731 research outputs found
Construção social de mercados e valorização de produtos agroextrativistas do Cerrado pelos atores gastronômicos
Este trabalho tem como objetivo analisar como as ações implementadas pelos atores da gastronomia estão envolvidas no processo de construção social de mercados e valorização de produtos agroextrativistas do Cerrado. O foco do trabalho centrouse na primeira e segunda edição do Festival Gastronômico Cerrado Week, organizadas em 2014 e 2015 pelo Slow Food Cerrado e outros atores locais e regionais. (Résumé d'auteur
Massive 3+1 Aharonov-Bohm fermions in an MIT cylinder
We study the effect of a background flux string on the vacuum energy of
massive Dirac fermions in 3+1 dimensions confined to a finite spatial region
through MIT boundary conditions. We treat two admissible self-adjoint
extensions of the Hamiltonian. The external sector is also studied and
unambiguous results for the Casimir energy of massive fermions in the whole
space are obtained.Comment: 12 pages, 5 figures, LaTe
PACCE: Perl Algorithm to Compute Continuum and Equivalent Widths
We present Perl Algorithm to Compute continuum and Equivalent Widths (pacce).
We describe the methods used in the computations and the requirements for its
usage. We compare the measurements made with pacce and "manual" ones made using
iraf splot task. These tests show that for SSP models the equivalent widths
strengths are very similar (differences <0.2A) for both measurements. In real
stellar spectra, the correlation between both values is still very good, but
with differences of up to 0.5A. pacce is also able to determine mean continuum
and continuum at line center values, which are helpful in stellar population
studies. In addition, it is also able to compute the uncertainties in the
equivalent widths using photon statistics. The code is made available for the
community through the web at http://www.if.ufrgs.br/~riffel/software.html.Comment: 8 pages, 5 figures, accepted by Astrophysics and Space Scienc
Scaling anomaly in cosmic string background
We show that the classical scale symmetry of a particle moving in cosmic
string background is broken upon inequivalent quantization of the classical
system, leading to anomaly. The consequence of this anomaly is the formation of
single bound state in the coupling interval \gamma\in(-1,1). The inequivalent
quantization is characterized by a 1-parameter family of self-adjoint extension
parameter \omega. It has been conjectured that the formation of loosely bound
state in cosmic string background may lead to the so called anomalous
scattering cross section for the particles, which is usually seen in molecular
physics.Comment: 4 pages,1 figur
Semiclassical Quantization for the Spherically Symmetric Systems under an Aharonov-Bohm magnetic flux
The semiclassical quantization rule is derived for a system with a
spherically symmetric potential and an
Aharonov-Bohm magnetic flux. Numerical results are presented and compared with
known results for models with . It is shown that the
results provided by our method are in good agreement with previous results. One
expects that the semiclassical quantization rule shown in this paper will
provide a good approximation for all principle quantum number even the rule is
derived in the large principal quantum number limit . We also discuss
the power parameter dependence of the energy spectra pattern in this
paper.Comment: 13 pages, 4 figures, some typos correcte
Optimization of low temperature RF-magnetron sputtering of indium tin oxide films for solar cell applications
In this work we have studied the influence of argon working pressure, substrate temperature, low power plasma irradiation and partial pressure of hydrogen in the RF-magnetron sputtering of indium tin oxide (ITO) thin films on glass substrates. This work aims at identifying the best conditions to achieve good quality ITO films at low temperature for deposition on heat-sensitive substrates. Four sets of samples were prepared which were characterized by X-ray diffraction (XRD), Van der Pauw and transmittance measurements. It was found that structural, electrical and optical properties of the films depend strongly on the deposition parameters. ITO films with a thickness of ~300 nm, displaying a sheet resistance of 68 Ω/sq and average transmittance, in the visible range, of about 90% were produced performing the deposition at low pressure and at room temperature. However, further improvements in the sheet resistance up to a factor of 3 were obtained by decreasing a little more the argon working pressure or applying a low power plasma irradiation or adding a partial pressure of hydrogen to the working gas. Films produced at low working pressures are crystalline and have [222] preferential orientation. The conductivity and transmittance of these films are higher than those of films deposited at high pressures. The electrical resistivity of the ITO thin films decreased sharply either with low power plasma irradiation or the addition of a partial pressure of H2 to the working gas. All the films showed an average transmittance of over 80% in the visible range. Therefore, as a result of this work we established that the addition of a small partial pressure of H2 to the working gas during growth allowed us to achieve the main aim of depositing low resistivity ITO films at low substrate temperature suitable for the envisaged applications. At the same time, we concluded that this approach leads to a drastic reduction in the amount of target surface conditioning required every time a new target was installed because it turns the properties of the ITO films more independent of the target surface properties.publishe
Half-BPS cosmic string in N=2 supergravity in the presence of a dilaton
We construct new half-BPS cosmic string solutions in D=4 N=2 supergravity
compatible with a consistent truncation to N=1 supergravity where they describe
D-term cosmic strings. The constant Fayet-Iliopoulos term in the N=1 D-term is
not put in by hand but is geometrically engineered by a gauging in the mother
N=2 supergravity theory. The coupling of the N=2 vector multiplets is
characterized by a cubic prepotential admitting an axion-dilaton field, a
common property of many compactifications of string theory. The axion-dilaton
field survives the truncation to N=1 supergravity. On the string configuration
the BPS equations constrain the dilaton to be an arbitrary constant. All the
cosmic string solutions with different values of the dilaton have the same
energy per unit length but different lenght scales.Comment: 52 pages; typos correcte
Annealing of RF-magnetron sputtered SnS2 precursors as a new route for single phase SnS thin films
Tin sulphide thin films have been grown on soda-lime glass substrates through the annealing of RF-magnetron
sputtered SnS2 precursors. Three different approaches to the annealing were compared and the
resulting films thoroughly studied. One series of precursors was annealed in a tubular furnace directly
exposed to a flux of sulphur vapour plus forming gas, N2 + 5%H2, and at a constant pressure of 500 mbar.
