Identification and filtering of uncharacteristic noise in the CMS hadron calorimeter

Commissioning studies of the CMS hadron calorimeter have identified sporadic uncharacteristic noise and a small number of malfunctioning calorimeter channels. Algorithms have been developed to identify and address these problems in the data. The methods have been tested on cosmic ray muon data, calorimeter noise data, and single beam data collected with CMS in 2008. The noise rejection algorithms can be applied to LHC collision data at the trigger level or in the offline analysis. The application of the algorithms at the trigger level is shown to remove 90% of noise events with fake missing transverse energy above 100 GeV, which is sufficient for the CMS physics trigger operation. © 2010 IOP Publishing Ltd and SISSA.

Detecção de neutrinos no observatório Pierre Auger

Pós-graduação em Física - IFT

Aspergillus niger beta-Glucosidase Has a Cellulase-like Tadpole Molecular Shape INSIGHTS INTO GLYCOSIDE HYDROLASE FAMILY 3 (GH3) beta-GLUCOSIDASE STRUCTURE AND FUNCTION

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Soft edge of hadron scattering and minijet models for the total and inelastic pp cross sections at LHC and beyond

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Experimental evidence for the sensitivity of the air-shower radio signal to the longitudinal shower development

We observe a correlation between the slope of radio lateral distributions and the mean muon pseudorapidity of 59 individual cosmic-ray-air-shower events. The radio lateral distributions are measured with LOPES, a digital radio interferometer colocated with the multidetector-air-shower array KASCADE-Grande, which includes a muon-tracking detector. The result proves experimentally that radio measurements are sensitive to the longitudinal development of cosmic-ray air showers. This is one of the main prerequisites for using radio arrays for ultra-high-energy particle physics and astrophysics.

Description of atmospheric conditions at the Pierre Auger Observatory using the Global Data Assimilation System (GDAS)

Atmospheric conditions at the site of a cosmic ray observatory must be known for reconstructing observed extensive air showers. The Global Data Assimilation System (GDAS) is a global atmospheric model predicated on meteorological measurements and numerical weather predictions. GDAS provides altitude-dependent profiles of the main state variables of the atmosphere like temperature, pressure, and humidity. The original data and their application to the air shower reconstruction of the Pierre Auger Observatory are described. By comparisons with radiosonde and weather station measurements obtained on-site in Malargue and averaged monthly models, the utility of the GDAS data is shown. (C) 2012 Elsevier B.V. All rights reserved.

A search for point sources of EeV neutrons

A thorough search of the sky exposed at the Pierre Auger Cosmic Ray Observatory reveals no statistically significant excess of events in any small solid angle that would be indicative of a flux of neutral particles from a discrete source. The search covers from -90 degrees to +15 degrees in declination using four different energy ranges above 1 EeV (10(18) eV). The method used in this search is more sensitive to neutrons than to photons. The upper limit on a neutron flux is derived for a dense grid of directions for each of the four energy ranges. These results constrain scenarios for the production of ultrahigh energy cosmic rays in the Galaxy.

Constraints on the origin of cosmics rays above '10 POT. 18' eV from large-scale anisotropy searches in data of the Pierre Auger observatory

A thorough search for large-scale anisotropies in the distribution of arrival directions of cosmic rays detected above '10 POT. 18' eV at the Pierre Auger Observatory is reported. For the first time, these large-scale anisotropy searches are performed as a function of both the right ascension and the declination and expressed in terms of dipole and quadrupole moments.Within the systematic uncertainties, no significant deviation from isotropy is revealed. Upper limits on dipole and quadrupole amplitudes are derived under the hypothesis that any cosmic ray anisotropy is dominated by such moments in this energy range. These upper limits provide constraints on the production of cosmic rays above '10 POT. 18' eV, since they allow us to challenge an origin from stationary galactic sources densely distributed in the galactic disk and emitting predominantly light particles in all directions.

