998 resultados para Experiment container, ISS, FSL, FEM


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The OPERA experiment aims at the direct observation of ν_mu -> ν_tau oscillations in the CNGS (CERN Neutrinos to Gran Sasso) neutrino beam produced at CERN; since the ν_e contamination in the CNGS beam is low, OPERA will also be able to study the sub-dominant oscillation channel ν_mu -> ν_e. OPERA is a large scale hybrid apparatus divided in two supermodules, each equipped with electronic detectors, an iron spectrometer and a highly segmented ~0.7 kton target section made of Emulsion Cloud Chamber (ECC) units. During my research work in the Bologna Lab. I have taken part to the set-up of the automatic scanning microscopes studying and tuning the scanning system performances and efficiencies with emulsions exposed to a test beam at CERN in 2007. Once the triggered bricks were distributed to the collaboration laboratories, my work was centered on the procedure used for the localization and the reconstruction of neutrino events.

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Das experimentelle Studium der 1966 von Gerasimov, Drell undHearn unabhängig voneinander aufgestellten und als GDH-SummenregelbezeichnetenRelation macht die Vermessung totalerPhotoabsorptionswirkungsquerschnitte von zirkular polarisierten Photonen an longitudinalpolarisierten Nukleonen über einen weiten Energiebereich notwendig. Die im Sommer1998 erfolgte Messung am Mainzer Mikrotron stellt das erste derartigeExperiment mit reellen Photonen zur Messung des GDH-Integrals am Protondar. Die Verwendung eines Frozen-Spin-Butanoltargets, das eingesetzt wurde, umeinen möglichst hohen Proton-Polarisationsgrad zu erreichen, hat diezusätzliche experimentelle Schwierigkeit zur Folge, daß die imButanoltarget enthaltenen Kohlenstoffkerne ebenfalls Reaktionsprodukte liefern, diezusammen mit den am Proton erzeugten nachgewiesen werden.Ziel der Arbeit war die Bestimmung von Wirkungsquerschnittenam freien Proton aus Messungen an einem komplexen Target (CH2) wie esbeim polarisiertenTarget vorliegt. Die hierzu durchgeführten Pilotexperimentedienten neben der Entwicklung von Methoden zur Reaktionsidentifikation auchder Eichung des Detektorsystems. Durch die Reproduktion der schon bekanntenund vermessenen unpolarisierten differentiellen und totalenEin-Pion-Wirkungsquerschnitte am Proton (gamma p -> p pi0 und gamma p -> n pi+), die bis zueiner Photonenergievon etwa 400 MeV den Hauptbeitrag zum GDH-Integralausmachen, konnte gezeigt werden, daß eine Separation der Wasserstoff- vonKohlenstoffereignissen möglich ist. Die notwendigen Techniken hierzu wurden imRahmen dieser Arbeit zu einem allgemein nutzbaren Werkzeug entwickelt.Weiterhin konnte gezeigt werden, daß der vom Kohlenstoffstammende Anteil der Reaktionen keine Helizitätsabhängigkeit besitzt. Unterdieser Voraussetzung reduziert sich die Bestimmung der helizitätsabhängigenWirkungsquerschnittsdifferenz auf eine einfacheDifferenzbildung. Aus den erhaltenen Ergebnissen der intensiven Analyse von Daten, diemit einem unpolarisierten Target erhalten wurden, konnten so schnellerste Resultate für Messungen, die mit dem polarisierten Frozen-Spin-Targetaufgenommen wurden, geliefert werden. Es zeigt sich, daß sich dieseersten Resultate für polarisierte differentielle und totale (gammaN)-Wirkungsquerschnitte im Delta-Bereich in guter Übereinstimmung mit theoretischenAnalysen befinden.

