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Preliminary results on pion-pion Bose-Einstein correlations in central Pb+Pb collisions measured by the NA49 experiment are presented. Rapidity as well as transverse momentum dependence of the HBT-radii are shown for collisions at 20, 30, 40, 80, and 158 AGeV beam energy. Including results from AGS and RHIC experiments only a weak energy dependence of the radii is observed. Based on hydrodynamical models parameters like lifetime and geometrical radius of the source are derived from the dependence of the radii on transverse momentum.
Event-by-event fluctuations of particle ratios in central Pb + Pb collisions at 20 to 158 AGeV
(2004)
In the vicinity of the QCD phase transition, critical fluctuations have been predicted to lead to non-statistical fluctuations of particle ratios, depending on the nature of the phase transition. Recent results of the NA49 energy scan program show a sharp maximum of the ratio of K+ to Pi+ yields in central Pb+Pb collisions at beam energies of 20-30 AGeV. This observation has been interpreted as an indication of a phase transition at low SPS energies. We present first results on event-by-event fluctuations of the kaon to pion and proton to pion ratios at beam energies close to this maximum.
Results are presented on event-by-event electric charge fluctuations in central Pb+Pb collisions at 20, 30, 40, 80 and 158 AGeV. The observed fluctuations are close to those expected for a gas of pions correlated by global charge conservation only. These fluctuations are considerably larger than those calculated for an ideal gas of deconfined quarks and gluons. The present measurements do not necessarily exclude reduced fluctuations from a quark-gluon plasma because these might be masked by contributions from resonance decays.
System-size dependence of strangeness production in nucleus-nucleus collisions at √sNN = 17.3 GeV
(2005)
Emission of pi, K, phi and Lambda was measured in near-central C+C and Si+Si collisions at 158 AGeV beam energy. Together with earlier data for p+p, S+S and Pb+Pb, the system-size dependence of relative strangeness production in nucleus-nucleus collisions is obtained. Its fast rise and the saturation observed at about 60 participating nucleons can be understood as onset of the formation of coherent partonic subsystems of increasing size. PACS numbers: 25.75.-q
Results are presented on Omega production in central Pb+Pb collisions at 40 and 158 AGeV beam energy. Given are transverse-mass spectra, rapidity distributions, and total yields for the sum Omega+Antiomega at 40 AGeV and for Omega and Antiomega separately at 158 AGeV. The yields are strongly under-predicted by the string-hadronic UrQMD model and are in better agreement with predictions from a hadron gas models. PACS numbers: 25.75.Dw
System size and centrality dependence of the balance function in A + A collisions at √sNN = 17.2 GeV
(2004)
Electric charge correlations were studied for p+p, C+C, Si+Si and centrality selected Pb+Pb collisions at sqrt s_NN = 17.2$ GeV with the NA49 large acceptance detector at the CERN-SPS. In particular, long range pseudo-rapidity correlations of oppositely charged particles were measured using the Balance Function method. The width of the Balance Function decreases with increasing system size and centrality of the reactions. This decrease could be related to an increasing delay of hadronization in central Pb+Pb collisions.
The hadronic final state of central Pb+Pb collisions at 20, 30, 40, 80, and 158 AGeV has been measured by the CERN NA49 collaboration. The mean transverse mass of pions and kaons at midrapidity stays nearly constant in this energy range, whereas at lower energies, at the AGS, a steep increase with beam energy was measured. Compared to p+p collisions as well as to model calculations, anomalies in the energy dependence of pion and kaon production at lower SPS energies are observed. These findings can be explained, assuming that the energy density reached in central A+A collisions at lower SPS energies is sufficient to force the hot and dense nuclear matter into a deconfined phase.
System size dependence of multiplicity fluctuations of charged particles produced in nuclear collisions at 158 A GeV was studied in the NA49 CERN experiment. Results indicate a non-monotonic dependence of the scaled variance of the multiplicity distribution with a maximum for semi-peripheral Pb+Pb interactions with number of projectile participants of about 35. This effect is not observed in a string-hadronic model of nuclear collision HIJING.
The hadronic final state of central Pb+Pb collisions at 20, 30, 40, 80, and 158 AGeV has been measured by the CERN NA49 collaboration. The mean transverse mass of pions and kaons at midrapidity stays nearly constant in this energy range, whereas at lower energies, at the AGS, a steep increase with beam energy was measured. Compared to p+p collisions as well as to model calculations, anomalies in the energy dependence of pion and kaon production at lower SPS energies are observed. These findings can be explained, assuming that the energy density reached in central A+A collisions at lower SPS energies is sufficient to transform the hot and dense nuclear matter into a deconfined phase.
Phase diagram of strongly interacting matter is discussed within the exactly solvable statistical model of the quark-gluon bags. The model predicts two phases of matter: the hadron gas at a low temperature T and baryonic chemical potential muB, and the quark-gluon gas at a high T and/or muB. The nature of the phase transition depends on a form of the bag mass-volume spectrum (its pre-exponential factor), which is expected to change with the muB/T ratio. It is therefore likely that the line of the 1st} order transition at a high muB/T ratio is followed by the line of the 2nd order phase transition at an intermediate muB/T, and then by the lines of "higher order transitions" at a low muB/T.
