Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory

The Pierre Auger Collaboration has reported. evidence for anisotropy in the distribution of arrival directions of the cosmic rays with energies E > E(th) = 5.5 x 10(19) eV. These show a correlation with the distribution of nearby extragalactic objects, including an apparent excess around the direction of Centaurus A. If the particles responsible for these excesses at E > E(th) are heavy nuclei with charge Z, the proton component of the sources should lead to excesses in the same regions at energies E/Z. We here report the lack of anisotropies in these directions at energies above E(th)/Z (for illustrative values of Z = 6, 13, 26). If the anisotropies above E(th) are due to nuclei with charge Z, and under reasonable assumptions about the acceleration process, these observations imply stringent constraints on the allowed proton fraction at the lower energies.

Search for first harmonic modulation in the right ascension distribution of cosmic rays detected at the Pierre Auger Observatory

We present the results of searches for dipolar-type anisotropies in different energy ranges above 2.5 x 10(17) eV with the surface detector array of the Pierre Auger Observatory, reporting on both the phase and the amplitude measurements of the first harmonic modulation in the right-ascension distribution. Upper limits on the amplitudes are obtained, which provide the most stringent bounds at present, being below 2% at 99% C.L. for EeV energies. We also compare our results to those of previous experiments as well as with some theoretical expectations. (C) 2011 Elsevier B.V. All rights reserved.

The Pierre Auger Observatory scaler mode for the study of solar activity modulation of galactic cosmic rays

Since data-taking began in January 2004, the Pierre Auger Observatory has been recording the count rates of low energy secondary cosmic ray particles for the self-calibration of the ground detectors of its surface detector array. After correcting for atmospheric effects, modulations of galactic cosmic rays due to solar activity and transient events are observed. Temporal variations related with the activity of the heliosphere can be determined with high accuracy due to the high total count rates. In this study, the available data are presented together with an analysis focused on the observation of Forbush decreases, where a strong correlation with neutron monitor data is found.

The exposure of the hybrid detector of the Pierre Auger Observatory

The Pierre Auger Observatory is a detector for ultra-high energy cosmic rays. It consists of a surface array to measure secondary particles at ground level and a fluorescence detector to measure the development of air showers in the atmosphere above the array. The ""hybrid"" detection mode combines the information from the two subsystems. We describe the determination of the hybrid exposure for events observed by the fluorescence telescopes in coincidence with at least one water-Cherenkov detector of the surface array. A detailed knowledge of the time dependence of the detection operations is crucial for an accurate evaluation of the exposure. We discuss the relevance of monitoring data collected during operations, such as the status of the fluorescence detector, background light and atmospheric conditions, that are used in both simulation and reconstruction. (C) 2010 Elsevier B.V. All rights reserved.

Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter

Data collected by the Pierre Auger Observatory through 31 August 2007 showed evidence for anisotropy in the arrival directions of cosmic rays above the Greisen-Zatsepin-Kuz`min energy threshold, 6 x 10(19) eV. The anisotropy was measured by the fraction of arrival directions that are less than 3.1 degrees from the position of an active galactic nucleus within 75 Mpc (using the Veron-Cetty and Veron 12th catalog). An updated measurement of this fraction is reported here using the arrival directions of cosmic rays recorded above the same energy threshold through 31 December 2009. The number of arrival directions has increased from 27 to 69, allowing a more precise measurement. The correlating fraction is (38(-6)(+7))%, compared with 21% expected for isotropic cosmic rays. This is down from the early estimate of (69-(+11)(13))%. The enlarged set of arrival directions is examined also in relation to other populations of nearby extragalactic objects: galaxies in the 2 Microns All Sky Survey and active galactic nuclei detected in hard X-rays by the Swift Burst Alert Telescope. A celestial region around the position of the radiogalaxy Cen A has the largest excess of arrival directions relative to isotropic expectations. The 2-point autocorrelation function is shown for the enlarged set of arrival directions and compared to the isotropic expectation. (C) 2010 Elsevier B.V. All rights reserved.

The fluorescence detector of the Pierre Auger Observatory

The Pierre Auger Observatory is a hybrid detector for ultra-high energy cosmic rays. It combines a surface array to measure secondary particles at ground level together with a fluorescence detector to measure the development of air showers in the atmosphere above the array. The fluorescence detector comprises 24 large telescopes specialized for measuring the nitrogen fluorescence caused by charged particles of cosmic ray air showers. In this paper we describe the components of the fluorescence detector including its optical system, the design of the camera, the electronics, and the systems for relative and absolute calibration. We also discuss the operation and the monitoring of the detector. Finally, we evaluate the detector performance and precision of shower reconstructions. (C) 2010 Elsevier B.V All rights reserved.

