5,640 research outputs found
Custo de produção em pecuária de corte em 2009, no Pantanal de Aquidauana (MS).
Conforme os cálculos feitos com os dados levantados na região de Aquidauana, a receita da pecuária de corte consegue cobrir o custo operacional efetivo (COE) e o custo operacional total (COT), é suficiente para abater a depreciação, mas insuficiente para cobrir o capital investido (CI). Este fato indica que a atividade é um investimento sustentável e lucrativo, no curto e no médio prazo, mas não no longo prazo, pois o produtor não conseguirá remunerar seu capital investido.bitstream/CPAP-2010/57273/1/COT77.pd
Custo de produção em pecuária de corte em 2009, no Pantanal de Corumbá (MS).
De acordo com os cálculos dos dados levantados na região de Corumbá, o estudo revelou que a receita da pecuária de corte consegue cobrir o custo operacional efetivo (COE) e o custo operacional total (COT), é suficiente para abater a depreciação, mas insuficiente para cobrir o capital investido (CI). Este fato indica que a atividade é um investimento sustentável e lucrativo, no curto e no médio prazo, mas não em longo prazo, pois o produtor não conseguirá remunerar seu capital investido.bitstream/CPAP-2010/57272/1/COT76.pd
Extreme & High Synchrotron Peaked Blazars at the limit of Fermi-LAT detectability: the -ray spectrum of 1BIGB sources
We present the 1-100 GeV spectral energy distribution for a population of 148
high-synchrotron-peaked blazars (HSPs) recently detected with Fermi-LAT as part
of the First Brazil-ICRANet Gamma-ray Blazar catalogue (1BIGB). Most of the
1BIGB sources do not appear in previous Fermi-LAT catalogues and their
gamma-ray spectral properties are presented here for the first time,
representing a significant new extension of the gamma-ray blazar population.
Since our sample was originally selected from an excess signal in the 0.3-500
GeV band, the sources stand out as promising TeV blazar candidates, potentially
in reach of the forthcoming very-high-energy (VHE) gamma-ray observatory, CTA.
The flux estimates presented here are derived considering PASS8 data,
integrating over more than 9 years of Fermi-LAT observations. We also review
the full broadband fit between 0.3-500 GeV presented in the original 1BIGB
paper for all sources, updating the power-law parameters with currently
available Fermi-LAT dataset. The importance of these sources in the context of
VHE population studies with both current instruments and the future CTA is
evaluated. To do so, we select a subsample of 1BIGB sources and extrapolate
their gamma-ray SEDs to the highest energies, properly accounting for
absorption due to the extragalactic background light. We compare those
extrapolations to the published CTA sensitivity curves and estimate their
detectability by CTA. Two notable sources from our sample, namely 1BIGB
J224910.6-130002 and 1BIGB J194356.2+211821, are discussed in greater detail.
All gamma-ray SEDs, which are shown here for the first time, are made publicly
available via the Brazilian Science Data Center (BSDC) service, maintained at
CBPF, in Rio de Janeiro.Comment: 13 pages, 6 figure
LATTES: a novel detector concept for a gamma-ray experiment in the Southern hemisphere
The Large Array Telescope for Tracking Energetic Sources (LATTES), is a novel
concept for an array of hybrid EAS array detectors, composed of a Resistive
Plate Counter array coupled to a Water Cherenkov Detector, planned to cover
gamma rays from less than 100 GeV up to 100 TeVs. This experiment, to be
installed at high altitude in South America, could cover the existing gap in
sensitivity between satellite and ground arrays.
The low energy threshold, large duty cycle and wide field of view of LATTES
makes it a powerful tool to detect transient phenomena and perform long term
observations of variable sources. Moreover, given its characteristics, it would
be fully complementary to the planned Cherenkov Telescope Array (CTA) as it
would be able to issue alerts.
In this talk, a description of its main features and capabilities, as well as
results on its expected performance, and sensitivity, will be presented.Comment: Proceedings of the 35th International Cosmic Ray Conference
(ICRC2017), Busan, South Korea. Presented by R. Concei\c{c}\~{a}o. 8 pages;
v2: correct affiliation + journal referenc
Produtividade inicial de novas seleções e cultivares de cafeeiros com resistência à ferrugem na Zona da Mata de Minas.
