Underground Neutrino Detectors for Particle and Astroparticle Science: the Giant Liquid Argon Charge Imaging ExpeRiment (GLACIER)

The current focus of the CERN program is the Large Hadron Collider (LHC), however, CERN is engaged in long baseline neutrino physics with the CNGS project and supports T2K as recognized CERN RE13, and for good reasons: a number of observed phenomena in high-energy physics and cosmology lack their resolution within the Standard Model of particle physics; these puzzles include the origin of neutrino masses, CP-violation in the leptonic sector, and baryon asymmetry of the Universe. They will only partially be addressed at LHC. A positive measurement of $\sin^22\theta_{13}>0.01$ would certainly give a tremendous boost to neutrino physics by opening the possibility to study CP violation in the lepton sector and the determination of the neutrino mass hierarchy with upgraded conventional super-beams. These experiments (so called ``Phase II'') require, in addition to an upgraded beam power, next generation very massive neutrino detectors with excellent energy resolution and high detection efficiency in a wide neutrino energy range, to cover 1st and 2nd oscillation maxima, and excellent particle identification and $\pi^0$ background suppression. Two generations of large water Cherenkov detectors at Kamioka (Kamiokande and Super-Kamiokande) have been extremely successful. And there are good reasons to consider a third generation water Cherenkov detector with an order of magnitude larger mass than Super-Kamiokande for both non-accelerator (proton decay, supernovae, ...) and accelerator-based physics. On the other hand, a very massive underground liquid Argon detector of about 100 kton could represent a credible alternative for the precision measurements of ``Phase II'' and aim at significantly new results in neutrino astroparticle and non-accelerator-based particle physics (e.g. proton decay).Comment: 31 pages, 14 figure

Agrofloresta para agricultura familiar.

bitstream/CENARGEN/23823/1/ct016.pd

Riscos geotécnicos e vulnerabilidades: aplicação de grade regular para representação espacial da população na zona costeira.

Considerando o contexto de riscos e vulnerabilidades (UNISDR, 2004; 2013; BRASIL/PNPDC, 2012; IPCC, 2012) e de mudanças climáticas (BRASIL/PNMC, 2009; IPCC, 2007; 2014) no âmbito da gestão ou de políticas públicas, caracterizar as situações de riscos e vulnerabilidades nas zonas costeiras tem sido fundamental para as agendas científicas relacionadas à temática das dimensões humanas das mudanças climáticas e ambientais. Nesse sentido que esse trabalho buscou, mais do que caracterizar essas situações, identificar possíveis padrões no perfil socioeconômico da população que influenciam sua situação de vulnerabilidade, trazendo também ao debate uma reflexão sobre as limitações dos métodos propostos para a análise da vulnerabilidade, que muitas vezes (ou quase sempre), é apenas tangencial (MARANDOLA Jr., 2009). Por meio de uma análise geoespacial, buscou-se identificar quais são os principais elementos indicativos de vulnerabilidade na zona costeira de São Paulo, por meio da integração de dois conjuntos de dados organizados em um Sistema de Informações Geográficas (SIG): riscos geotécnicos sobrepostos em uma grade regular de células de tamanho de 250 m para as áreas urbanas e de 1000 m para áreas rurais (proposta por BUENO, 2014 ? em prep.; BUENO; DAGNINO, 2011). As variáveis do meio físico consistiram em: (a) riscos geotécnicos associados com processos geológicos e hidrológicos ? escorregamentos, inundação e recalques ou subsidência do solo; (b) declividade; (c) altitude e modelo digital de elevação e variáveis. As variáveis sociodemográficas foram: (d) número de pessoas (moradores); (e) gênero (pessoas responsáveis pelo domicílio de sexo masculino e feminino); (f) renda; (g) idade; (h) raça ou cor e (i) alfabetização, todas agregadas por grades regulares ou células como unidade de análise

Matter profile effect in neutrino factory

We point out that the matter profile effect --- the effect of matter density fluctuation on the baseline --- is very important to estimate the parameters in a neutrino factory with a very long baseline. To make it clear, we propose the method of the Fourier series expansion of the matter profile. By using this method, we can take account of both the matter profile effect and its ambiguity. For very long baseline experiment, such as L=7332km, in the analysis of the oscillation phenomena we need to introduce a new parameter $a_{1}$--- the Fourier coefficient of the matter profile --- as a theoretical parameter to deal with the matter profile effects.Comment: 21 pages, 15 figure

Testing whether muon neutrino flavor mixing is maximal

The small difference between the survival probabilities of muon neutrino and antineutrino beams, traveling through earth matter in a long baseline experiment such as MINOS, is shown to be an important measure of any possible deviation from maximality in the flavor mixing of those states.Comment: Some revision has been made in the experimental discussions with two new figures replacing the old ones and a clarification of the accuracy of the perturbative result has been included. This version will be published in Physical Review Letters. Title changed as asked by the editors of Physical Review Letter

