16,002 research outputs found
Shadows and strong gravitational lensing: a brief review
For ultra compact objects (UCOs), Light Rings (LRs) and Fundamental Photon
Orbits (FPOs) play a pivotal role in the theoretical analysis of strong
gravitational lensing effects, and of BH shadows in particular. In this short
review, specific models are considered to illustrate how FPOs can be useful in
order to understand some non-trivial gravitational lensing effects. This paper
aims at briefly overviewing the theoretical foundations of these effects,
touching also some of the related phenomenology, both in General Relativity
(GR) and alternative theories of gravity, hopefully providing some intuition
and new insights for the underlying physics, which might be critical when
testing the Kerr black hole hypothesis.Comment: 32 pages, 9 figures; Review paper in the General Relativity and
Gravitation (GRG) Topical Collection "Testing the Kerr spacetime with
gravitational-wave and electromagnetic observations" (Guest Editor: Emanuele
Berti); v2: Typo corrected and two references adde
Interpretation of Pliocene littoral blocks in eastern Leiria area (central Portugal)
Comunicação apresentada ao VIII Congresso Nacional de Geologia, em Braga (9-16 de Julho 2010)Foram estudados blocos que atingem 2 metros de diâmetro, constituídos por arenito silicioso
ou doleritos, que se encontram na área do sinclinal de Pousos (a leste de Leiria), estratigraficamente
atribuíveis à transição Zancliano-Placenciano. Interpretamos a génese dos blocos siliciosos a partir da
erosão litoral de arenitos siliciosos da Formação de Bom Sucesso e os de rocha básica a partir de
doleritos, durante o máximo transgressivo pliocénico.This paper analyses the large blocks, consisting of siliceous sandstone and basic rock that
are in the eastern area of Leiria (Pousos sinclyne), with Zanclean to Placenzian age. We assumed the
origin of the siliceous sandstone from the destruction by marine erosion of siliceous materials from the
Senhora do Bom Sucesso formation and the basic blocks from the dolerites during the Pliocene maximum
transgressive
Asteroseismic Theory of Rapidly Oscillating Ap Stars
This paper reviews some of the important advances made over the last decade
concerning theory of roAp stars.Comment: 9 pages, 5 figure
A thorough analysis of the short- and mid-term activity-related variations in the solar acoustic frequencies
The frequencies of the solar acoustic oscillations vary over the activity
cycle. The variations in other activity proxies are found to be well correlated
with the variations in the acoustic frequencies. However, each proxy has a
slightly different time behaviour. Our goal is to characterize the differences
between the time behaviour of the frequency shifts and of two other activity
proxies, namely, the area covered by sunspots and the 10.7cm flux. We define a
new observable that is particularly sensitive to the short-term frequency
variations. We then compare the observable when computed from model frequency
shifts and from observed frequency shifts obtained with the Global Oscillation
Network Group (GONG) for cycle 23. Our analysis shows that on the shortest
time-scales the variations in the frequency shifts seen in the GONG
observations are strongly correlated with the variations in the area covered by
sunspots. However, a significant loss of correlation is still found. We verify
that the times when the frequency shifts and the sunspot area do not vary in a
similar way tend to coincide with the times of the maxima of the quasi-biennial
variations seen in the solar seismic data. A similar analysis of the relation
between the 10.7cm flux and the frequency shifts reveals that the short-time
variations in the frequency shifts follow even more closely those of the 10.7cm
flux than those of the sunspot area. However, a loss of correlation between
frequency shifts and 10.7cm flux variations is still found around the same
times.Comment: 7 pages, 6 figures, accepted for publication in MNRA
Equipe técnica de abacaxi comemora 30 anos de atividades e realizações.