Im Kapitel 1 "Einleitung" wird aufgezeigt, wie die rasante technologische Entwicklung der Mikroelektronik nicht nur die Mikroskopie vorantreibt, sondern auch anderen, neuen Verfahren, wie z. B. dem Laser Scanning Mikroskop, zum Durchbruch verhilft. Damit verbunden ist ein Bedarf an neuen, geeigneten Messverfahren. Dazu stellt diese Arbeit ein neues, im Rahmen einer linearen Näherung arbeitendes, dreidimensionales Messverfahren vor, und demonstriert es am Beispiel des Lichtmikroskops im Hellfelddurchlichtbetrieb, wobei hier die 3. Dimension durch die Aufnahme einer Fokusserie entsteht. Im Kapitel 2 "Modellbildung" wird zuerst ein detailliertes, physikalisches Modell des experimentellen Aufbaus gebildet, um darauf aufbauend ein dreidimensionales, system-theoretisches Modell anzufertigen, anhand dessen das neue Messverfahren erarbeitet werden kann. Dabei wird auch die Berechnung der dreidimensionalen Übertragungsfunktionen des Lichtmikroskops für die drei Fälle absorbierende Objekte, Phasenobjekte und transparente Selbstleuchter beschrieben. Innerhalb des Kapitels 3 "Messverfahren" werden im Kapitel 3.1 zunächst die bekannten Verfahren skizziert. Anschließend, dies ist der Kern der Arbeit, wird im Kapitel 3.2 das neue Messverfahren beschrieben. Es verwendet als Anregung zweidimensionales Rauschen, hier ein Rauschen um eine Ebene senkrecht zur optischen Achse. Das Verfahren wird zunächst für absorbierende Objekte, anschließend auch für Phasenobjekte ausgearbeitet, und dabei experimentell demonstriert. Von zentraler Beutung ist, dass das neue Messverfahren in der Lage ist, auch die Phase der dreidimensionalen Übertragungsfunktion aus den Bildern der Rauschanregung zu berechnen, falls die Übertragung durch die Aufnahmeeinheit gewisse, häufig bei einem vernachlässigbaren Fehler vorliegende, Symmetrieeigenschaften besitzt. Es werden verschiedene Fälle von Symmetrieeigenschaften berücksichtigt, um unterschiedliche experimentelle Gegebenheiten und die drei Fälle absorbierende Objekte, Phasenobjekte und transparente Selbstleuchter abzudecken. Das Kapitel 4 "Messungen" vergleicht die mit dem neuen Messverfahren, mit einem bekannten Messverfahren und durch Berechnung ermittelten Übertragungseigenschaften auch bei Modifikationen des Strahlengangs durch Einfügen von Zentralblenden in die Pupille des Objektivs und in die Pupille des Kondensors. Die auf unterschiedlichen Wegen ermittelten Übertragungseigenschaften werden miteinander verglichen. Der Vergleich veranschaulicht die Leistungsfähigkeit des neuen Messverfahrens. Das Kapitel 5 "Die Bildgewinnung" stellt verschiedene, mehr oder weniger bekannte Ansätze zur Nutzung des vorgestellten Messverfahrens zusammen, darunter vor allem auch die Wiener-Inversfilterung.
The negative-pion multiplicity is measured for central collisions of 40Ar with KCl at eight energies from 0.36 to 1.8 GeV/nucleon and for 4He on KCl and 40Ar on BaI2 at 977 and 772 MeV/nucleon, respectively. A systematic discrepancy with a cascade-model calculation which fits proton- and pion-nucleus cross sections but omits potential-energy effects is used to derive the energy going into bulk compression of the system. A value of the incompressibility constant of K=240 MeV is extracted in a parabolic form of the nuclear-matter equation of state.
The parities of eleven J=1 levels in 208Pb were determined by nuclear resonance fluorescence scattering of linearly polarized photons. A new 1+ level at Ex=5.846 MeV with Gamma 02 / Gamma =1.2±0.4 eV was found. This level can probably be identified with the theoretically predicted isoscalar 1+ state in 208Pb. All other bound dipole states below 7 MeV with Gamma 02 / Gamma >1.5 eV have negative parity. The 1- assignment to the 4.842-MeV level is of special significance because of previous conflicting results about its parity.
The 16O ( gamma ,p0) reaction has been studied with linearly polarized bremsstrahlung photons in and below the giant E1 resonance. The parity of the absorbed radiation was determined from the observed azimuthal asymmetry of the emitted protons. Combined with unpolarized measurements the polarized results determine the proton decay amplitudes of the M1 resonance at Ex=16.2 MeV in 16O. The shape of the unpolarized 16O ( gamma ,p3) angular distribution in the giant E1 resonance was derived from the measured analyzing power. NUCLEAR REACTIONS 16O( gamma ,p), E=15-25 MeV; measured analyzing power theta =90° linearly polarized bremsstrahlung; 16O dipole levels deduced pi ; 16.2 MeV 1+ resonance deduced p0 decay amplitudes; 16O GEDR deduced p3 angular distribution.
