1,970 research outputs found
The effect of geometry on charge confinement in three dimensions
We show that, in contrast to the flat case, the Maxwell theory is not
confining in the background of the three dimensional BTZ black-hole (covering
space). We also study the effect of the curvature on screening behavior of
Maxwell-Chern-Simons model in this space-time.Comment: 8 pages. To be published in Europhysics Letter
Gravitational Geometric Phase in the Presence of Torsion
We investigate the relativistic and non-relativistic quantum dynamics of a
neutral spin-1/2 particle submitted an external electromagnetic field in the
presence of a cosmic dislocation. We analyze the explicit contribution of the
torsion in the geometric phase acquired in the dynamic of this neutral
spinorial particle. We discuss the influence of the torsion in the relativistic
geometric phase. Using the Foldy-Wouthuysen approximation, the non-relativistic
quantum dynamics are studied and the influence of the torsion in the
Aharonov-Casher and He-McKellar-Wilkens effects are discussed.Comment: 14 pages, no figur
Spacetime Defects: von K\'arm\'an vortex street like configurations
A special arrangement of spinning strings with dislocations similar to a von
K\'arm\'an vortex street is studied. We numerically solve the geodesic
equations for the special case of a test particle moving along twoinfinite rows
of pure dislocations and also discuss the case of pure spinning defects.Comment: 9 pages, 2figures, CQG in pres
Falsifying Tree Level String Motivated Bouncing Cosmologies
The string effective action at tree level contains, in its bosonic sector,
the Einstein-Hilbert term, the dilaton, and the axion, besides scalar and gauge
fields coming from the Ramond-Ramond sector. The reduction to four dimensions
brings to scene moduli fields. We generalize this effective action by
introducing two arbitrary parameters, and , connected with the
dilaton and axion couplings. In this way, more general frameworks can be
analyzed. Regular solutions with a bounce can be obtained for a range of
(negative) values of the parameter which, however, exclude the pure
string configuration (). We study the evolution of scalar
perturbations in such cosmological scenarios. The predicted primordial power
spectrum decreases with the wavenumber with spectral index , in
contradiction with the results of the . Hence, all such effective string
motivated cosmological bouncing models seem to be ruled out, at least at the
tree level approximation.Comment: Latex file, 19 pages, 3 figures in eps forma
Composição quĂmica e protĂ©ico-molecular da farinha de resĂduos de camarĂŁo-sete-barbas (Xiphopenaeus Kroyeri).
Non-relativistic quantum systems on topological defects space-times
We study the behavior of non-relativistic quantum particles interacting with
different potentials in the space-times generated by a cosmic string and a
global monopole. We find the energy spectra in the presence of these
topological defects and show how they differ from their free space-time values.Comment: 17 pages, LATEX fil
Desempenho de progĂȘnies de açaizeiros provenientes de duas procedĂȘncias avaliadas pelo grĂĄfico de caixa.
Um importante componente da dieta alimentar dos habitantes ribeirinhos e nas cidades do AmapĂĄ e ParĂĄ Ă© o açaĂ, havendo tambĂ©m o interesse em outras regiĂ”es e paĂses. SĂŁo, portanto, importantes as pesquisas visando seleção de materiais superiores para suprir a crescente demanda de consumo. No presente estudo foram comparadas, no campo experimental de MazagĂŁo, da Embrapa AmapĂĄ, 75 progĂȘnies da regiĂŁo do municĂpio do AfuĂĄ, PA com 100 progĂȘnies da regiĂŁo leste da ilha de MarajĂł, PA. O experimento foi instalado em blocos ao acaso com duas repetiçÔes, sendo avaliados os caracteres: quantidade de estipes adultas, quantidade de estipes jovens, quantidade de rebentos, altura de planta adulta, altura de planta jovem, circunferĂȘncia do estipe mais velho, circunferĂȘncia mĂ©dia das estipes jovens, nĂșmero de cachos, comprimento do entrenĂł e quantidade de folhas. Os resultados indicaram desempenhos diferentes entre as procedĂȘncias para todos os caracteres avaliados. As procedĂȘncias oriundas do AfuĂĄ apresentaram valores superiores Ă s do MarajĂł, excetuando-se apenas a quantidade de rebentos. O nĂșmero de folhas foi o Ășnico carĂĄter que nĂŁo apresentou diferenças. Foram observados valores nos extremos dos grĂĄficos de caixa que apresentam progĂȘnies com potencial para serem selecionadas. O grĂĄfico de caixa demonstrou ser um instrumento eficiente para distinguir as duas procedĂȘncias
The Dynamic Universe: Realizing the Potential of Classical Time Domain and Multimessenger Astrophysics
In parallel with the multi-messenger revolution, major advances in time-domain astronomy across multiple science disciplines relevant to astrophysics are becoming more urgent to address. Aside from electromagnetic observations of gravitational wave events and explosive counterparts, there are a number of âclassicalâ astrophysical areas that require new thinking for proper exploration in the time domain. How NASA, NSF, ESA, and ESO consider the 2020 USA Decadal Survey within the astronomy community, as well as the worldwide call to support and expand time domain and multi-messenger astrophysics, it is crucial that all areas of astrophysics, including stellar, galactic, Solar System, and exoplanetary science participate in the discussion, and that it not be made into an exclusive preserve of cosmological, high-energy, explosive and transient science. Time domain astronomy is used to explore many aspects of astrophysicsâparticularly concerning ground- and space-based mission science goals of exploring how the Universe works, understanding how did we get here, and are we alone. Time domain studies are already built into the core operations of many currently operating and future space telescopes (e.g., Roman, PLATO) as well as current and planned large areal ground-based surveys (e.g., Rubin). Time-domain observations designed for one scientific purpose, also lead to great discoveries in many other science areas. The recent advent of user-friendly hardware, software, observational approaches, and online data infrastructure has also helped make time domain observations especially suitable and appealing for citizen science projects. We provide a review of the current state of TDAMM alerts and observational protocols, revealing a wide array of software and applications, much of which is incompatible. Any conversation regarding TDAMM astrophysics should include all aspects of the field, including those aspects seen as classical applications
Electrophoretic profile of mechanically separated meat (MSM) and fillet of fresh Nile tilapia (Oreochromis niloticus) and evaluation of the protein integrity in MSM canned pùté.
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