Strangeness production process pp -> nK(+)Sigma(+) within resonance model

We explore production mechanism and final state interaction in the pp -> nK(+)Sigma(+) channel based on the inconsistent experimental data published respectively by COSY-11 and COSY-ANKE. The scattering parameter a > 0 for n Sigma(+) interaction is favoured by large near-threshold cross section within a nonrelativistic parametrization investigation, and a strong n Sigma(+) interaction comparable to pp interaction is also indicated. Based on this analysis we calculate the contribution from resonance Delta*(1920) through pi(+) exchange within resonance model, and the numerical result suggests a rather small near-threshold total cross section, which is consistent with the COSY-ANKE data. With an additional sub-threshold resonance Delta*(1620), the model gives a much better description to the rather large near-threshold total cross section published by COSY-11

Dynamics of strangeness production in heavy-ion collisions near threshold energies

Within the framework of the improved isospin-dependent quantum molecular dynamics (ImIQMD) model, the dynamics of strangeness (K-0,K-+, Lambda, and Sigma(-,0,+)) production in heavy-ion collisions near threshold energies is investigated systematically, with the strange particles considered to be produced mainly by inelastic collisions of baryon-baryon and pion-baryon. Collisions in the region of suprasaturation densities of the dense baryonic matter formed in heavy-ion collisions dominate the yields of strangeness production. Total multiplicities as functions of incident energies and collision centralities are calculated with the Skyrme parameter SLy6. The excitation function of strangeness production is analyzed and also compared with the KaoS data for K+ production in the reactions C-12 + C-12 and Au-197 + Au-197.

Strangeness data with light projectiles from a hydrodynamical point of view

The usual particle emission scenario used in hydrodynamics presupposes that particles instantaneously stop interacting (freeze-out) once they reach some three-dimensional surface. Another formalism has recently been developed where particle emission occurs continuously during the whole expansion of thermalized matter. Here we compare both mechanisms in a simplified hydrodynamical framework and show that they lead to a drastically different interpretation of data.

Strangeness data with heavy projectiles from a hydrodynamical point of view

We compare the results obtained by using the continuous emission model with data from Ph-Ph collisions. We determine the initial conditions necessary to reproduce the strange particle ratios (experiment WA97) and with the obtained results, we study the dependence on particle mass of the inverse slope parameter T. Some particle spectra are also shown.

Can the meson cloud explain the nucleon strangeness?

We use a version of the meson cloud model, including the kaon and the K-* contributions, to estimate the electric and magnetic strange form factors of the nucleon. We compare our results with the recent measurements of the strange quark contribution to parity-violating asymmetries in the forward G0 electron-proton scattering experiment. We conclude that it is very important to determine experimentally the electric and magnetic strange form factors, and not only the combination G(E)(s)+eta G(M)(s), if one does really intend to understand the strangeness of the nucleon.

Confronting particle emission scenarios with strangeness data

We show that a hadron gas model with continuous particle emission instead of freeze-out may solve some of the problems (high values of the freeze-out density and specific net charge) that one encounters in the latter case when studying strange particle ratios such as those from the experiment WA85. This underlines the necessity to understand better particle emission in hydrodynamics to be able to analyze data. It also reopens the possibility of a quark-hadron transition occurring with phase equilibrium instead of explosively.

Strangeness content and structure function of the nucleon in a statistical quark model

The strangeness content of the nucleon is determined from a statistical model using confined quark levels, and is shown to have a good agreement with the corresponding values extracted from experimental data. The quark levels are generated in a Dirac equation that uses a linear confining potential (scalar plus vector). With the requirement that the result for the Gottfried sum rule violation, given by the New Muon Collaboration (NMC), is well reproduced, we also obtain the difference between the structure functions of the proton and neutron, and the corresponding sea quark contributions.

On the kaon' s̄ structure function from the strangeness asymmetry in the nucleon

We propose a phenomenological approach based in the meson cloud model to obtain the strange quark structure function inside a kaon, considering the strange quark asymmetry inside the nucleon. © 2009 American Institute of Physics.

