Refine
Document Type
- Article (8)
- Doctoral Thesis (1)
- Preprint (1)
Has Fulltext
- yes (10)
Is part of the Bibliography
- no (10)
Keywords
- Anti-kaon–nucleon physics (1)
- Baryonic resonances (1)
- Ellenberg indicator value (1)
- Freezeout (1)
- Gap Light Analyzer (1)
- Heavy-ion reactions (1)
- Kaonic nuclei (1)
- Low energy QCD (1)
- Partial wave analysis (1)
- SideLook (1)
Institute
- Physik (7)
- Biowissenschaften (1)
- Informatik und Mathematik (1)
Observation of enhanced subthreshold K+ production in central collisions between heavy nuclei
(1994)
In the very heavy collision system 197Au+197Au the K+ production process was studied as a function of impact parameter at 1 GeV/nucleon, a beam energy well below the free N-N threshold. The K+ multiplicity increases more than linearly with the number of participant nucleons and the K+/ pi + ratio rises significantly when going from peripheral to central collisions. The measured K+ double differential cross section is enhanced by a factor of 6 compared to microscopic transport calculations if secondary processes (Delta N-->K Lambda N and Delta Delta -->K Lambda N) are ignored.
Das Monitoring von Ökosystemeigenschaften leistet einen wichtigen Beitrag zur Renaturierung von Ökosystemen. Dabei ist es entscheidend, nicht nur Vegetationsdaten, sondern auch Standortfaktoren, wie zum Beispiel Licht, direkt zu erfassen. Das Projekt "Dynamisierung der Donauauen zwischen Neuburg und Ingolstadt" (Bayern) wurde mit der Zielsetzung implementiert, das typische Flutungsregime und die damit verbundenen Grundwasserschwankungen eines naturnahen Auwaldes wiederherzustellen. Ein Teilprojekt des darauf abgestimmten Monitoringprogramms konzentriert sich seit 2007 auf die Beobachtung von Vegetationsveränderungen an einem neu angelegten Umgehungsgewässer, die entlang von rechtwinklig zum Gewässer verlaufenden Transekten erfasst werden. Hierbei wurde der Standortfaktor Licht anhand der sogenannten "Wörlein-Skala" abgeschätzt. Das Ziel dieser Arbeit war es, eine quantitative Methode auf der Basis der digitalen Hemisphärenphotographie zu entwickeln, die genauere Ergebnisse als die Schätzung liefert und dabei zeitsparend und flexibel eingesetzt werden kann. Aufgrund der so erhobenen Daten sollten folgende Fragen beantwortet werden: (1) Liefert die Wörlein-Skala im Vergleich zu den Messdaten eine verlässliche Datengrundlage? (2) Stellen Ellenberg-Lichtzeigerwerte eine sinnvolle Alternative zur direkten Messung oder Schätzung des Standortfaktors Licht dar? In einer Vorstudie wurde die Vergleichbarkeit spezieller Kameraaufbauten unter verschiedenen Umweltbedingungen getestet. Die Bearbeitung der digitalen Photographien erfolgte mit dem Programm "SideLook" zur Schwellenwertermittlung und der Modellierungssoftware "Gap Light Analyzer". Die Prüfung der Verlässlichkeit der Wörlein-Skala und der Ellenberg-Zeigerwerte erfolgte anhand von induktiver Statistik. Der Methodenvergleich ergab deutliche Unterschiede in der Erfassung des Standortfaktors Licht im Auwald: Die Wörlein-Skala repräsentierte die aus den Photographien abgeleiteten Messwerte relativ gut, nur die Schätzungen für die schattigeren Bereiche waren weniger gut aufgelöst. Die Ellenberg-Lichtzeigerwerte korrelierten nur schwach mit den Messwerten sowohl bei logarithmischer Korrektur der Deckung, als auch bei Gewichtung entsprechend der Deckung der Pflanzenarten. Zusammenfassend erfüllt die digitale Hemisphärenphotographie die meisten Anforderungen an Messungen des Standortfaktors Licht. Die Wörlein-Skala kann als verlässliche Alternative betrachtet werden, solange ihr logarithmischer Verlauf entsprechend des Weber-Fechner`schen Gesetzes beachtet wird. Der Ellenberg-Zeigerwert eignet sich dagegen weniger zur Erfassung des Standortfaktors Licht in Auwaldgebieten.