The ultrarelativistic quantum molecular dynamics model (UrQMD) is used to study global observables in central reactions of Au+Au at sqrt[s]=200A GeV at the Relativistic Heavy Ion Collider (RHIC). Strong stopping governed by massive particle production is predicted if secondary interactions are taken into account. The underlying string dynamics and the early hadronic decoupling implies only small transverse expansion rates. However, rescattering with mesons is found to act as a source of pressure leading to additional flow of baryons and kaons, while cooling down pions.
11 262 keV 1+ state in 20Ne
(1983)
The excitation energy of the lowest 1+, T=1 state in 20Ne, which is important for parity nonconservation studies, has been determined in a photon scattering experiment to be 11 262.3 ± 1.9 keV. Values for the gamma -ray branching of this level to the ground state and to the first 2+ level in 20Ne are 84 ± 5% and 16 ± 5%, respectively. NUCLEAR REACTIONS 20Ne( gamma , gamma ), E gamma <18 MeV, bremsstrahlung; measured E gamma , gamma branching. Ne natural targets.
Proton emission in relativistic nuclear collisions is examined for events of low and high multiplicity, corresponding to large and small impact parameters. Peripheral reactions exhibit distributions of protons in agreement with spectator-participant decay modes. Central collisions of equal-size nuclei are dominated by the formation and decay of a fireball system. Central collisions of light projectiles with heavy targets exhibit an enhancement in sideward emission which is predicted by recent hydrodynamical calculations.
Angular distributions for elastic and inelastic transitions in 20Ne + 16O scattering have been measured at E(20Ne)=50 MeV. For the 0+, 2+, and 4+ members of the 20Ne ground-state rotational band, the angular distributions exhibit pronounced backward peaking characteristic of an alpha -cluster exchange mechanism. The analysis of the ground-state transition in the first-order elastic transfer model yields no satisfactory fit although microscopic cluster form factors and full recoil corrections are employed. A coupled channels calculation for the 0+, 2+, and 4+ transitions reveals very strong coupling effects, indicating that the coherent superposition of first-order optical model and distorted-wave Born-approximation amplitudes may not be an adequate model for these reactions. NUCLEAR REACTIONS 16O(20Ne, 16O) and 16O(20Ne, 20Ne), elastic and inelastic transfer; E=50MeV; measured sigma (Ef , theta ); optical model + DWBA, and CCBA analyses.
The elastic alpha scattering to backward angles has been studied for 40,42,44,48Ca between 40.7 and 72.3 MeV. The cross sections for 40Ca are larger than those for the higher isotopes up to the highest energies. They show backward increases that disappear above 50 MeV. The enhancement factor for 40Ca over 42,44Ca varies smoothly with energy. 48Ca does also show a backward cross-section enhancement over 42,44Ca. alpha -cluster rotational bands in the 44Ti compound state, four-nucleon correlations in 40Ca, and the l-dependent optical model are discussed as approaches to understand the anomaly. The rotator model appears to agree qualitatively with the experimental data. It involves rotational bands extending at least up to J=16 in 44Ti.
Back-angle enhancements of elastic alpha -scattering cross sections have been observed for nuclei at the ends of the 1p, 2s-1d, and f7 / 2 shells. Strong reduction of this enhancement occurs if excess neutrons enter the next open major shell. The results are discussed in terms of intermediate alpha structure.
Pion-production cross sections have been measured for the reaction 40Ar+40Ca--> pi ++X at a laboratory energy of 1.05 GeV/nucleon. A maximum in the pi + cross section occurs at mid-rapidity, which is anomalous relative to p+p and p+nucleus reactions and compared to many other heavy-ion reactions. Calculations based on cascade and thermal models fail to fit the data.
Inclusive energy spectra of protons, deuterons, and tritons were measured with a telescope of silicon and germanium detectors with a detection range for proton energies up to 200 MeV. Fifteen sets of data were taken using projectiles ranging from protons to 40Ar on targets from 27Al to 238U at bombarding energies from 240 MeV/nucleon to 2.1 GeV/nucleon. Particular attention was paid to the absolute normalization of the cross sections. For three previously reported reactions, He fragment cross sections have been corrected and are presented. To facilitate a comparison with theory the sum of nucleonic charges emitted as protons plus composite particles was estimated and is presented as a function of fragment energy per nucleon in the interval from 15 to 200 MeV/nucleon. For low-energy fragments at forward angles the protons account for only 25% of the nucleonic charges. The equal mass 40Ar plus Ca systems were examined in the center of mass. Here at 0.4 GeV/nucleon 40Ar plus Ca the proton spectra appear to be nearly isotropic in the center of mass over the region measured. Comparisons of some data with firestreak, cascade, and fluid dynamics models indicate a failure of the first and a fair agreement with the latter two. In addition, associated fast charged particle multiplicities (where the particles had energies larger than 25 MeV/nucleon) and azimuthal correlations were measured with an 80 counter array of plastic scintillators. It was found that the associated multiplicities were a smooth function of the total kinetic energy of the projectile. NUCLEAR REACTIONS U(20Ne,X), E / A=240 MeV/nucleon; U(40Ar,X), Ca(40Ar,X), U(20Ne,X), Au(20Ne,X), Ag(20Ne,X), Al(20Ne,X), U(4He,X), Al(4He,X), E / A=390 MeV/nucleon; U(40Ar,X), Ca(40Ar,X), U(20Ne,X), U(4He,X), U(p,X), E / A=1.04 GeV/nucleon; U(20Ne,X), E / A=2.1 GeV/nucleon; measured sigma (E, theta ), X=p,d,t.