LATTES: A new gamma-ray detector concept for South America
Currently the detection of Very High Energy gamma-rays for astrophysics rely on the measurement of the Extensive Air Showers (EAS) either using Cherenkov detectors or EAS arrays with larger field of views but also larger energy thresholds. In this talk we present a novel hybrid detector concept for a EAS array with an improved sensitivity in the lower energies (~ 100 GeV). We discuss its main features, capabilities and present preliminary results on its expected perfomances and sensitivities.This wide field of view experiment is planned to be installed at high altitude in South America making it a complementary project to the planned Cherenkov telescope experiments and a powerful tool to trigger further observations of variable sources and to detect transients phenomena
Semiclassical theory for small displacements
Characteristic functions contain complete information about all the moments
of a classical distribution and the same holds for the Fourier transform of the
Wigner function: a quantum characteristic function, or the chord function.
However, knowledge of a finite number of moments does not allow for accurate
determination of the chord function. For pure states this provides the overlap
of the state with all its possible rigid translations (or displacements). We
here present a semiclassical approximation of the chord function for large
Bohr-quantized states, which is accurate right up to a caustic, beyond which
the chord function becomes evanescent. It is verified to pick out blind spots,
which are displacements for zero overlaps. These occur even for translations
within a Planck area of the origin. We derive a simple approximation for the
closest blind spots, depending on the Schroedinger covariance matrix, which is
verified for Bohr-quantized states.Comment: 16 pages, 4 figures
G-band Spectral Synthesis in Solar Magnetic Concentrations
Narrow band imaging in the G-band is commonly used to trace the small
magnetic field concentrations of the Sun, although the mechanism that makes
them bright has remained unclear. We carry out LTE syntheses of the G-band in
an assorted set of semi-empirical model magnetic concentrations. The syntheses
include all CH lines as well as the main atomic lines within the band-pass. The
model atmospheres produce bright G-band spectra having many properties in
common with the observed G-band bright points. In particular, the contrast
referred to the quiet Sun is about twice the contrast in continuum wavelengths.
The agreement with observations does not depend on the specificities of the
model atmosphere, rather it holds from single fluxtubes to MIcro-Structured
Magnetic Atmospheres. However, the agreement requires that the real G-band
bright points are not spatially resolved, even in the best observations. Since
the predicted G-band intensities exceed by far the observed values, we foresee
a notable increase of contrast of the G-band images upon improvement of the
angular resolution. According to the LTE modeling, the G-band spectrum emerges
from the deep photosphere that produces the continuum. Our syntheses also
predict solar magnetic concentrations showing up in continuum images but not in
the G-band . Finally, we have examined the importance of the CH
photo-dissociation in setting the amount of G-band absorption. It turns out to
play a minor role.Comment: To appear in ApJ, 554 n2 Jun 20, 33 pages and 9 figure
Efeito de extratos de pimenta do gênero capsicum no controle da mela do feijoeiro (Rhizoctonia solani) in vivo.
O presente trabalho teve como objetivo testar 25 extratos aquosos de pimentas do gênero Capsicum, obtidos a partir de sementes (s), folhas (fo) e frutos (fr) das variedades: ? Bode Amarela?, ?de Gaúcho?, ?Peito-de-Moça?, ?Jurema?, ?Amarela?, ?Acerola?, ?Chifre de Gazela?, ?Carrapeta?, ?Mexicana Roxa Comprida?, ?Mexicana Roxa Pequena?, ?Dedo-de-Moça?, ?dos Desejos?, ?Pitanga Amarela?, ?Biquinho?, ?Síria?, ?Tororó?, ?Três Quinas? e ?Bode Vermelha?
Measuring the Polarization of Boosted Hadronic Tops
We propose a new technique for measuring the polarization of hadronically
decaying boosted top quarks. In particular, we apply a subjet-based technique
to events where the decay products of the top are clustered within a single
jet. The technique requires neither b-tagging nor W-reconstruction, and does
not rely on assumptions about either the top production mechanism or the
sources of missing energy in the event. We include results for various new
physics scenarios made with different Monte Carlo generators to demonstrate the
robustness of the technique.Comment: v2: version accepted for publication in JHE
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