and secondary hadron as well as ion beams are used by the experiment.

2 Particle ratios in inelastic p+p collisions and inverse slope parameter T

The excellent particle identification based on the Time-off-Flight (ToF) and energy loss (dE/dx) measurements allows to calculate the ratio of yields $K^{+}/\pi^{+}$. The energy dependence of the $K^{+}/\pi^{+}$ ratio at midrapidity for inelastic p+p interactions and central Pb+Pb/Au+Au collisions is presented in Fig. 2 (left). The NA61/SHINE data suggest that even in inelastic p+p interactions the energy dependence of the $K^{+}/\pi^{+}$ ratio exhibits rapid changes in the SPS energy range. However, the horn structure 6 observed in central Pb+Pb collisions is reduced to a step. Data obtained beyond the SPS energy range, namely at RHIC and LHC 7 ; 8 ; 9 ; 10 ; 11 , continue the trend seen at the SPS.

The inverse slope parameters T for $\pi$, K and p of the spectra of transverse mass $m_{T}=\sqrt{p_{T}^{2}+m^{2}}$ were fitted in inelastic p+p reactions. Fig. 2 (right) presents the energy dependence of T for K- in p+p collision. The NA61/SHINE results from inelastic p+p collisions exhibit rapid changes like those observed in central Pb+Pb interactions. World data for p+p and Pb+Pb/Au+Au reactions are plotted for a comparison and were taken from Refs. 10 ; 12 ; 13 ; 14 .

The dependence of the mean pion multiplicity divided by the mean number of wounded nucleons (participants) as function of collision energy, the so called kink plot, is shown for inelastic p+p, Ar+Sc and A+A interactions in Fig. 3. The pion multiplicity $\left\langle\pi\right\rangle$ in the SPS energy range increases faster in central Pb+Pb than in p+p collisions. The two dependencies cross at about 40A GeV/c. For high SPS energies results from Ar+Sc reactions follow the Pb+Pb trend while for low SPS energies Ar+Sc follows the p+p tendency. The situation is opposite for Be+Be collisions.

Spectra of transverse mass $m_{T}-m_{0}$ of $\pi^{-}$ mesons in Ar+Sc are shown and compared to measurements for p+p, Be+Be, and Pb+Pb collisions in Fig. 4. Spectra in p+p reactions are exponential. A concave shape is observed in Pb+Pb, Ar+Sc and Be+Be collisions. The shape difference between p+p and A+A reactions is attributed to transverse collective flow in A+A.

3 $\Lambda$ spectra in p+p interactions

The transverse momentum distributions of $\Lambda$ hyperons shown in Fig. 5 (left) are for inelastic p+p collisions at a beam momentum of 40 GeV/c. The yields are corrected for acceptance and for losses due to the topological and track selection cuts. Integration and extrapolation of the transverse momentum distributions provide the data points for the distributions of rapidity $dn/dy$ and the Feynman variable $dn/dx_{F}$. The Feynman variable distribution of $\Lambda$ hyperons produced in inelastic p+p reactions at 40 GeV/c is shown in Fig.5 (right).

The $\Lambda$ cross-section produced in inelastic p+p interactions at 40 GeV is presented in Fig. 5 (left). Results are shown as function of transverse momentum in rapidity intervals. Fig. 5 (right) depicts the dependence of the $\Lambda$ production cross-section as function of $x_{F}$ together with the extrapolation line for determining the total yield.

Extrapolation of the $x_{F}$ distributions into the unmeasured region provides estimates of the $\Lambda$ yields. The corresponding multiplicities (average yields per event) are compared to world data in Fig. 6 (left) as function of center-of-mass energy $\sqrt{s_{NN}}$. The NA61 data follow the trend set by the world data and at the same time reduce the uncertainties of the yields significantly at the two energies analysed by NA61. Above $\sqrt{s_{NN}}=19$ GeV the experimental data have large errors and lie consistently below the EPOS model calculation. It is desirable to obtain new experimental data in this energy range. Below 10 GeV EPOS seems to overpredict $\Lambda$ yields. However, this model is not meant to provide reliable results at this energy and below. The ratio $\left\langle\Lambda\right\rangle/\left\langle\pi\right\rangle$ is shown in Fig. 6 (right) as function of $\sqrt{s_{NN}}$. The presented NA61/SHINE results agree with the world data. Measurements in A+A collisions at the AGS and by NA49 show a different behaviour than that observed in p+p reactions.

Acknowledgments

This work was supported by the Polish Ministry of Science and Higher Education (grants 667/N-CERN/2010/0, NN 202 48 4339 and NN 202 23 1837), the Polish National Center for Science (grants 2013/11/N/ST2/03879, 2014/12/T/ST2/00692, and 2015/18/M/ST2/00125),