Exclusive pi - and charged-particle production in collisions of Ar+KCl is studied at incident energies from 0.4 to 1.8 GeV/u. Complete disintegration of both nuclei is observed. The correlation between pi - and total charge multiplicity shows no islands of anomalous pion production. For constant numbers of proton participants the pi - multiplicity distributions are Poissons. For central collisions <n pi -> increases smoothly and to first order linearly with the c.m. energy. Disagreement with the firestreak model is found. Pacs numbers: 25.70.Hi, 24.10.Dp
Lambda 's produced in central collisions of 40Ar+KC1 at 1.8-GeV/u incident energy were detected in a streamer chamber by their charged-particle decay. For central collisions with impact parameters b<2.4 fm the Lambda production cross section is 7.6±2.2 mb. A calculation in which Lambda production occurs in the early stage of the collision qualitatively reproduces the results but underestimates the transverse momenta. An average Lambda polarization of -0.10±0.05 is observed. PACS numbers: 25.70 Bc
Pion production and charged-particle multiplicity selection in relativistic nuclear collisions
(1982)
Spectra of positive pions with energies of 15-95 MeV were measured for high energy proton, 4He, 20Ne, and 40Ar bombardments of targets of 27Al, 40Ca, 107,109Ag, 197Au, and 238U. A Si-Ge telescope was used to identify charged pions by dE / dx-E and, in addition, stopped pi + were tagged by the subsequent muon decay. In all, results for 14 target-projectile combinations are presented to study the dependence of pion emission patterns on the bombarding energy (from E / A=0.25 to 2.1 GeV) and on the target and the projectile masses. In addition, associated charged-particle multiplicities were measured in an 80-paddle array of plastic scintillators, and used to make impact parameter selections on the pion-inclusive data. NUCLEAR REACTIONS U(20Ne, pi +), E / A=250 MeV; U(40Ar, pi +), Ca(40Ar, pi +), U(20Ne, pi +), Au(20Ne, pi +), Ag(20Ne, pi +), Al(20Ne, pi +), U(4He, pi +), Al(4He, pi +). E / A=400 MeV; Ca(40Ar, pi +), U(20Ne, pi +), U(4He, pi +), U(p, pi +), E / A=1.05), GeV; U(20Ne, pi +), E / A=2.1 GeV; measured sigma (E, theta ), inclusive and selected on associated charged-particle multiplicity.
Energy spectra and angular distributions have been measured of 3He and 4He fragments emitted from Ag and U targets, bombarded with 2.7-GeV protons, and 1.05-GeV/nucleon alpha particles and 16O ions. All cross sections increase dramatically with projectile mass. No narrow peaks are found in the angular distributions or in the energy spectra.
Double-differential cross sections have been measured for high-energy p, d, t, 3He, and 4He particles emitted from uranium targets irradiated with 20Ne ions at energies of 250, 400, and 2100 MeV/nucleon and 4He ions at 400 MeV/nucleon. By using the shape and yield of the proton energy spectra, the shape and yield of the d, t, 3He, and 4He energy spectra can be deduced at all measured angles for all incident projectile energies by assuming that they are formed by a coalescence of cascade nucleons, using a model analogous to that of Butler and Pearson, and Schwarzschild and Zupancic-caron.
A simple model is proposed for the emission of nucleons with velocities intermediate between those of the target and projectile. In this model, the nucleons which are mutually swept out from the target and projectile form a hot quasiequilibrated fireball which decays as an ideal gas. The overall features of the proton-inclusive spectra from 250- and 400-MeV/nucleon 20Ne ions and 400-MeV/nucleon 4He ions interacting with uranium are fitted without any adjustable parameters.
The energy spectra of protons and light nuclei produced by the interaction of 4He and 20Ne projectiles with Al and U targets have been investigated at incident energies ranging from 0.25 to 2.1 GeV per nucleon. Single fragment inclusive spectra have been obtained at angles between 25° and 150°, in the energy range from 30 to 150 MeV/nucleon. The multiplicity of intermediate and high energy charged particles was determined in coincidence with the measured fragments. In a separate study, fragment spectra were obtained in the evaporation energy range from 12C and 20Ne bombardment of uranium. We observe structureless, exponentially decaying spectra throughout the range of studied fragment masses. There is evidence for two major classes of fragments; one with emission at intermediate temperature from a system moving slowly in the lab frame, and the other with high temperature emission from a system propagating at a velocity intermediate between target and projectile. The high energy proton spectra are fairly well reproduced by a nuclear fireball model based on simple geometrical, kinematical, and statistical assumptions. Light cluster emission is also discussed in the framework of statistical models. NUCLEAR REACTIONS U(20Ne,X), E=250 MeV/nucl.; U(20Ne,X), U(α,X) E=400 MeV/nucl.; U(20Ne,X), Al(20Ne,X), E=2.1 GeV/nucl.; measured σ(E,θ), X=p, d, t, 3He,4He. U(20Ne,X), U(α,X), E=400 MeV/nucl.; U(20Ne,X), E=2.1 GeV/nucl.; measured σ(E, θ), Li to O. U(20Ne,X), U(12C,X), E=2.1 GeV/nucl.; measured σ(E, 90°), 4He to B. Nuclear fireballs, coalescence, thermodynamics of light nuclei production.