The other two series of identical precursors were annealed in the same furnace but inside a graphite box
with and without elemental sulphur evaporation again in the presence of N2 + 5%H2 and at the same pressure
as for the sulphur flux experiments. Different maximum annealing temperatures for each set of samples,
in the range of 300–570 C, were tested to study their effects on the properties of the final films. The
resulting phases were structurally investigated by X-Ray Diffraction (XRD) and Raman spectroscopy.
Annealing of SnS2 precursors in sulphur flux produced films where SnS2 was dominant for temperatures
up to 480 C. Increasing the temperature to 530 C and 570 C led to films where the dominant phase
became Sn2S3. Annealing of SnS2 precursors in a graphite box with sulphur vapour at temperatures in
the range between 300 C and 480 C the films are multi-phase, containing Sn2S3, SnS2 and SnS. For high
annealing temperatures of 530 C and 570 C the films have SnS as the dominant phase. Annealing of SnS2
precursors in a graphite box without sulphur vapour at 300 C and 360 C the films are essentially amorphous,
at 420 C SnS2 is the dominant phase. For temperatures of 480 C and 530 C SnS is the dominant
phase but also same residual SnS2 and Sn2S3 phases are observed. For annealing at 570 C, according to
the XRD results the films appear to be single phase SnS. The composition was studied using energy dispersive
spectroscopy being then correlated with the annealing temperature. Scanning electron microscopy
studies revealed that the SnS films exhibit small grain structure and the film surface is rough.
Optical measurements were performed, from which the band gap energies were estimated. These studies
show that the direct absorption transitions of SnS are at 1.68 eV and 1.41 eV for annealing in graphite box
with and without elemental sulphur evaporation, respectively. For the indirect transition the values varied
from 1.49 eV to 1.37 eV. The results of this work show that the third approach is better suited to produce
single phase SnS films. However, a finer tunning of the duration of the high temperature plateau of
the annealing profile is required in order to eliminate the b-Sn top layer.info:eu-repo/semantics/publishedVersio
Enriquecimiento nutricional de aceites vegetales con ácidos grasos n-3 de cadena larga mediante interesterificación enzimática con una nueva lipasa vegetal
The aim of the present work was to produce vegetable oils enriched with long-chain n-3 fatty acids of nutraceutical interest, through an enzyme-catalyzed interesterification with a new lipase, from physic nut (Jatropha curcas L.). The Vegetable Lipase Powder (biocatalyst) called VLP, which has never been applied in functional foods, was obtained from the physic nut seed, and efficiently hydrolyzed the 95% of waste fish oil in 24 h. Urea precipitation was used to concentrate polyunsaturated fatty acids (PUFA) and was further interesterified with oils of different sources by means of enzymatic catalysis. After the interesterification reaction, which was also catalyzed by the VLP, the PUFA content in coconut oil increased almost ten-fold from 1.8% to 17.7%. In palm oil, the PUFA content increased two-fold from 10.5% to 21.8%, while in olive oil the level of PUFA increased from 8.6% to 21.3%. The mixture of eicosapentaenoic acid (EPA) and docosahexaenoic acid (DHA) (3.7% to 3.9%) was incorporated into the triacylglycerol fraction of each of the coconut, palm and olive oils. Through the hydroesterification (hydrolysis followed by interesterification) all the interesterified vegetable oils tested presented sufficient EPA and DHA levels to satisfy the levels recommended for intake by human adults in one tablespoon.El objetivo del presente trabajo fue producir aceites vegetales enriquecidos con ácidos grasos n-3 de cadena larga de interés nutraceutico, por interesterificación catalizada mediante una nueva lipasa, una enzima de semilla de Jatropha curcas L. La lipasa vegetal en polvo (biocatalizador) llamada VLP, nunca ha sido aplicada en alimentos funcionales, se obtuvo mediante procedimientos físicos con semillas de nueces, e hidrolizó eficientemente el 95% de aceites de residuos de pescado en 24 h. La precipitación con urea se utilizó para concentrar los ácidos grasos poliinsaturados (PUFA) que fueron posteriormente interesterificados con aceites de diferentes fuentes mediante catálisis enzimática. Tras la reacción de interesterificación, que también fue catalizada por la VLP, el contenido de PUFA en el aceite de coco aumentó casi diez veces de 1,8% a 17,7%. En el aceite de palma, el contenido de PUFA aumentó dos veces desde 10,5% a 21,8%, mientras que en el aceite de oliva el nivel de PUFA incrementó de 8,6% a 21,3%. La mezcla de ácido eicosapentaenoico (EPA) y ácido docosahexaenoico (DHA) (3,7% a 3,9%) fué incorporada a la fracción de triacilgliceroles de cada uno de los aceites, coco, palma y oliva. Mediante hidroesterificación (hidrólisis seguido de interesterificación) todos los aceites vegetales interesterificados ensayados contienen en una cucharada suficientes niveles de EPA y DHA para cubrir los niveles recomendados de ingesta de humanos adultos
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