Detecção do Southern bean mosaic virus no Paraná, e separação do Bean rugose mosaic virus em feijoeiro

Em lavouras de feijoeiro (Phaseolus vulgaris) da cultivar Carioca Comum, no município de Londrina, Estado do Paraná, foram encontradas plantas com sintomas de necrose da haste, mosaico clorótico leve e porte reduzido, semelhantes aos sintomas causados por infecção viral. Exames de microscopia eletrônica revelaram a presença de partículas isométricas. em testes de imunodifusão dupla em gel de ágar os extratos foliares de plantas infetadas reagiram positivamente com anti-soro específico para o Southern bean mosaic virus (SBMV). O vírus foi purificado e a massa molecular de sua proteína capsidial foi estimada em 30 kDa, valor esperado para proteínas do capsídeo de vírus do gênero Sobemovirus. A gama de hospedeiras do SBMV isolado no Paraná foi restrita ao feijoeiro e a algumas cultivares de soja (Glycine max). A separação de dois vírus isométricos comuns em infecções mistas no feijoeiro foi possível através da reação de imunidade ao SBMV apresentada por Crotalaria sp, Chenopodium quinoa e Mucuna deeringiana, e da reação de susceptibilidade dessas mesmas hospedeiras ao Bean rugose mosaic virus (BRMV).

Identificação e caracterização de um potyvírus isolado de Zinnia elegans

O presente trabalho teve como objetivo a identificação e caracterização de um potyvírus isolado de Zinnia elegans, na Região Noroeste do Estado de São Paulo. O potyvírus foi transmitido por inoculação mecânica e apresentou uma gama restrita de hospedeiras sendo que as espécies mais afetadas pertencem à família Asteraceae. em SDS-PAGE, a massa molecular da proteína capsidial (CP) foi estimada em 33 kDa e, em Western-blot, reagiu com anti-soro para o Bidens mosaic virus (BiMV). Um fragmento de aproximadamente 820 pb foi amplificado por RT/PCR, clonado e seqüenciado. O fragmento, que inclui o gene da proteína capsidial, mostrou similaridade de aminoácidos do core da CP variando de 55% (Tobacco vein mottling virus, TVMV) a 95% (Sunflower chlorotic mottle virus, SuCMoV) e da CP completa de 55% (TVMV) a 91% (SuCMoV). Na região N-terminal, o potyvírus de Zinnia tem uma deleção de quatro aminoácidos (posições 9 a 12 após o sítio de clivagem entre a proteína NIb e a CP) quando comparada com a seqüência do SuCMoV. A análise filogenética agrupou o potyvírus de Zinnia e o SuCMoV em um mesmo ramo em 100% das réplicas, mostrando uma relação de parentesco muito próxima entre esses dois vírus. Os resultados obtidos no presente trabalho demonstraram que o potyvírus de Zinnia e o SuCMoV são estirpes do mesmo vírus. Sugere-se o nome Sunflower chlorotic mottle virus, isolado Zinnia (SuCMoV-Zi), ao potyvírus encontrado em Z. elegans no Brasil.

Kinematics of a spacetime with an infinite cosmological constant

A solution of the sourceless Einstein's equation with an infinite value for the cosmological constant L is discussed by using Inonu-Wigner contractions of the de Sitter groups and spaces. When Lambda --> infinity, spacetime becomes a four-dimensional cone, dual to Minkowski space by a spacetime inversion. This inversion relates the four-cone vertex to the infinity of Minkowski space, and the four-cone infinity to the Minkowski light-cone. The non-relativistic limit c --> infinity. is further considered, the kinematical group in this case being a modified Galilei group in which the space and time translations are replaced by the non-relativistic limits of the corresponding proper conformal transformations. This group presents the same abstract Lie algebra as the Galilei group and can be named the conformal Galilei group. The results may be of interest to the early Universe Cosmology.