Results are presented from a search for the decays D0 -> K min pi plus and D0 bar -> K plus pi min in a sample of 3.8x10^6 central Pb-Pb events collected with a beam energy of 158A GeV by NA49 at the CERN SPS. No signal is observed. An upper limit on D0 production is derived and compared to predictions from several models.
Particle production in central Pb+Pb collisions was studied with the NA49 large acceptance spectrometer at the CERN SPS at beam energies of 20, 30, 40, 80, and 158 GeV per nucleon. A change of the energy dependence is observed around 30A GeV for the yields of pions and strange particles as well as for the shapes of the transverse mass spectra. At present only a reaction scenario with onset of deconfinement is able to reproduce the measurements.
The transverse mass spectra of Omega hyperons and phi mesons measured recently by STAR Collaboration in Au+Au collisions at sqrt(s_NN) = 130 GeV are described within a hydrodynamic model of the quark gluon plasma expansion and hadronization. The flow parameters at the plasma hadronization extracted by fitting these data are used to predict the transverse mass spectra of J/psi and psi' mesons.
We argue that the shape of the system-size dependence of strangeness production in nucleus-nucleus collisions can be understood in a picture that is based on the formation of clusters of overlapping strings. A string percolation model combined with a statistical description of the hadronization yields a quantitative agreement with the data at sqrt s_NN = 17.3 GeV. The model is also applied to RHIC energies.
A steep maximum occurs in the Wroblewski ratio between strange and non-strange quarks created in central nucleus-nucleus collisions, of about A=200, at the lower SPS energy square root s approximately equal to 7 GeV. By analyzing hadronic multiplicities within the grand canonical statistical hadronization model this maximum is shown to occur at a baryochemical potential of about 450 MeV. In comparison, recent QCD lattice calculations at finite baryochemical potential suggest a steep maximum of the light quark susceptibility, to occur at similar mu B, indicative of "critical fluctuation" expected to occur at or near the QCD critical endpoint. This endpoint hat not been firmly pinned down but should occur in the 300 MeV < mu c B < 700 MeV interval. It is argued that central collisions within the low SPS energy range should exhibit a turning point between compression/heating, and expansion/cooling at energy density, temperature and mu B close to the suspected critical point. Whereas from top SPS to RHIC energy the primordial dynamics create a turning point far above in epsilon and T, and far below in mu B. And at lower AGS energies the dynamical trajectory stays below the phase boundary. Thus, the observed sharp strangeness maximum might coincide with the critical square root s at which the dynamics settles at, or near the QCD endpoint.
Strangeness enhancement is discussed as a feature specific to relativistic nuclear collisions which create a fireball of strongly interacting matter at high energy density. At very high energy this is suggested to be partonic matter, but at lower energy it should consist of yet unknown hadronic degrees of freedom. The freeze-out of this high density state to a hadron gas can tell us about properties of fireball matter. The hadron gas at the instant of its formation captures conditions directly at the QCD phase boundary at top SPS and RHIC energy, chiefly the critical temperature and energy density.
Relativistic nucleus-nucleus collisions create a "fireball" of strongly interacting matter at high energy density. At very high energy this is suggested to be partonic matter, but at lower energy it should consist of yet unknown hadronic, perhaps coherent degrees of freedom. The freeze-out of this high density state to a hadron gas can tell us about properties of fireball matter. Date (v1): Thu, 19 Dec 2002 12:52:34 GMT (146kb) Date (revised v2): Thu, 16 Jan 2003 15:11:47 GMT (146kb) Date (revised v3): Wed, 14 May 2003 12:49:35 GMT (146kb)
With new data available from the SPS, at 40 and 80 GeV/A, I review the systematics of bulk hadron multiplicities, with prime focus on strangeness production. The classical concept of strangeness enhancement in central AA collisions is reviewed, in view of the statistical hadronization model which suggests to understand strangeness enhancement to arise chiefly in the transition from the canonical to the grand canonical version of that model. I. e. enhancement results from the fading away of canonical suppression. The model also captures the striking strangeness maximum observed in the vicinity of sqrt s approx 8 GeV. A puzzle remains in the understanding of apparent grand canonical order at the lower SPS, and at AGS energies.
Transverse momentum event-by-event fluctuations are studied within the string-hadronic model of high energy nuclear collisions, LUCIAE. Data on non-statistical pT fluctuations in p+p interactions are reproduced. Fluctuations of similar magnitude are predicted for nucleus-nucleus collisions, in contradiction to the preliminary NA49 results. The introduction of a string clustering mechanism (Firecracker Model) leads to a further, significant increase of pT fluctuations for nucleus-nucleus collisions. Secondary hadronic interactions, as implemented in LUCIAE, cause only a small reduction of pT fluctuations.
Hadronic yields and yield ratios observed in Pb+Pb collisions at the SPS energy of 158 GeV per nucleon are known to resemble a thermal equilibrium population at T=180 +/- 10 MeV, also observed in elementary e+ + e- to hadron data at LEP. We argue that this is the universal consequence of the QCD parton to hadron phase transition populating the maximum entropy state. This state is shown to survive the hadronic rescattering and expansion phase, freezing in right after hadronization due to the very rapid longitudinal and transverse expansion that is inferred from Bose-Einstein pion correlation analysis of central Pb+Pb collisions.
