The ProtoDUNE-SP detector is a single-phase liquid argon time projection chamber with an active volume of 7.2× 6.1× 7.0 m3. It is installed at the CERN Neutrino Platform in a specially-constructed beam that delivers charged pions, kaons, protons, muons and electrons with momenta in the range 0.3 GeV/c to 7 GeV/c. Beam line instrumentation provides accurate momentum measurements and particle identification. The ProtoDUNE-SP detector is a prototype for the first far detector module of the Deep Underground Neutrino Experiment, and it incorporates full-size components as designed for that module. This paper describes the beam line, the time projection chamber, the photon detectors, the cosmic-ray tagger, the signal processing and particle reconstruction. It presents the first results on ProtoDUNE-SP's performance, including noise and gain measurements, dE/dx calibration for muons, protons, pions and electrons, drift electron lifetime measurements, and photon detector noise, signal sensitivity and time resolution measurements. The measured values meet or exceed the specifications for the DUNE far detector, in several cases by large margins. ProtoDUNE-SP's successful operation starting in 2018 and its production of large samples of high-quality data demonstrate the effectiveness of the single-phase far detector design.

The deep underground neutrino experiment (DUNE), a 40-kton underground liquid argon time projection chamber experiment, will be sensitive to the electron-neutrino flavor component of the burst of neutrinos expected from the next Galactic core-collapse supernova. Such an observation will bring unique insight into the astrophysics of core collapse as well as into the properties of neutrinos. The general capabilities of DUNE for neutrino detection in the relevant few- to few-tens-of-MeV neutrino energy range will be described. As an example, DUNE’s ability to constrain the $$\nu _e$$ ν e spectral parameters of the neutrino burst will be considered.

We have measured rapidity densities dN/dy of π ± and K ± over a broad rapidity range (−0.1 < y < 3.5) for central Au+Au collisions at √ sNN = 200 GeV. These data have significant implications for the chemistry and dynamics of the dense system that is initially created in the collisions. The full phase-space yields are 1660±15±133 (πThe systematics of the strange to non-strange meson ratios are found to track the variation of the baryo-chemical potential with rapidity and energy. Landau-Carruthers hydrodynamic is found to describe the bulk transport of the pions in the longitudinal direction.In ultra-relativistic heavy ion collisions at RHIC energies, charged pions and kaons are produced copiously. The yields of these light mesons are indicators of the entropy and strangeness created in the reactions, sensitive observables to the possible existence of an early color deconfined phase, the so-called quark gluon plasma. In such collisions, the large number of produced particles and their subsequent reinteractions, either at the partonic or hadronic level, motivate the application of concepts of gas or fluid dynamics in their interpretation. Hydrodynamical properties of the expanding matter created in heavy ion reactions have been discussed by Landau [1] (full stopping) and Bjorken [2] (transparency), in theoretical pictures using different initial conditions. In both scenarios, thermal equilibrium is quickly achieved and the subsequent isentropic expansion is governed by hydrodynamics. The relative abundances and kinematic properties of particles provide an important tool for testing whether equilibrium occurs in the course of the collision. In discussing the source characteristics, it is important to measure most of the produced particles in order not to violate conservation laws (e.g. strangeness and charge conservation).In this letter, we report on the first measurements at RHIC energies of transverse momentum (p T ) spectra of π ± and K ± over the rapidity range −0.1 < y < 3.5 for the 5% most central Au+Au collisions at √ s N N = 200 GeV. The spectra are integrated to obtain yields as a function of rapidity (dN/dy), giving full phase-space (4π) yields. At RHIC energies, a low net-baryon density is observed at mid-rapidity [3], so mesons may be predominantly produced from the decay of the strong color field created initially. At forward rapidities, where primordial baryons are more abundant [4], other production mechanisms, for example associated strangeness production, play a larger role. Therefore, the observed rapidity distributions provide a sensitive test of models describing the space-time evolution of the reaction, such as Landau and Bjorken models [1,2]. In addition, integrated yields are a key input to statistical models of particle production [5,6].BRAHMS consists of two hadron spectrometers, a mid-rapidity arm (MRS) and a forward rapidity arm (FS), as well as a set of detectors for global event characterization [7]. Collision centrality is determined from charged particle multiplicities, measured by sc...

The sensitivity of the Deep Underground Neutrino Experiment (DUNE) to neutrino oscillation is determined, based on a full simulation, reconstruction, and event selection of the far detector and a full simulation and parameterized analysis of the near detector. Detailed uncertainties due to the flux prediction, neutrino interaction model, and detector effects are included. DUNE will resolve the neutrino mass ordering to a precision of 5$$\sigma $$ σ , for all $$\delta _{\mathrm{CP}}$$ δ CP values, after 2 years of running with the nominal detector design and beam configuration. It has the potential to observe charge-parity violation in the neutrino sector to a precision of 3$$\sigma $$ σ (5$$\sigma $$ σ ) after an exposure of 5 (10) years, for 50% of all $$\delta _{\mathrm{CP}}$$ δ CP values. It will also make precise measurements of other parameters governing long-baseline neutrino oscillation, and after an exposure of 15 years will achieve a similar sensitivity to $$\sin ^{2} 2\theta _{13}$$ sin 2 2 θ 13 to current reactor experiments.

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