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This thesis is about three major aspects of the identification of top quarks. First comes the understanding of their production mechanism, their decay channels and how to translate theoretical formulae into programs that can simulate such physical processes using Monte Carlo techniques. In particular, the author has been involved in the introduction of the POWHEG generator in the framework of the ATLAS experiment. POWHEG is now fully used as the benchmark program for the simulation of ttbar pairs production and decay, along with MC@NLO and AcerMC: this will be shown in chapter one. The second chapter illustrates the ATLAS detectors and its sub-units, such as calorimeters and muon chambers. It is very important to evaluate their efficiency in order to fully understand what happens during the passage of radiation through the detector and to use this knowledge in the calculation of final quantities such as the ttbar production cross section. The last part of this thesis concerns the evaluation of this quantity deploying the so-called "golden channel" of ttbar decays, yielding one energetic charged lepton, four particle jets and a relevant quantity of missing transverse energy due to the neutrino. The most important systematic errors arising from the various part of the calculation are studied in detail. Jet energy scale, trigger efficiency, Monte Carlo models, reconstruction algorithms and luminosity measurement are examples of what can contribute to the uncertainty about the cross-section.

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The ALICE experiment at the LHC has been designed to cope with the experimental conditions and observables of a Quark Gluon Plasma reaction. One of the main assets of the ALICE experiment with respect to the other LHC experiments is the particle identification. The large Time-Of-Flight (TOF) detector is the main particle identification detector of the ALICE experiment. The overall time resolution, better that 80 ps, allows the particle identification over a large momentum range (up to 2.5 GeV/c for pi/K and 4 GeV/c for K/p). The TOF makes use of the Multi-gap Resistive Plate Chamber (MRPC), a detector with high efficiency, fast response and intrinsic time resoltion better than 40 ps. The TOF detector embeds a highly-segmented trigger system that exploits the fast rise time and the relatively low noise of the MRPC strips, in order to identify several event topologies. This work aims to provide detailed description of the TOF trigger system. The results achieved in the 2009 cosmic-ray run at CERN are presented to show the performances and readiness of TOF trigger system. The proposed trigger configuration for the proton-proton and Pb-Pb beams are detailed as well with estimates of the efficiencies and purity samples.

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Tesi svolta presso l'azienda “Riba composites S.r.l.” con lo scopo di riprogettare una passerella nautica utilizzata in imbarcazioni a vela da competizione, attualmente realizzata mediante formatura in autoclave di tessuti pre-impregnati, per il processo produttivo di Vacuum Assisted Resin Injection (VARI). La formatura in autoclave di tessuti pre-­impregnati è una delle tecnologie più onerose, tra i vari processi produttivi nel settore dei materiali compositi, ma assicura proprietà meccaniche e livelli estetici superlativi. L’obiettivo della Riba Composites è ridurre i costi di produzione per offrire un prodotto dalle proprietà analoghe a un prezzo più competitivo. Nella fase di riprogettazione ci siamo affidati a un software di calcolo agli elementi finiti che simula il processo del VARI, l’applicativo PAM-­RTM, del gruppo ESI. Al fine di ottenere una simulazione quanto più precisa possibile del processo, abbiamo realizzato molteplici prove sperimentali per ricavare i valori di compressibilità e permeabilità dei rinforzi da inserire nel software FEM.

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La misura della luminosità è un obiettivo importante per tutta la fisica del modello standard e per la scoperta di nuova fisica, poiché è legata alla sezione d'urto (σ) e al rate di produzione (R) di un determinato processo dalla relazione L = R*σ. Nell'eserimento ATLAS a LHC è installato un monitor di luminosità dedicato chiamato LUCID (Luminosity measurements Using Cherenkov Integrating Detector). Grazie ai dati acquisiti durante il 2010 la valutazione off-line delle performances del LUCID e l'implementazione di controlli on-line sulla qualità dei dati raccolti è stata possibile. I dati reali sono stati confrontati con i dati Monte Carlo e le simulazioni sono state opportunamente aggiustate per ottimizzare l'accordo tra i due. La calibrazione della luminosità relativa che permette di ottenere una valutazione della luminosità assoluta è stata possibile grazie ai cosiddetti Van der Meer scan, grazie ai quale è stata ottenuta una precisione dell'11%. L'analisi della fisica del decadimento della Z è in tuttora in corso per ottenere tramite il rate a cui avviene il processo una normalizzazione della luminosità con una precisione migliore del 5%.