A Embrapa Mandioca e Fruticultura Tropical instituiu há poucos anos atrás, os ?Dias dos Produtos? pesquisados pelo Centro. A data escolhida para a comemoração do ?Dia do Abacaxi? foi 04 de novembro. Isso porque foi nessa data que o navegador genovês, Cristóvão Colombo, em uma de suas históricas viagens, aportou na ilha de Guadalupe, e lá encontrou o abacaxi sendo cultivado pelos nativos. Impressionado pela beleza e forma da planta, pelo aroma e sabor do fruto, coletou alguns exemplares e os levou para a Europa, onde esse fruto teve grande aceitação. Em 2007, a comemoração do ?Dia do Abacaxi? foi adiada e ocorreu no dia 10/12/2007 à tarde, e também teve uma programação diferente, da qual constou, além da confraternização informal de praxe, uma sessão técnica composta de um painel. Nesse painel foram apresentadas quatro palestras referentes a alguns dos impactos e avanços obtidos pela Equipe Técnica de Abacaxi /ETA, da Unidade, ao longo de sua existência. Os temas das palestras versaram sobre o VI Simpósio Internacional de Abacaxi (pela primeira vez realizado no continente sulamericano e, mais especificamente, no Brasil); fitossanidade (fusariose) e produção integrada (com destaque para o Tocantins); melhoramento genético (híbridos resistentes e herança da resistência); usos alternativos do abacaxi (como ornamental, flor de corte, de vaso e de jardim); e aspectos econômicos e de mercado (peso médio do fruto brasileiro e posição do Brasil no mercado internacional). As palestras foram apresentadas, respectivamente, pelos pesquisadores Domingo Haroldo Reinhardt (coordenador do simpósio), Aristóteles Pires de Matos, José Renato Santos Cabral, Janay dos Santos-Serejo, Fernanda Vidigal Duarte Souza e Clóvis Oliveira de Almeida.bitstream/CNPMF/24074/1/documentos_170.pd
On the relation between activity-related frequency shifts and the sunspot distribution over the solar cycle 23
The activity-related variations in the solar acoustic frequencies have been
known for 30 years. However, the importance of the different contributions is
still not well established. With this in mind, we developed an empirical model
to estimate the spot-induced frequency shifts, which takes into account the
sunspot properties, such as area and latitude. The comparison between the model
frequency shifts obtained from the daily sunspot records and those observed
suggests that the contribution from a stochastic component to the total
frequency shifts is about 30%. The remaining 70% is related to a global,
long-term variation. We also propose a new observable to investigate the short-
and mid-term variations of the frequency shifts, which is insensitive to the
long-term variations contained in the data. On the shortest time scales the
variations in the frequency shifts are strongly correlated with the variations
in the total area covered by sunspots. However, a significant loss of
correlation is still found, which cannot be fully explained by ignoring the
invisible side of the Sun when accounting for the total sunspot area. We also
verify that the times when the frequency shifts and the sunspot areas do not
vary in a similar way tend to coincide with the times of the maximum amplitude
of the quasi-biennial variations found in the seismic data.Comment: 4 pages, 2 figures, proceedings of the Joint TASC2 - KASC9 Workshop -
SPACEINN - HELAS8 Conference "Seismology of the Sun and the Distant Stars
2016: Using Today's Successes to Prepare the Future". To be published by the
EPJ Web of Conference
Spin-polarized transport in ferromagnetic multilayered semiconductor nanostructures
The occurrence of inhomogeneous spin-density distribution in multilayered
ferromagnetic diluted magnetic semiconductor nanostructures leads to strong
dependence of the spin-polarized transport properties on these systems. The
spin-dependent mobility, conductivity and resistivity in
(Ga,Mn)As/GaAs,(Ga,Mn)N/GaN, and (Si,Mn)/Si multilayers are calculated as a
function of temperature, scaled by the average magnetization of the diluted
magnetic semiconductor layers. An increase of the resistivity near the
transition temperature is obtained. We observed that the spin-polarized
transport properties changes strongly among the three materials.Comment: 3 pages, 4 figure
Impact of micro-telluric lines on precise radial velocities and its correction
Context: In the near future, new instruments such as ESPRESSO will arrive,
allowing us to reach a precision in radial-velocity measurements on the order
of 10 cm/s. At this level of precision, several noise sources that until now
have been outweighed by photon noise will start to contribute significantly to
the error budget. The telluric lines that are not neglected by the masks for
the radial velocity computation, here called micro-telluric lines, are one such
noise source. Aims: In this work we investigate the impact of micro-telluric
lines in the radial velocities calculations. We also investigate how to correct
the effect of these atmospheric lines on radial velocities. Methods: The work
presented here follows two parallel lines. First, we calculated the impact of
the micro-telluric lines by multiplying a synthetic solar-like stellar spectrum
by synthetic atmospheric spectra and evaluated the effect created by the
presence of the telluric lines. Then, we divided HARPS spectra by synthetic
atmospheric spectra to correct for its presence on real data and calculated the
radial velocity on the corrected spectra. When doing so, one considers two
atmospheric models for the synthetic atmospheric spectra: the LBLRTM and TAPAS.
Results: We find that the micro-telluric lines can induce an impact on the
radial velocities calculation that can already be close to the current
precision achieved with HARPS, and so its effect should not be neglected,
especially for future instruments such as ESPRESSO. Moreover, we find that the
micro-telluric lines' impact depends on factors, such as the radial velocity of
the star, airmass, relative humidity, and the barycentric Earth radial velocity
projected along the line of sight at the time of the observation.Comment: Accepted in A&
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