The change in allele frequencies within a population over time represents a fundamental process of evolution. By monitoring allele frequencies, we can analyze the effects of natural selection and genetic drift on populations. To efficiently track time-resolved genetic change, large experimental or wild populations can be sequenced as pools of individuals sampled over time using high-throughput genome sequencing (called the Evolve & Resequence approach, E&R). Here, we present a set of experiments using hundreds of natural genotypes of the model plant Arabidopsis thaliana to showcase the power of this approach to study rapid evolution at large scale. First, we validate that sequencing DNA directly extracted from pools of flowers from multiple plants -- organs that are relatively consistent in size and easy to sample -- produces comparable results to other, more expensive state-of-the-art approaches such as sampling and sequencing of individual leaves. Sequencing pools of flowers from 25-50 individuals at ∼40X coverage recovers genome-wide frequencies in diverse populations with accuracy r > 0.95. Secondly, to enable analyses of evolutionary adaptation using E&R approaches of plants in highly replicated environments, we provide open source tools that streamline sequencing data curation and calculate various population genetic statistics two orders of magnitude faster than current software. To directly demonstrate the usefulness of our method, we conducted a two-year outdoor evolution experiment with A. thaliana to show signals of rapid evolution in multiple genomic regions. We demonstrate how these laboratory and computational Pool-seq-based methods can be scaled to study hundreds of populations across many climates.
We present first data on sub-threshold production of Ks0 mesons and Λ hyperons in Au+Au collisions at sNN=2.4 GeV. We observe an universal 〈Apart〉 scaling of hadrons containing strangeness, independent of their corresponding production thresholds. Comparing the yields, their 〈Apart〉 scaling, and the shapes of the rapidity and the pt spectra to state-of-the-art transport model (UrQMD, HSD, IQMD) predictions, we find that none of them can simultaneously describe these observables with reasonable χ2 values.
We investigate identical pion HBT intensity interferometry in central Au+Au collisions at 1.23A GeV. High-statistics π−π− and π+π+ data are measured with HADES at SIS18/GSI. The radius parameters, derived from the correlation function depending on relative momenta in the longitudinally comoving system and parametrized as three-dimensional Gaussian distribution, are studied as function of transverse momentum. A substantial charge-sign difference of the source radii is found, particularly pronounced at low transverse momentum. The extracted source parameters agree well with a smooth extrapolation of the center-of-mass energy dependence established at higher energies, extending the corresponding excitation functions down towards a very low energy.
In March 2019 the HADES experiment recorded 14 billion Ag+Ag collisions at √sNN = 2.55 GeV as a part of the FAIR phase-0 physics program. In this contribution, we present and investigate our capabilities to reconstruct and analyze weakly decaying strange hadrons and hypernuclei emerging from these collisions. The focus is put on measuring the mean lifetimes of these particles.
We present data on charged kaons (K±) and ϕ mesons in Au(1.23A GeV)+Au collisions. It is the first simultaneous measurement of K− and ϕ mesons in central heavy-ion collisions below a kinetic beam energy of 10A GeV. The ϕ/K− multiplicity ratio is found to be surprisingly high with a value of 0.52±0.16 and shows no dependence on the centrality of the collision. Consequently, the different slopes of the K+ and K− transverse-mass spectra can be explained solely by feed-down, which substantially softens the spectra of K− mesons. Hence, in contrast to the commonly adapted argumentation in literature, the different slopes do not necessarily imply diverging freeze-out temperatures of K+ and K− mesons caused by different couplings to baryons.
Partial wave analysis of the reaction p(3.5 GeV) + p → pK +Λ to search for the "ppK−" bound state
(2015)
Employing the Bonn–Gatchina partial wave analysis framework (PWA), we have analyzed HADES data of the reaction p(3.5 GeV) + p → pK +Λ. This reaction might contain information about the kaonic cluster “ppK −” (with quantum numbers J P = 0− and total isospin I = 1/2) via its decay into pΛ. Due to interference effects in our coherent description of the data, a hypothetical KNN (or, specifically “ppK −”) cluster signal need not necessarily show up as a pronounced feature (e.g. a peak) in an invariant mass spectrum like pΛ. Our PWA analysis includes a variety of resonant and non-resonant intermediate states and delivers a good description of our data (various angular distributions and two-hadron invariant mass spectra) without a contribution of a KNN cluster. At a confidence level of CLs = 95% such a cluster cannot contribute more than 2–12% to the total cross section with a pK +Λ final state, which translates into a production cross-section between 0.7 μb and 4.2 μb, respectively. The range of the upper limit depends on the assumed cluster mass, width and production process.
In this letter we report the first multi-differential measurement of correlated pion-proton pairs from 2 billion Au+Au collisions at sNN=2.42 GeV collected with HADES. In this energy regime the population of Δ(1232) resonances plays an important role in the way energy is distributed between intrinsic excitation energy and kinetic energy of the hadrons in the fireball. The triple differential d3N/dMπ±pdpTdy distributions of correlated π±p pairs have been determined by subtracting the πp combinatorial background using an iterative method. The invariant-mass distributions in the Δ(1232) mass region show strong deviations from a Breit-Wigner function with vacuum width and mass. The yield of correlated pion-proton pairs exhibits a complex isospin, rapidity and transverse-momentum dependence. In the invariant mass range 1.1<Minv(GeV/c2)<1.4, the yield is found to be similar for π+p and π−p pairs, and to follow a power law 〈Apart〉α, where 〈Apart〉 is the mean number of participating nucleons. The exponent α depends strongly on the pair transverse momentum (pT) while its pT-integrated and charge-averaged value is α=1.5±0.08st±0.2sy.