Transport parameters from AMS-02 F/Si data and fluorine source abundance

The AMS-02 collaboration recently released cosmic-ray F/Si data of unprecedented accuracy. CR F is predominantly produced by fragmentation of heavier progenitors, while Si is mostly accelerated at source. This ratio is thus maximally sensitive to CR propagation. We study the compatibility of the transport parameters derived from the F/Si ratio with those obtained from the lighter Li/C, Be/C, and B/C ratios. We also inspect the CR source abundance of F, one of the few elements with a high first ionisation potential but only moderately volatile, and a potentially key element to study the acceleration mechanism of CRs. We use the 1D diffusion model implemented in the USINE code and perform $\chi^2$ analyses accounting for several systematic effects (energy correlations in data, nuclear cross sections and solar modulation uncertainties). We also take advantage of the EXFOR nuclear database to update the F production cross sections for its most important progenitors (identified to be 56Fe, 32S, 28Si, 27Al, 24Mg, 22Ne, and 20Ne). The transport parameters obtained from AMS-02 F/Si data are compatible with those obtained from AMS-02 (Li,Be,B)/C data. The combined fit of all these ratios leads to a $\chi^2/dof\approx1.1$, with $\lesssim 10\%$ adjustments of the B and F production cross sections (the latter are based on very few nuclear data points, and would strongly benefit from new measurements). The F/Si ratio is compatible with a pure secondary origin of F, with a best-fit relative source abundance 19F/28Si$_{CRS}\sim 10^{-3}$ and an upper limit of $\sim 5\times 10^{-3}$. Unfortunately, this limit is not sufficient to test global acceleration models of CR nuclei, for which values at the level of $\sim 10^{-4}$ are required. Such levels could be attained with F/Si data of a few percent accuracy at a few tens of TV, possibly within reach of the next generation of CR experiments.Comment: 15 pages, 13 figures, 3 table (1 appendix). Submitted to A&

On the bicrossproduct structures for the Uλ(isoω2...ωN(N)){\cal U}_\lambda(iso_{\omega_2... \omega_N}(N)) family of algebras

It is shown that the family of deformed algebras ${\cal U}_\lambda(iso_{\omega_2... \omega_N}(N))$ has a different bicrossproduct structure for each $\omega_a=0$ in analogy to the undeformed case.Comment: Latex2e file. 14 page

Agenda de transferência de tecnologia: promovendo o desenvolvimento local e regional.

A implantação da Agenda de TT evidencia-se como um mecanismo estratégico e inovador para disponibilizar conhecimentos e tecnologias gerados pela pesquisa aos diversos segmentos da sociedade, contribuindo para o desenvolvimento do setor agropecuário e para a melhoria da qualidade de vida da população brasileira. Além disso, na medida em que incentiva o estabelecimento de alianças estratégicas, a Agenda de TT representa um catalisador do processo de estruturação de Sistemas Locais e/ou Regionais de Inovação

Neutrino physics at accelerators

Present and future neutrino experiments at accelerators are mainly concerned with understanding the neutrino oscillation phenomenon and its implications. Here a brief account of neutrino oscillations is given together with a description of the supporting data. Some current and planned accelerator neutrino experiments are also explained.Comment: 23 pages, 24 figures. Talk given at the Corfu Summer Institute on Elementary Particle Physics 200

The rigidity dependence of galactic cosmic-ray fluxes and its connection with the diffusion coefficient

Thanks to tremendous experimental efforts, galactic cosmic-ray fluxes are being measured up to the unprecedented per cent precision level. The logarithmic slope of these fluxes is a crucial quantity that promises us information on the diffusion properties and the primary or secondary nature of the different species. However, these measured slopes are sometimes interpreted in the pure diffusive regime, guiding to misleading conclusions. In this paper, we have studied the propagation of galactic cosmic rays by computing the fluxes of species between H and Fe using the USINE code and considering all the relevant physical processes and an updated set of cross-section data. We show that the slope of the well-studied secondary-to-primary B/C ratio is distinctly different from the diffusion coefficient slope, by an offset of about 0.2 in the rigidity range in which the AMS-02 data reach their best precision (several tens of GV). Furthermore, we have demonstrated that none of the species from H to Fe follows the expectations of the pure-diffusive regime. We argue that these differences arise from propagation processes such as fragmentation, convection, and reacceleration, which cannot be neglected. On this basis, we also provide predictions for the spectral slope of elemental fluxes not yet analysed by the AMS collaboration