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Die vorliegende Dissertation beinhaltet Anwendungen der Quantenchemie und methodische Entwicklungen im Bereich der "Coupled-Cluster"-Theorie zu den folgenden Themen: 1.) Die Bestimmung von Geometrieparametern in wasserstoffverbrückten Komplexen mit Pikometer-Genauigkeit durch Kopplung von NMR-Experimenten und quantenchemischen Rechnungen wird an zwei Beispielen dargelegt. 2.) Die hierin auftretenden Unterschiede in Theorie und Experiment werden diskutiert. Hierzu wurde die Schwingungsmittelung des Dipolkopplungstensors implementiert, um Nullpunkt-Effekte betrachten zu können. 3.) Ein weiterer Aspekt der Arbeit behandelt die Strukturaufklärung an diskotischen Flüssigkristallen. Die quantenchemische Modellbildung und das Zusammenspiel mit experimentellen Methoden, vor allem der Festkörper-NMR, wird vorgestellt. 4.) Innerhalb dieser Arbeit wurde mit der Parallelisierung des Quantenchemiepaketes ACESII begonnen. Die grundlegende Strategie und erste Ergebnisse werden vorgestellt. 5.) Zur Skalenreduktion des CCCSD(T)-Verfahrens durch Faktorisierung wurden verschiedene Zerlegungen des Energienenners getestet. Ein sich hieraus ergebendes Verfahren zur Berechnung der CCSD(T)-Energie wurde implementiert. 6.) Die Reaktionsaufklärung der Bildung von HSOH aus di-tert-Butyl-Sulfoxid wird vorgestellt. Dazu wurde die Thermodynamik der Reaktionsschritte mit Methoden der Quantenchemie berechnet.

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In this thesis we describe in detail the Monte Carlo simulation (LVDG4) built to interpret the experimental data collected by LVD and to measure the muon-induced neutron yield in iron and liquid scintillator. A full Monte Carlo simulation, based on the Geant4 (v 9.3) toolkit, has been developed and validation tests have been performed. We used the LVDG4 to determine the active vetoing and the shielding power of LVD. The idea was to evaluate the feasibility to host a dark matter detector in the most internal part, called Core Facility (LVD-CF). The first conclusion is that LVD is a good moderator, but the iron supporting structure produce a great number of neutrons near the core. The second conclusions is that if LVD is used as an active veto for muons, the neutron flux in the LVD-CF is reduced by a factor 50, of the same order of magnitude of the neutron flux in the deepest laboratory of the world, Sudbury. Finally, the muon-induced neutron yield has been measured. In liquid scintillator we found $(3.2 \pm 0.2) \times 10^{-4}$ n/g/cm$^2$, in agreement with previous measurements performed at different depths and with the general trend predicted by theoretical calculations and Monte Carlo simulations. Moreover we present the first measurement, in our knowledge, of the neutron yield in iron: $(1.9 \pm 0.1) \times 10^{-3}$ n/g/cm$^2$. That measurement provides an important check for the MC of neutron production in heavy materials that are often used as shield in low background experiments.

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In the thesis is presented the measurement of the neutrino velocity with the OPERA experiment in the CNGS beam, a muon neutrino beam produced at CERN. The OPERA detector observes muon neutrinos 730 km away from the source. Previous measurements of the neutrino velocity have been performed by other experiments. Since the OPERA experiment aims the direct observation of muon neutrinos oscillations into tau neutrinos, a higher energy beam is employed. This characteristic together with the higher number of interactions in the detector allows for a measurement with a much smaller statistical uncertainty. Moreover, a much more sophisticated timing system (composed by cesium clocks and GPS receivers operating in “common view mode”), and a Fast Waveform Digitizer (installed at CERN and able to measure the internal time structure of the proton pulses used for the CNGS beam), allows for a new measurement with a smaller systematic error. Theoretical models on Lorentz violating effects can be investigated by neutrino velocity measurements with terrestrial beams. The analysis has been carried out with blind method in order to guarantee the internal consistency and the goodness of each calibration measurement. The performed measurement is the most precise one done with a terrestrial neutrino beam, the statistical accuracy achieved by the OPERA measurement is about 10 ns and the systematic error is about 20 ns.