Strangeness Enhancement in Cu-Cu and Au-Au Collisions at root s(NN)=200 GeV

We report new STAR measurements of midrapidity yields for the Lambda, (Lambda) over bar, K-S(0), Xi(-), (Xi) over bar (+), Omega(-), (Omega) over bar (+) particles in Cu + Cu collisions at root s(NN) = 200 GeV, and midrapidity yields for the Lambda, (Lambda) over bar, K-S(0) particles in Au + Au at root s(NN) = 200 GeV. We show that, at a given number of participating nucleons, the production of strange hadrons is higher in Cu + Cu collisions than in Au + Au collisions at the same center-of-mass energy. We find that aspects of the enhancement factors for all particles can be described by a parametrization based on the fraction of participants that undergo multiple collisions.

Untergrundstudien zur Messung der Strangeness-Vektorformfaktoren des Protons durch paritätsverletzende Elektronenstreuung unter Rückwärtswinkeln

Im Rahmen des A4-Experiments werden die Beiträge des Strange-Quarks zu den elektromagnetischen Formfaktoren des Protons gemessen. Solche Seequarkeffekte bei Niederenergieobservablen sind für das Verständnis der Hadronenstruktur wichtig, denn sie stellen eine direkte Manifestation der QCD-Freiheitsgrade im nichtperturbativen Bereich dar.rnrnLinearkombinationen der Strangeness-Vektorformfaktoren des Protons $G_E^s$ und $G_M^s$ sind experimentell über die Messung der paritätsverletzenden Asymmetrie im Wirkungsquerschnitt der elastischen Streuung longitudinal polarisierter Elektronen an unpolarisierten Nukleonen zugänglich. Vor dieser Arbeit hatte die A4-Kollaboration zwei solche Messungen unter Vorwärtsstreuwinkeln bei den Viererimpulsübertägen $Q^2$ von jeweils 0.23 und 0.10 (GeV/c)$^2$ veröffentlicht. Um die Separation von $G_E^s$ und $G_M^s$ beim höheren $Q^2$-Wert zu erhalten, wurde eine Messung unter Rückwärtswinkeln mit der Strahlenergie von 315 MeV durchgeführt.rnrnIm A4-Experiment werden die an einem Flüssigwasserstoff-Target gestreuten Elektronen eines longitudinal polarisierten Strahls mit einem Cherenkov-Kalorimeter einzeln gezählt. Durch die kalorimetrische Energiemessung erfolgt die Trennung der elastischen von den inelastischen Ereignissen. Bei Rückwärtswinkeln wurde dieses Apparat mit einem Szintillator als Elektronentagger erweitert, um den $\gamma$-Untergrund aus dem $\pi^0$-Zerfall zu unterdrücken.rnrnUm die Auswertung dieser Messung zu ermöglichen, wurden im Rahmen dieser Arbeit die gemessenen Energiespektren anhand von ausführlichen Simulationen der Streuprozesse und des Antwortverhaltens der Detektoren untersucht, und eine Methode zur Behandlung des restlichen Untergrunds aus der $\gamma$-Konversionrnvor dem Szintillator entwickelt. Die Simulationergebnisse sind auf dem 5%-Niveau mit den Messungen verträglich, und es wurde bewiesen, dass die Methode der Untergrundbehandlung anwendbar ist.rnrnDie Asymmetriemessung bei Rückwärtswinkeln, die man nach Anwendung der hier erarbeiteten Untergrundbehandlung erhält, wurde für die Separation von $G_E^s$ und $G_M^s$ bei $Q^2$=0.22 (GeV/c)^2 mit der Vorwärtswinkelmessung beim selbenrn$Q^2$ kombiniert. Es ergeben sich die Werte:rnrn$G_M^s$= -0.14 ± 0.11_{exp} ± 0.11_{theo} undrn$G_E^s$= 0.050 ± 0.038_{exp} ± 0.019_{theo}, rnrnwobei die systematische Unsicherheit wegen der Untergrundbehandlung im experimentellen Fehler enthalten ist. Am Ende der Arbeit werden die aus diesen Resultaten folgenden Rückschlüsse auf den Einfluss der Strangeness auf die statischen elektromagnetischen Eigenschaften des Protons diskutiert.rn