A selection of recent data referring to Pb+Pb collisions at the SPS CERN energy of 158 GeV per nucleon is presented which might describe the state of highly excited strongly interacting matter both above and below the deconfinement to hadronization (phase) transition predicted by lattice QCD. A tentative picture emerges in which a partonic state is indeed formed in central Pb+Pb collisions which hadronizes at about T = 185 MeV, and expands its volume more than tenfold, cooling to about 120 MeV before hadronic collisions cease. We suggest further that all SPS collisions, from central S+S onward, reach that partonic phase, the maximum energy density increasing with more massive collision systems.
We investigate the sensitivity of several observables to the density dependence of the symmetry potential within the microscopic transport model UrQMD (ultrarelativistic quantum molecular dynamics model). The same systems are used to probe the symmetry potential at both low and high densities. The influence of the symmetry potentials on the yields of pi-, pi+, the pi-/pi+ ratio, the n/p ratio of free nucleons and the t/3He ratio are studied for neutron-rich heavy ion collisions (208Pb+208Pb, 132Sn+124Sn, 96Zr+96Zr) at E_b=0.4A GeV. We find that these multiple probes provides comprehensive information on the density dependence of the symmetry potential.
Diese Arbeit befaßt sich mit der Untersuchung des Emissionsverhaltens der K+ Mesonen in Au + Au Stößen bei 1AGeV. Das Experiment wurde mit dem Kaonen-Spektrometer KaoS am Schwerionensynchrotron SIS der Gesellschaft für Schwerionenforschung GSI durchgeführt. In zahlreichen Untersuchungen relativistischer Schwerionenstöße wurde eine kollektive Bewegung der Nukleonen beobachtet, die als Fluß bezeichnet wird. In nichtzentralen Stößen wurde u. a. ein gerichteter Seitwärtsfluß der Nukleonen und Pionen in die Reaktionsebene und ein elliptischer Fluß senkrecht zur Reaktionsebene gefunden. Der Nukleonenfluß wird als hydrodynamischer Effekt aufgrund des Drucks in der Reaktionszone interpretiert, während der Fluß der Pionen als Folge der Endzustandswechselwirkung verstanden wird. In dieser Arbeit wurde die Untersuchung des Flußphänomens auf die positiv geladenen Kaonen erweitert. Die Kaonen, die ein seltsames Quark enthalten, stellen eine besonders geeignete Sonde der dichten Reaktionszone dar. Wegen der großen mittleren freien Wegläange sollten die Kaonen fast ungestört nach außen emittiert werden. Zur Untersuchung dieser Fragestellung wurden die spektralen Energieverteilungen und die azimutalen Winkelverteilungen studiert. Um diese in Abhängigkeit von der Zentralität der Schwerionenreaktion zu untersuchen, wurden Stoßparameter und Anzahl der partizipierenden Nukleonen experimentell bestimmt. Dazu wurden die mit dem Großwinkel-Hodoskop bestimmte Teilchenmultiplizität und die mit dem Kleinwinkel-Hodoskop bestimmte Ladungssumme der Projektilspektatoren benutzt. Der Nachweis der Projektilspektatoren mit dem Kleinwinkel-Hodoskop erlaubt ferner, für jedes Ereignis die Reaktionsebene einer Schwerionenreaktion zu bestimmen. Der Emissionswinkel der positiv geladenen Kaonen konnte dann in Bezug auf die Reaktionsebene untersucht werden. Die Energiespektren der Kaonen, die bei Theta CM ~ 90° und Theta QCM ~ 130° in zentralen Stößen gemessen wurden, haben einen Steigungsparameter (Temperatur) von etwa 87MeV. Die transversalen kinetischen Energiespektren bei vier verschiedenen Rapiditätsintervallen in zentralen Stößen haben einen Steigungsparameter von etwa 90MeV und keine Abweichung von einem thermischen Verhalten innerhalb der Meßgenauigkeit. Die Ausbeuten sind dagegen unterschiedlich. Bei R¨uckw ¨ artswinkel bzw. bei Targetrapidität wurde ein fast doppelt so großer Wirkungsquerschnitt wie bei Schwerpunktrapidität gemessen. Die polare Winkelverteilung der positiv geladenen Kaonen ist also nicht isotrop. In dieser Arbeit konnte zum ersten Mal der elliptische Fluß der positiv geladenen Kaonen nachgewiesen werden: K+ Mesonen werden bevorzugt senkrecht zur Reaktionsebene emittiert. Die azimutale Anisotropie ist am stärksten für periphere und semi-zentrale Stöße und im Bereich der Schwerpunktrapidität. Im Gegensatz zu den Pionen zeigt die Stärke der Anisotropie keine Abhängigkeit vom Transversalimpuls. Während im Falle der Pionen die azimutale Anisotropie auf die Abschattung durch die Spektatoren zurückgeführt wird, kann dieser Effekt die Kaonendaten nicht erklären, da die K+ Mesonen eine große mittlere freie Weglänge in Kernmaterie besitzen. Mikroskopische Transportmodellrechnungen wie RBUU und QMD können den elliptischen Fluß der Kaonen nur unter Berücksichtigung des Kaon-Nukleon-Potentials im nuklearen Medium wiedergeben [Li97, Wan98a]. Als ein anderer experimenteller Hinweis auf das KN-Potential im Medium wurde das Verschwinden des gerichteten Seitwärtsflusses der Kaonen vorhergesagt [Li95a]. Die Analyse der experimentellen Daten in einem Rapiditätsintervall von y/yStrahl = 0:2 ~ 0:8 zeigt keine in die Reaktionsebene gerichtete Flußkomponente.