Edelgase in Enstatit-Chondriten

Zusammenfassung - Die vorliegende Dissertation beschreibt die massenspektrometrische Bestimmung der Edelgaskonzentrationen und -isotopenverhältnisse von insgesamt 47 Enstatit-Chondriten (E-Chondriten). E-Chondrite bilden eine Meteoritengruppe, die sich durch einen hohen Reduktionsgrad auszeichnet. Es gibt Hinweise darauf, dass sie im inneren Bereich des Sonnensystems entstanden. Ihre chemischen und mineralogischen Eigenschaften können daher auch Aufschluss über die Genese der terrestrischen Planeten geben. Die Edelgasmessungen hatten im wesentlichen die Berechnung von Bestrahlungsaltern sowie die Untersuchung der getrappten Edelgaskomponenten zum Ziel. Die Bestrahlungsalter der E-Chondrite liegen zwischen 0.5 und 50 Millionen Jahren. Eine zweifelsfreie Aussage über Häufungen in der Altersverteilung, die auf große Impaktereignisse auf dem Mutterkörper hinweisen könnten, lässt sich aufgrund der relativ hohen Unsicherheit der Alter (20 Prozent) nicht treffen.Etwa 10 Prozent der E-Chondrite enthalten signifikante solare Gasanteile. Alle zählen zum nicht-equilibrierten petrologischen Typ 3.In der elementaren Zusammensetzung der getrappten schweren Edelgase fällt auf, dass EH3-Chondrite (H für high iron) vorrangig ein stärker fraktioniertes (planetares), relativ Ar-armes Edelgasmuster aufweisen, während alle übrigen Typen E4-6 von einer sog. subsolaren, relativ Ar-reichen Signatur dominiert werden. Diese Verteilung und Zusammensetzung lassen sich nicht ohne weiteres mit dem Modell zur Entstehung der petrologischen Typen durch Metamorphose, wie es für die gewöhnlichen Chondrite formuliert wurde, erklären.

Measurement of the atmospheric muon charge ratio with the OPERA detector

The atmospheric muon charge ratio, defined as the number of positive over negative charged muons, is an interesting quantity for the study of high energy hadronic interactions in atmosphere and the nature of the primary cosmic rays. The measurement of the charge ratio in the TeV muon energy range allows to study the hadronic interactions in kinematic regions not yet explored at accelerators. The OPERA experiment is a hybrid electronic detector/emulsion apparatus, located in the underground Gran Sasso Laboratory, at an average depth of 3800 meters water equivalent (m.w.e.). OPERA is the first large magnetized detector that can measure the muon charge ratio at the LNGS depth, with a wide acceptance for cosmic ray muons coming from above. In this thesis, the muon charge ratio is measured using the spectrometers of the OPERA detector in the highest energy region. The charge ratio was computed separately for single and for multiple muon events, in order to select different primary cosmic ray samples in energy and composition. The measurement as a function of the surface muon energy is used to infer parameters characterizing the particle production in atmosphere, that will be used to constrain Monte Carlo predictions. Finally, the experimental results are interpreted in terms of cosmic ray and particle physics models.