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In this thesis the analysis to reconstruct the transverse momentum p_{t} spectra for pions, kaons and protons identified with the TOF detector of the ALICE experiment in pp Minimum Bias collisions at $\sqrt{s}=7$ TeV was reported. After a detailed description of all the parameters which influence the TOF PID performance (time resolution, calibration, alignment, matching efficiency, time-zero of the event) the method used to identify the particles, the unfolding procedure, was discussed. With this method, thanks also to the excellent TOF performance, the pion and kaon spectra can be reconstructed in the 0.5

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The surprising discovery of the X(3872) resonance by the Belle experiment in 2003, and subsequent confirmation by BaBar, CDF and D0, opened up a new chapter of QCD studies and puzzles. Since then, detailed experimental and theoretical studies have been performed in attempt to determine and explain the proprieties of this state. Since the end of 2009 the world’s largest and highest-energy particle accelerator, the Large Hadron Collider (LHC), started its operations at the CERN laboratories in Geneva. One of the main experiments at LHC is CMS (Compact Muon Solenoid), a general purpose detector projected to address a wide range of physical phenomena, in particular the search of the Higgs boson, the only still unconfirmed element of the Standard Model (SM) of particle interactions and, new physics beyond the SM itself. Even if CMS has been designed to study high energy events, it’s high resolution central tracker and superior muon spectrometer made it an optimal tool to study the X(3872) state. In this thesis are presented the results of a series of study on the X(3872) state performed with the CMS experiment. Already with the first year worth of data, a clear peak for the X(3872) has been identified, and the measurement of the cross section ratio with respect to the Psi(2S) has been performed. With the increased statistic collected during 2011 it has been possible to study, in bins of transverse momentum, the cross section ratio between X(3872) and Psi(2S) and separate their prompt and non-prompt component.

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Die vorliegende Arbeit befasst sich mit der Entwicklung und dem Aufbau eines Experiments zur hochpräzisen Bestimmung des g-Faktors gebundener Elektronen in hochgeladenen Ionen. Der g-Faktor eines Teilchens ist eine dimensionslose Konstante, die die Stärke der Wechselwirkung mit einem magnetischen Feld beschreibt. Im Falle eines an ein hochgeladenes Ion gebundenen Elektrons, dient es als einer der genausten Tests der Quantenelektrodynamik gebundener Zustande (BS-QED). Die Messung wird in einem dreifach Penning-Fallen System durchgeführt und basiert auf dem kontinuierlichen Stern-Gerlach-Effekt. Der erste Teil dieser Arbeit gibt den aktuellen Wissensstand über magnetische Momente wieder. Der hier gewählte experimentelle Aufbau wird begründet. Anschließend werden die experimentellen Anforderungen und die verwendeten Messtechniken erläutert. Das Ladungsbrüten der Ionen - einer der wichtigsten Aufgaben dieser Arbeit - ist dargestellt. Seine Realisierung basiert auf einer Feld-Emissions-Spitzen-Anordnung, die die Messung des Wirkungsquerschnitts für Elektronenstoßionisation ermöglicht. Der letzte Teil der Arbeit widmet sich der Entwicklung und dem Aufbau des Penning-Fallen Systems, sowie der Implementierung des Nachweisprozesses. Gegenwärtig ist der Aufbau zur Erzeugung hochgeladener Ionen und der dazugehörigen Messung des g-Faktors abgeschlossen, einschließlich des Steuerprogramms für die erste Datennahme. Die Ionenerzeugung und das Ladungsbrüten werden die nächsten Schritte sein.

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Among the scientific objectives addressed by the Radio Science Experiment hosted on board the ESA mission BepiColombo is the retrieval of the rotational state of planet Mercury. In fact, the estimation of the obliquity and the librations amplitude were proven to be fundamental for constraining the interior composition of Mercury. This is accomplished by the Mercury Orbiter Radio science Experiment (MORE) via a strict interaction among different payloads thus making the experiment particularly challenging. The underlying idea consists in capturing images of the same landmark on the surface of the planet in different epochs in order to observe a displacement of the identified features with respect to a nominal rotation which allows to estimate the rotational parameters. Observations must be planned accurately in order to obtain image pairs carrying the highest information content for the following estimation process. This is not a trivial task especially in light of the several dynamical constraints involved. Another delicate issue is represented by the pattern matching process between image pairs for which the lowest correlation errors are desired. The research activity was conducted in the frame of the MORE rotation experiment and addressed the design and implementation of an end-to-end simulator of the experiment with the final objective of establishing an optimal science planning of the observations. In the thesis, the implementation of the singular modules forming the simulator is illustrated along with the simulations performed. The results obtained from the preliminary release of the optimization algorithm are finally presented although the software implemented is only at a preliminary release and will be improved and refined in the future also taking into account the developments of the mission.