We present a detailed study of chemical freeze-out in nucleus-nucleus collisions at beam energies of 11.6, 30, 40, 80 and 158A GeV. By analyzing hadronic multiplicities within the statistical hadronization approach, we have studied the chemical equilibration of the system as a function of center of mass energy and of the parameters of the source. Additionally, we have tested and compared different versions of the statistical model, with special emphasis on possible explanations of the observed strangeness hadronic phase space under-saturation.
Cancer has become one of the most fatal diseases. The Heidelberg Heavy Ion Cancer Therapy (HICAT) has the potential to become an important and efficient treatment method because of its excellent “Bragg peak” characteristics and on-line irradiation control by the PET diagnostics. The dedicated Heidelberg Heavy Ion Cancer Therapy Project includes two ECR ion sources, a RF linear injector, a synchrotron and three treatment rooms. It will deliver 4*10 high 10 protons, or 1*10 high 10 He, or 1*10 high 9 Carbons, or 5*10 high 8 Oxygens per synchrotron cycle with the beam energy 50-430AMeV for the treatments. The RF linear injector consists of a 400AkeV RFQ and of a very compact 7AMeV IH-DTL accelerator operated at 216.816MHz. The development of the IH-DTL within the HICAT project is a great challenge with respect to the present state of the DTL art because of the following reasons: • The highest operating frequency (216.816MHz) of all IH-DTL cavities; • Extremely large cavity length to diameter ratio of about 11; • IH-DTL with three internal triplets; • The highest effective voltage gain per meter (5.5MV/m); • Very short MEBT design for the beam matching. The following achievements have been reached during the development of the IH-DTL injector for HICAT : The KONUS beam dynamics design with LORASR code fulfills the beam requirement of the HICAT synchrotron at the injection point. The simulations for the IH-DTL injector have been performed not only with a homogeneous input beam, but also with the actual particle distribution from the exit of the HICAT RFQ accelerator as delivered by the PARMTEQ code. The output longitudinal normalized emittance for 95% of all particles is 2.00AkeVns, the emittance growth is less than 24%, while the X-X’ and Y-Y’ normalized emittance are 0.77mmmrad and 0.62mmmrad, respectively. The emittance growth in X-X’ is less than 18%, and the emittance growth in Y-Y’ is less than 5%. Based on the transverse envelopes of the transported particles, the redesign of the buncher drift tubes at the RFQ high energy end has been made to get a higher transit time factor for this novel RFQ internal buncher. An optimized effective buncher gap voltage of 45.4KV has been calculated to deliver a minimized longitudinal beam emittance, while the influence of the effective buncher voltage on the transverse emittance can be neglected. Six different tuning concepts were investigated in detail while tuning the 1:2 scaled HICAT IH model cavity. ‘Volume Tuning’ by a variation of the cavity cross sectional area can compensate the unbalanced capacitance distribution in case of an extreme beta-lambda-variation along an IH cavity. ‘Additional Capacitance Plates’ or copper sheets clamped on drift tube stems are a fast way for checking the tuning sensitivity, but they will be replaced by massive copper blocks mounted on the drift tube girders finally. ‘Lens Coupling’ is an important tuning to stabilize the operation mode and to increase or decrease the coupling between neighboring sections. ‘Tube Tuning’ is the fine tuning concept and also the standard tuning method to reach the needed field distributions as well as the gap voltage distributions. ‘Undercut Tuning’ is a very sensitive tuning for the end sections and with respect to the voltage distribution balance along the structure. The different types of ‘plungers’ in the 3rd and 4th sections have different effects on the resonance frequency and on the field distribution. The different triplet stems and the geometry of the cavity end have been also investigated to reach the design field and voltage distributions. Finally, the needed uniform field distribution along the IH-DTL cavity and the corresponding effective voltage distribution were realized, the remaining maximum gap voltage difference was less than 5% for the model cavity. The several important higher order modes were also measured. The RF tuning of the IH-DTL model cavity delivers the final geometry parameters of the IH-DTL power cavity. A rectangular cavity cross section was adopted for the first time for this IH-DTL cavity. This eases the realization of the volume tuning concept in the 1st and 2nd sections. Lens coupling determines the final distance between the triplet and the girder. The triplets are mounted on the lower cavity half shell. The Microwave Studio simulations have been carried out not only for the HICAT model cavity, but also for the final geometry of the IH-DTL power cavity. The field distribution for the operation mode H110 fits to the model cavity measurement as well as the Higher Order Modes. The simulations prove the IH-DTL geometrical design. On the other hand, the precision of one simulation with 2.3 million mesh points for full cross section area and the CPU time more than 15hours on a DELL PC with Intel Pentium 4 of 2.4GHz and 2.096GRAM were exploited to their limit when calculating the real parameters for the two final machining iterations during production. The shunt impedance of the IH-DTL power cavity is estimated by comparison with the existing tanks to about 195.8MOmega/m, which fits to the simulation result of 200.3MOmega/m with reducing the conductivity to the 5.0*10 high 7 Omega-1m-1. The effective shunt impedance is 153 MOmega/m. The needed RF power is 755kW. The expected quality factor of the IH-DTL cavity is about 15600. The IH-DTL power cavity tuning measurements before cavity copper plating have been performed. The results are within the specifications. There is no doubt that the needed accuracy of the voltage distribution will be reached with the foreseen fine tuning concepts in the last steps.