Measurement of the energy spectrum of cosmic rays above 10(18) eV using the Pierre Auger Observatory

We report a measurement of the flux of cosmic rays with unprecedented precision and Statistics using the Pierre Auger Observatory Based on fluorescence observations in coincidence with at least one Surface detector we derive a spectrum for energies above 10(18) eV We also update the previously published energy spectrum obtained with the surface detector array The two spectra are combined addressing the systematic uncertainties and, in particular. the influence of the energy resolution on the spectral shape The spectrum can be described by a broken power law E(-gamma) with index gamma = 3 3 below the ankle which is measured at log(10)(E(ankle)/eV) = 18 6 Above the ankle the spectrum is described by a power law with index 2 6 followed by a flux suppression, above about log(10)(E/eV) = 19 5, detected with high statistical significance (C) 2010 Elsevier B V All rights reserved

A study of the effect of molecular and aerosol conditions in the atmosphere on air fluorescence measurements at the Pierre Auger Observatory

The air fluorescence detector of the Pierre Auger Observatory is designed to perforin calorimetric measurements of extensive air showers created by Cosmic rays of above 10(18) eV. To correct these measurements for the effects introduced by atmospheric fluctuations, the Observatory contains a group Of monitoring instruments to record atmospheric conditions across the detector site, ail area exceeding 3000 km(2). The atmospheric data are used extensively in the reconstruction of air showers, and are particularly important for the correct determination of shower energies and the depths of shower maxima. This paper contains a summary of the molecular and aerosol conditions measured at the Pierre Auger Observatory since the start of regular operations in 2004, and includes a discussion of the impact of these measurements oil air shower reconstructions. Between 10(18) and 10(20) eV, the systematic Uncertainties due to all atmospheric effects increase from 4% to 8% in measurements of shower energy, and 4 g cm(-2) to 8 g cm(-2) in measurements of the shower maximum. (C) 2010 Elsevier B.V. All rights reserved.

Derivações em anéis primos e semiprimos

Dissertacao essencialmente sobre derivacoes em aneis mostra que toda derivacao de jordan num anel primo e livre de 2-torcao e uma derivacao usual. prova que toda derivacao de hasse-schmidt-jordan definida num anel semiprimo e livre de 2-torcao e uma derivacao de hasse-schmidt. finalisa com derivacoes algebricas d definidas num anel primo r (c0m unidade) e com suas respectivas extensoes d* ao anel de quocientes (a direita) de martingale de r denotado por q. e demonstrado entao, uma equivalencia entre as r, q e c-algebricidades de d e d*, onde c denota o centroide estendido de r.

Derivações de ordem superior em anéis primos e semiprimos

Nesta tese estudamos as derivações de ordem superior (DOS) em anéis não-comutativos. Inicialmente, mostramos que toda derivação tripla de Jordan de ordem superior em um anel semiprimo livre de 2-torção é uma DOS. Em particular, toda derivação de Jordan de ordem superior (DJOS) num anel deste tipo é uma DOS. Estendemos também o resultado a ideais de Lie U, provando que se R é um anel primo livre de 2-torção e D é uma DJOS de U em R onde U ct Z(R) é tal que U2E U para todo u E U, então D é uma DOS de U em R. Nestas condições, se U C Z(R), então o resultado não é válido. Estudamos ainda as DOS cujas componentes satisfazem relações de dependência linear sobre R ou Q (o anel de quocientes à direita de M artindale de R). Caracterizamos tais DOS, e mostramos que as relações de dependência linear são preservadas ao estendermos uma DOS de R a Q.

Anéis de fatoração única

Este trabalho tem por objetivo estudar condições necessárias e sufi- cientes sobre um determinado anel R, não necessariamente comutativo, para que suas extensões polinomiais apresentem fatoração única. O estudo de tal propriedade é feito para anéis primos Noetherianos e para anéis primos não necessariamente Noetherianos.

Anéis e módulos distributivos

Este trabalho tem por objetivo apresentar resultados sobre módulos e anéis distributivos. Vamos estudar a classe dos módulos distributivos, algumas de suas caracterizações e propriedades mais importantes. Concluiremos o trabalho com dois teoremas centrais. O primeiro deles trata da relação existente entre domínios distributivos e domínios de cadeia. O segundo teorema nos fornece um resultado importante sobre o radical primo de um anel distributivo à direita satisfazendo as condições de cadeia sobre os anuladores principais à direita.

Co-módulos primos e co-álgebras primas

Seja C uma co-álgebra. Consideremos o anel de convolução C*, que é a álgebra dual de C. Dado um co-módulo à direita (resp. à esquerda) sobre C é possível definir um C*-módulo à esquerda (resp. à direita) racional. Nesta tese, estudamos as noções correspondentes dos conceitos de primos, fortemente primos, semiprimos e fortemente semiprimos, que são encontrados na literatura em [2], [3], [4], [13] e [17], para co-módulos. A noção do conceito de primo é obtida também para co-álgebras. Mostramos que uma co-álgebra C é prima se, e somente se, C é uma co-álgebra simples.

Ideais primos e ideais fechados em anéis de polinômios

Este trabalho tem por objetivo estudar os ideais primos do anel de polinômios R[X], com R um anel primo, não necessariamente comutativo. Para tanto, introduzimos o conceito de ideais principais fechados em R[X], que permite caracterizar os ideais primos como contração de ideais de Q[X] sendo definidos por polinômios mônicos irredutíveis de C[X], onde Q é o anel de quocientes µa direita de Martindale de R e C é o centro de Q, que é um corpo.