Anisotrope Kolloide aus flüssigkristallinen Polymeren

In dieser Arbeit wird die Synthese, Charakterisierung und Manipulation anisotroper Kolloide aus flüssigkristallinen Polymeren beschrieben. Um Kolloide verschiedener Größe und aus verschiedenen Polymeren zu erhalten, wurden verschiedene Techniken verwendet. Einerseits wurden Kolloide aus nematischen und smektischen Polymeren mit Durchmessern meist im Bereich von 0,5 bis 3,5 Mikrometern hergestellt. Dazu wurden 16 verschiedene Acrylat- und Methacrylatmonomere synthetisiert und mittels Dispersionspolymerisation polymerisiert. Durch Variation der Polymerisationsbedingungen wurden Kolloide verschiedener Größe und Polydispersität erhalten. Durch Saatpolymerisation konnten zudem die Kugelgrößen bei gleichbleibend geringer Polydispersität erhöht werden. Polarisationsmikroskopie zeigt, dass die meisten Kolloide mit einer Größe zwischen ca. 2 bis 4 Mikrometern eine bipolare Direktorkonfiguration haben. Einige dieser Kolloide wurden mit einer optischen Pinzette mit zirkular polarisiertem Licht eingefangen und rotiert. Zum anderen wurden verschiedene flüssigkristalline Polymere (Polysiloxane, Hauptkettenpolymere und Polyacrylate) durch den Miniemulsionsprozess in Kolloide mit Durchmessern im Bereich von ca. 50 bis 300 nm überführt. Durch Variation der Emulgator- und Polymermenge sowie der Art des Emulgators konnte die Kugelgröße beeinflusst werden. Für die Polysiloxankolloide erfolgte die Aufklärung ihrer inneren Struktur mittels TEM und Kryo-TEM, da durch das Silizium im Polymerrückgrat ohne zusätzliches Anfärben ein Kontrast vorhanden ist. Die TEM-Aufnahmen zeigen deutlich die smektische Schichtstruktur innerhalb der Kolloide aus „verdünnten“ Copolysiloxanen und sind somit der erste direkte Beweis für die Mikrophasenseparation zwischen den Mesogenen und Polysiloxanketten, die bisher basierend auf Röntgenmessungen nur indirekt vorhergesagt wurde. Für die Copolysiloxane mit 2-Ring-Mesogenen wurden zwiebelartige Strukturen und für die Copolysiloxane mit 3-Ring-Mesogenen parallele Schichtstrukturen gefunden. Im ersten Fall folgt die smektische Schichtstruktur der Kugelsymmetrie des Kolloids, im zweiten Fall dominiert die Tendenz der smektischen Schichten, sich parallel anzuordnen.

Tracking, b-tagging and measurement of the b-jet production cross section with the ATLAS detector

The Standard Model of elementary particle physics was developed to describe the fundamental particles which constitute matter and the interactions between them. The Large Hadron Collider (LHC) at CERN in Geneva was built to solve some of the remaining open questions in the Standard Model and to explore physics beyond it, by colliding two proton beams at world-record centre-of-mass energies. The ATLAS experiment is designed to reconstruct particles and their decay products originating from these collisions. The precise reconstruction of particle trajectories plays an important role in the identification of particle jets which originate from bottom quarks (b-tagging). This thesis describes the step-wise commissioning of the ATLAS track reconstruction and b-tagging software and one of the first measurements of the b-jet production cross section in pp collisions at sqrt(s)=7 TeV with the ATLAS detector. The performance of the track reconstruction software was studied in great detail, first using data from cosmic ray showers and then collisions at sqrt(s)=900 GeV and 7 TeV. The good understanding of the track reconstruction software allowed a very early deployment of the b-tagging algorithms. First studies of these algorithms and the measurement of the b-tagging efficiency in the data are presented. They agree well with predictions from Monte Carlo simulations. The b-jet production cross section was measured with the 2010 dataset recorded by the ATLAS detector, employing muons in jets to estimate the fraction of b-jets. The measurement is in good agreement with the Standard Model predictions.

Molecular Dynamics Simulations of the d(TAT) Triple Helix

Molecular dynamics (MD) simulations have been used to study the dynamical and time-averaged characteristics of the DNA triple helix d(T)10âd(A)10âd(T)10. The structures sampled during the trajectory resemble closely the B-type model for the DNA triplex proposed on the basis of NMR data, although there are some subtle differences. Alternative P- and A-type conformations for the triplex, suggested from X-ray experiments, are not predicted to contribute significantly to the structure of the DNA triplex in solution. Comparison with the best available experimental data supports the correctnes of the MD-generated structures. The analysis of the collected data gives a detailed picture of the characteristics of triple-helix DNA. A new and interesting pattern of hydration, specific for triplex DNA, is an important observation. The results suggest that molecular dynamics can be useful for the study of novel nucleic acid structures.