Recent results from NA61/SHINE Seweryn Kowalski for the NA61/SHINE Collaboration University of Silesia, Katowice.

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Presentation transcript:

Recent results from NA61/SHINE Seweryn Kowalski for the NA61/SHINE Collaboration University of Silesia, Katowice

NA61/SHINE – few facts Located at the CERN SPS Successor of NA49 Large acceptance spectrometer for fixed target experiment on primary (ions) and secondary (ions, hadrons) beams Data taking since 2009 NA61/SHINE is the second largest non-LHC experiment at CERN 2

Physics program Strong interactions program search for the critical point of strongly interacting matter study of the properties of the onset of deconfinement study high pT particles production (energy dependence of nuclear modification factor) Hadron-production measurements for neutrino experiments reference measurements of p+C interactions for the T2K experiment for computing initial neutrino fluxes at J-PARC Hadron-production measurements for cosmic ray experiments reference measurements of p+C, p+p, p+C, and K+C interactions for cosmic-ray physics (Pierre-Auger and KASCADE experiments) for improving air shower simulations 3

NA61/SHINE 2D scan goals 4

Facility 5

Beams for NA61/SHINE Available beams: Primary ions (13A - 158A GeV/c): Argon Xenon Lead Secondary: hadrons (p,  ±, K ± ) GeV/c ions (Be,... ) 13A - 150A GeV/c 6 Secondary ion beam composition (Pb fragmentation on Be target)

Experimental layout Unique, multi-purpose facility to study hadron production in hadron-proton, hadron-nucleus and nucleus-nucleus collisions at the CERN SPS 7

Single particle spectra in p+p 8

Single particle spectra from p+p interactions 9

Rapid changes in p+p at SPS 10 K + /  + ratio and inverse slop parameter of m T spectrum of K - exhibits rapid changes in the SPS energy range

Rapid changes in p+p at SPS – comparison with models 11 Monte-Carlo models provide poor description of data

 spectra in p+p at 158 GeV/c 12 NA61/SHINE results are consistent with world data Other NA61/SHINE energies – work in progress

Single particle spectra in Be+Be 13

Centrality selection in ion collisions 14 PSD (Projectile Spectator Detector) is located on the beam axis and measures the forward energy E F related to the non-interacting nucleons of the beam nucleus Cuts on E F allows to select different centrality classes Four event classes %5 - 10% % %

Inelastic 7 Be+ 9 Be cross section 15 13A GeV/c 20A GeV/c 30A GeV/c NA61 measurements together with 1A GeV/c Bevalac data established energy dependence of the inelastic cross section

Rapidity distributions 16

Asymmetry in  - distributions in 7 Be+ 9 Be 17 Fitted: double Gaussian function symmetrically displaced from mid– rapidity (both Gaussians have the same width, but they differ in amplitude) Asymmetry decreases from 0.86 (0-5%) to 0.97 (15-20%) Two opposite effects influence asymmetry of the spectra: asymmetric system 7 Be projectile on 9 Be target (small effect), centrality selection based on projectile spectators (large effect).

Mean multiplicities of  - in 7 Be+ 9 Be 18 NA61/SHINE p+p results published in Eur.Phys.J. C74 (2014) 2794

Transverse mass spectra of  - 19

Comparison of  - transverse mass spectra Ratio of normalized m T spectra at different energies allows to compare shape of the spectra 20 From m T – m  - > 0.3 GeV/c 2 the ratio increases with beam momentum Up to m T – m  - < 0.3 GeV/c 2 the ratio decreases with beam momentum The beam momentum dependence of the ratio observed in 7 Be+ 9 Be is not visible in Pb+Pb collisions The shape of the ratio indicates the presence of radial collective fow in 7 Be+ 9 Be The energy dependence of the ratio suggests that the radial ow increases with the collision energy

Collective effects Effect of radial flow for Pb+Pb at all energies Inverse slop parameter T larger in 7 Be+ 9 Be than in p+p → possible evidence of transverse collective flow in 7 Be+ 9 Be 21

Fluctuations and correlations 22

Fluctuations 23 Theoretical fluctuations in presence of critical point N-p T fluctuations in p+p and centrality selected Be+Be No sign of any anomaly that can be attributed to the critical point (neither in p+p nor Be+Be)

