17,673 research outputs found
Effect of the Canting of Local Anisotropy Axes on Ground-State Properties of a Ferrimagnetic Chain with Regularly Alternating Ising and Heisenberg Spins
The effect of the canting of local anisotropy axes on the ground-state phase
diagram and magnetization of a ferrimagnetic chain with regularly alternating
Ising and Heisenberg spins is exactly examined in an arbitrarily oriented
magnetic field. It is shown that individual contributions of Ising and
Heisenberg spins to the total magnetization basically depend on the spatial
orientation of the magnetic field and the canting angle between two different
local anisotropy axes of the Ising spins.Comment: 3 pages, 3 figure
H\"older mean applied to Anderson localization
The phase diagram of correlated, disordered electron systems is calculated
within dynamical mean-field theory using the H\"older mean local density of
states. A critical disorder strength is determined in the
Anderson-Falicov-Kimball model and the arithmetically and the geometrically
averages are found to be just particular means used respectively to detect or
not the Anderson localization. Correlated metal, Mott insulator and Anderson
insulator phases, as well as coexistence and crossover regimes are analyzed in
this new perspective.Comment: 6 pages, 6 figures: Phys. Rev. B 76, 035111 (2007
Mercado e comercialização na ovinocultura de corte no Brasil.
Resumo: O objetivo deste artigo é apresentar os dados relativos ao mercado e à comercialização da carne ovina no Brasil. Especificamente destacam-se os principais estados produtores, a questão da importação, os preços praticados, a estrutura agrária brasileira como um fator significativo para análise deste setor produtivo e o mercado internacional da ovinocultura. Para tanto são utilizados dados do Instituto Brasileiro de Geografia e Estatística, da Organização das Nações Unidas para Agricultura e Alimentação e outras fontes secundárias especializadas no setor. Os países com o maior rebanho ovino no mundo são China, Índia e Austrália, respectivamente, e a produção de carne ovina está concentrada majoritariamente no continente asiático (52%). Os dados demonstram que o Brasil possui o rebanho ovino concentrado em alguns estados da região Nordeste e no Rio Grande do Sul, os preços aos produtores têm se mantido estáveis no último ano com uma leve tendência de alta, que há uma tendência para o desenvolvimento da indústria de abate e de processamento e, como consequência, uma aproximação ao mercado consumidor. No entanto, conclui-se que persistem entraves organizacionais que impedem o desenvolvimento do setor e que precisam ser superados com urgência. Abstract: The aim of this paper is to present data on the market and the commercialization of sheep meat in Brazil. Specifically we highlight the major producing states, the issue of importation, the prices, the Brazilian agrarian structure as a significant factor for the analysis of this sector and the international market. To achieve this goal, the data were provided by the Brazilian Institute of Geography and Statistics and by the United Nations Food and Agriculture and other specialized secondary sources. Countries with the largest sheep flock in the world are China, India and Australia, respectively, and the meat production is mainly concentrated in Asia (52%). The data show that Brazilian sheep flock are concentrated in a few states in the Northeast and Rio Grande do Sul, the producer prices have remained stable over the last year with a slight upward trend, there is a tendency for the development of slaughter and processing industry and, as a consequence, an approximation to the consumer market. However, it is concluded that organizational obstacles remain and hinder the development of the sector and they must be overcome urgently
Detectability of the First Cosmic Explosions
We present a fully self-consistent simulation of a synthetic survey of the
furthermost cosmic explosions. The appearance of the first generation of stars
(Population III) in the Universe represents a critical point during cosmic
evolution, signaling the end of the dark ages, a period of absence of light
sources. Despite their importance, there is no confirmed detection of
Population III stars so far. A fraction of these primordial stars are expected
to die as pair-instability supernovae (PISNe), and should be bright enough to
be observed up to a few hundred million years after the big bang. While the
quest for Population III stars continues, detailed theoretical models and
computer simulations serve as a testbed for their observability. With the
upcoming near-infrared missions, estimates of the feasibility of detecting
PISNe are not only timely but imperative. To address this problem, we combine
state-of-the-art cosmological and radiative simulations into a complete and
self-consistent framework, which includes detailed features of the
observational process. We show that a dedicated observational strategy using
per cent of total allocation time of the James Webb Space
Telescope mission can provide us up to detectable PISNe per year.Comment: 9 pages, 8 figures. Minor corrections added to match published
versio
Using gamma regression for photometric redshifts of survey galaxies
Machine learning techniques offer a plethora of opportunities in tackling big
data within the astronomical community. We present the set of Generalized
Linear Models as a fast alternative for determining photometric redshifts of
galaxies, a set of tools not commonly applied within astronomy, despite being
widely used in other professions. With this technique, we achieve catastrophic
outlier rates of the order of ~1%, that can be achieved in a matter of seconds
on large datasets of size ~1,000,000. To make these techniques easily
accessible to the astronomical community, we developed a set of libraries and
tools that are publicly available.Comment: Refereed Proceeding of "The Universe of Digital Sky Surveys"
conference held at the INAF - Observatory of Capodimonte, Naples, on
25th-28th November 2014, to be published in the Astrophysics and Space
Science Proceedings, edited by Longo, Napolitano, Marconi, Paolillo, Iodice,
6 pages, and 1 figur
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