Conformal Klein-Gordon equations and quasinormal modes

Using conformal coordinates associated with conformal relativity-associated with de Sitter spacetime homeomorphic projection into Minkowski spacetime-we obtain a conformal Klein-Gordon partial differential equation, which is intimately related to the production of quasi-normal modes (QNMs) oscillations, in the context of electromagnetic and/or gravitational perturbations around, e.g., black holes. While QNMs arise as the solution of a wave-like equation with a Poschl-Teller potential, here we deduce and analytically solve a conformal 'radial' d'Alembert-like equation, from which we derive QNMs formal solutions, in a proposed alternative to more completely describe QNMs. As a by-product we show that this 'radial' equation can be identified with a Schrodinger-like equation in which the potential is exactly the second Poschl-Teller potential, and it can shed some new light on the investigations concerning QNMs.

Spacetime algebraic skeleton

The cosmological constant is shown to have an algebraic meaning: it is essentially an eigenvalue of a Casimir invariant of the Lorentz group acting on the spaces tangent to every spacetime. This is found in the context of de Sitter spacetimes, for which the Einstein equation is a relation between operators. Nevertheless, the result brings, to the foreground the skeleton algebraic structure underlying the geometry of general physical spacetimes. which differ from one another by the fleshening of that structure by different tetrad fields.

Cosmological term and fundamental physics

A nonvanishing cosmological term in Einstein's equations implies a nonvanishing spacetime curvature even in the absence of any kind of matter. It would, in consequence, affect many of the underlying kinematic tenets of physical theory. The usual commutative spacetime translations of the Poincare group would be replaced by the mixed conformal translations of the de Sitter group, leading to obvious alterations in elementary concepts such as time, energy and momentum. Although negligible at small scales, such modifications may come to have important consequences both in the large and for the inflationary picture of the early Universe. A qualitative discussion is presented, which suggests deep changes in Hamiltonian, Quantum and Statistical Mechanics. In the primeval universe as described by the standard cosmological model, in particular, the equations of state of the matter sources could be quite different from those usually introduced.

Non-relativistic spacetimes with cosmological constant

Recent data on supernovae favour high values of the cosmological constant. Spacetimes with a cosmological constant have non-relativistic kinematics quite different from Galilean kinematics. de Sitter spacetimes, vacuum solutions of Einstein's equations with a cosmological constant, reduce in the non-relativistic limit to Newton-Hooke spacetimes, which are non-metric homogeneous spacetimes with non-vanishing curvature. The whole non-relativistic kinematics would then be modified, with possible consequences to cosmology, and in particular to the missing-mass problem.

A singular conformal spacetime

The infinite cosmological constant limit of the de Sitter solutions to Einstein's equation is studied. The corresponding spacetime is a singular, four-dimensional cone-space, transitive under proper conformal transformations, which constitutes a new example of maximally-symmetric spacetime. Grounded on its geometric and thermodynamic properties, some speculations are made in connection with the primordial universe. (c) 2005 Elsevier B.V. All rights reserved.

Primeval symmetries

A detailed examination of the Killing equations in Robertson-Walker coordinates shows how the addition of matter and/or radiation to a de Sitter Universe breaks the symmetry generated by four of its Killing fields. The product U = a(2) H of the squared scale parameter by the time-derivative of the Hubble function encapsulates the relationship between the two cases: the symmetry is maximal when U is a constant, and reduces to the six-parameter symmetry of a generic Friedmann-Robertson-Walker model when it is not. As the fields physical interpretation is not clear in these coordinates, comparison is made with the Killing fields in static coordinates, whose interpretation is made clearer by their direct relationship to the Poincare group generators via Wigner-Inonu contractions.

IS PHYSICS ASKING FOR A NEW KINEMATICS?

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Gravitação semiclássica

Fazemos aqui uma breve descrição da teoria semiclássica da gravitação que tem conseguido antecipar de forma bastante robusta alguns efeitos de gravitação quântica.

Natural antibodies in paracoccidioidomycosis

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Anatomy and ontogeny of Pterodon emarginatus (Fabaceae: Faboideae) seed

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Taxonomy of Ophiuroidea (Echinonermata) from the continental shelf and slope of the southern and southeastern Brazilian coast

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Ichthyofauna of the rio Itatinga in the Parque das Neblinas, Bertioga, São Paulo State: composition and biogeography

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)