Two-particle correlations in ,  in p+p 24 NA61/SHINE: maximum at (  ) = (0,  ) probably due to resonance decays and momentum conservation NA61 results show stronger enhancement in    and no “jet peak” at   0 (in comparison with ALICE)

Future of NA61/SHINE 25

Open charm measurements 26 D 0 candidates selected by TPCs and vertex detector D 0 candidates selected by TPCs only Feasibility of the D 0 meson measurements in two body decay channel: D 0  K + +  -, in central Pb+Pb collisions at the top SPS energy Simulation for 200k events (0.5 day of data taking) Vertex detector: four pixel detection stations MIMOSA-26AHR sensor

Extension of the data taking plan 27

Summary NA61/SHINE measures collisions of hadrons and ions for three physics programs: strong interactions, neutrions and cosmic ray studies in SPS energy range High precision double – differential pion spectra were measured in p+p and 7 Be+ 9 Be collisions at 5 different energies Rapid changes in particle production observed in p+p interactions at mid-SPS energy Collective effects are observed in 7 Be+ 9 Be reactions No sign of any anomaly that can be attributed to critical point in p+p and 7 Be+ 9 Be interactions 28

THANK YOU 29

BACKUP SLIDES 30

Secondary beryllium beam Fragmentation target length optimized to maximize the production of the desired fragment Double magnetic spectrometer separates fragments according to the selected magnetic rigidity Possible to use degrader, Cu plate where ions lose energy according to the charge 31 Secondary beam

NA61/SHINE Detector 32 Large acceptance: 50% High momentum resolution:  (p)/p 2 ≈ (GeV /c) -1 (at full B=9 T m) ToF walls resolution: ToF-L/R:  (t) ≈ 60ps; ToF-F:  (t) ≈ 120ps Good particle identification:  (dE/dx)/ ≈ 0.04;  (m inv ) ≈ 5MeV High detector efficiency: 95% Event recording rate: 70 events/sec 7 Be+ 9 GeV/c

Energy loss (dE/dx) method In each p, p T bin sum of Gauss functions is fitted to the dE/dx spectrum For each track the probability for being a hadron of specific type is calculated based on the fitted dE/dx distribution Sum of these probabilities gives the mean multiplicity of the identified hadrons 33

Energy loss (dE/dx) vs time of flight (tof) method 34 Fit a two-dimensional weighted Gaussian function in the mass 2 vs dE/dx plane

V 0 – method 35 Results are consistent with PDG value (c   = 7.89 cm) Lifetime is calculated based on the difference between position of the main and the decay vertex  mass from PDG ±0.006±0.006 GeV/c 2

h - analysis method 36

Precise measurements (  - meson) 7 Be+ 9 Be collisions 37 p+p collisions

Hadron-production measurements for neutrino experiments 38 The T2K experiment published a measurement of  13 angle in the neutrino mixing matrix (PRL 107, (2011)) Systematic error estimate was based on the NA61/SHINE results

39  KK p KK  K0sK0s High statistics 2009 p+C at 31GeV/c “thin-target” dataset s inel = ± 2.8(stat) ± 2.4(det) ± 0.3(mod) mb s prod = ± 2.8(stat) ± 2.4(det) ± 3.6(mod) mb Hadron-production measurements for neutrino experiments

Extension of the neutrino program by measurements for FERMILAB experiments Six US-NA61 Measurements with NuMi and LBNE replica target 40

Hadron-production measurements for cosmic ray experiments 41 m production related to hadronic interactions at fixed-target energies m production related to hadronic interactions at fixed-target energies Modern detector installations: high statistics/quality data Modern detector installations: high statistics/quality data Strong model dependence: due mainly to simulation of m production Strong model dependence: due mainly to simulation of m production Indirect measurement (extensive air showers): simulations needed Indirect measurement (extensive air showers): simulations needed Cosmic ray composition of central importance for understanding sources, kink, ankle... Cosmic ray composition of central importance for understanding sources, kink, ankle...

Hadron-production measurements for cosmic ray experiments 42 Input for validation/tuning of Monte Carlo generators Cross sections measurements