HADES ist ein hochauflösendes Dielektronenspektrometer, welches derzeit an der GSI in Darmstadt aufgebaut wird. Ziel ist die Messung von Leptonenpaaren, die in schwerioneninduzierten Reaktionen entstehen. Die invariante Masse der Leptonenpaare soll mit einer Genauigkeit von ~ 1% bestimmt werden. Das HADES-Detektorsystem verwendet Vieldraht-Proportionalkammern zur Rekonstruktion der Teilchenspuren. Aus diesen werden in Verbindung mit der Feldinformation des supraleitenden Magneten die Teilchenimpulse gewonnen, welche wiederum in die invariante Masse eingehen. Über die Driftzeit1 werden die genauen Durchstoßpunkte der Teilchenbahnen durch die verschiedenen Ebenen der Driftkammern erhalten. Dazu ist es erforderlich, die Driftgeschwindigkeit der Elektronen im verwendeten Zählgas zu kennen. Änderungen im Mischungsverhältnis des Zählgases (Helium und Isobutan), aber auch Verunreinigungen des Gases (H2O) können die Driftgeschwindigkeit beeinträchtigen. Verunreinigungen (O2) können weiterhin die Effizienz der Driftkammern verschlechtern. Ziel war deshalb der Aufbau eines Monitorsystems, welches auf Änderungen der Gasmischung und auf eventuelle Kontaminationen (im wesentlichen O2 und H2O) sensitiv ist. Zu diesem Zweck wurde ein Driftgeschwindigkeitsmonitor getestet. Er erlaubt eine Messung der Driftgeschwindigkeit mit einer Genauigkeit von bis zu 0,1% (sigma), allerdings bei anderen elektrischen Feldstärken als in den HADES Driftkammern. Während der einwöchigen Strahlzeit im Mai 2000 wurde die Driftgeschwindigkeit mit dem Prototypen des Driftgeschwindigkeitsmonitors gemessen. Die druckkorrigierte Driftgeschwindigkeit erlaubt Rückschlüsse auf die Gasqualität. Die Messungen ergaben, daß die Ortsauflösung in den HADES Driftkammern nicht von Driftgeschwindigkeitsschwankungen dominiert wird. Eine Extrapolation der Meßergebnisse auf die in den HADES Driftkammern vorherrschenden Feldstärkeverhältnisse ist möglich. Eine relative Signalhöhenmessung ist sensitiv auf den Sauerstoffgehalt des Zählgases bis in den ppm-Bereich. Zwei endgültige Versionen des Driftgeschwindigkeitsmonitors wurden aufgebaut und in das HADES Detektorsystem integriert. Je ein Driftgeschwindigkeitsmonitor wurde am Gasein- und am Gasausfluß aufgestellt, um die Driftgeschwindigkeit dort zu messen und Vergleiche zwischen Frischgas und aus den Kammern ausströmendem ”alten“ Gas zuzulassen. Die Auslese und Datenanalyse des Monitorsystems wurde automatisiert.
Fluctuations and NA49
(2005)
A systematic analysis of data on strangeness and pion production in nucleon–nucleon and central nucleus–nucleus collisions is presented. It is shown that at all collision energies the pion/baryon and strangeness/pion ratios indicate saturation with the size of the colliding nuclei. The energy dependence of the saturation level suggests that the transition to the Quark Gluon Plasma occurs between 15 A·GeV/c (BNL AGS) and 160 A·GeV/c (CERN SPS) collision energies. The experimental results interpreted in the framework of a statistical approach show that the effective number of degrees of freedom increases in the course of the phase transition and that the plasma created at CERN SPS energies may have a temperature of about 280 MeV (energy density ~ 10 GeV/fm exp-3). The presence of the phase transition can lead to the non–monotonic collision energy dependence of the strangeness/pion ratio. After an initial increase the ratio should drop to the characteristic value for the QGP. Above the transition region the ratio is expected to be collision energy independent. Experimental studies of central Pb+Pb collisions in the energy range 20–160 A·GeV/c are urgently needed in order to localize the threshold energy, and study the properties of the QCD phase transition.
We argue that the measurement of open charm gives a unique opportunity to test the validity of pQCD-based and statistical models of nucleus-nucleus collisions at high energies. We show that various approaches used to estimate D-meson multiplicity in central Pb+Pb collisions at 158 A GeV give predictions which differ by more than a factor of 100. Finally we demonstrate that decisive experimental results concerning the open charm yield in A+A collisions can be obtained using data of the NA49 experiment at the CERN SPS.