Gerasimov-Drell-Hearn sum rule and the single-pion photoproduction multipole E0+ close to threshold

The long-standing discrepancy between the Gerasimov-Drell-Hearn sum rule and the analysis of pion photoproduction multipoles is greatly diminished by use of s-wave multipoles that are in accord with the predictions of chiral perturbation theory and describe the experimental data in the threshold region. The remaining difference may be due to contributions of channels with more pions and/or heavier mesons whose contributions to the sum rule remain to be investigated by a direct measurement of the photoabsorption cross sections.

Identification of races of Bremia lactucae in São Paulo, Brazil

Lettuce, Lactuca sativa, is the most important leafy vegetable in the diet of the Brazilian people. However, the lettuce crop is susceptible to downy mildew disease which is caused by the fungus Bremia lactucae. Downy mildew is most troublesome during winter conditions in regions with mild temperatures. This coincides with the time for growing large quantities of lettuce. The high cost of cultivation and the infection of downy mildew in the winter, just when market prices are low, provides an economic challenge for Brazilian growers. The objective of this study was to identify the races of Bremia lactucae that occur in the growing regions of São Paulo during 2004. The study was conducted in the Laboratory of Vegetable Crop Genetics in the Department of Crop Production of the Faculty of Agricultural and Veterinary Sciences - UNESP, Jaboticabal Campus. In the present study, 92 isolates of B. lactucae were identified from São Paulo. The isolates were shown to display mainly a Sextet code 63/63/51/00 behavior, characterizing the race with regard to coverage and economic importance. The genes that confer resistance accounting for this behavior are DM 17, DM 18 and DM 38. Their use is recommended as sources of resistance to downy mildew in lettuce breeding programs.

Las raíces del proteccionismo en los Estados Unidos

Incluye Bibliografía

Identidades y sentido de pertenencia y sus tensiones contemporáneas para la cohesión social: ¿del derrotero a las raíces y

Incluye Bibliografía

Las relaciones entre niveles de gobierno en Argentina. Raíces históricas, instituciones y conflictos persistentes

Incluye Bibliografía

Chaotic diffusion caused by close encounters with several massive asteroids: II. the regions of (10) Hygiea, (2) Pallas, and (31) Euphrosyne

Context. Close encounters with (1) Ceres and (4) Vesta, the two most massive bodies in the main belt, are known to be a mechanism of dynamical mobility able to significantly alter proper elements of minor bodies, and they are the main source of dynamical mobility for medium-sized and large asteroids (D > 20 km, approximately). Recently, it has been shown that drift rates caused by close encounters with massive asteroids may change significantly on timescales of 30 Myr when different models (i.e., different numbers of massive asteroids) are considered. Aims. So far, not much attention has been given to the case of diffusion caused by the other most massive bodies in the main belt: (2) Pallas, (10) Hygiea, and (31) Euphrosyne, the third, fourth, and one of the most massive highly inclined asteroids in the main belt, respectively. Since (2) Pallas is a highly inclined object, relative velocities at encounter with other asteroids tend to be high and changes in proper elements are therefore relatively small. It was thus believed that the scattering effect caused by highly inclined objects in general should be small. Can diffusion by close encounters with these asteroids be a significant mechanism of long-term dynamical mobility? Methods. By performing simulations with symplectic integrators, we studied the problem of scattering caused by close encounters with (2) Pallas, (10) Hygiea, and (31) Euphrosyne when only the massive asteroids (and the eight planets) are considered, and the other massive main belt asteroids and non-gravitational forces are also accounted for. Results. By finding relatively small values of drift rates for (2) Pallas, we confirm that orbital scattering by this highly inclined object is indeed a minor effect. Unexpectedly, however, we obtained values of drift rates for changes in proper semi-major axis a caused by (10) Hygiea and (31) Euphrosyne larger than what was previously found for scattering by (4) Vesta. These high rates may have repercussions on the orbital evolution and age estimate of their respective families. © 2013 ESO.

Nota de la Secretaría sobre la elección de nuevos miembros del Consejo Directivo del Instituto Latinoamericano de Planificación Económica y Social = Note by the Secretariat on the election of new members of the Governing Council of the Latin American Institute for Economic and Social Planning

Incluye Bibliografía

Four-Boson Systems Close to a Universal Regime

Universal properties of weakly-bound four-boson systems near the scaling limit are discussed by considering recent results obtained from the solution of Faddeev-Yakubovsky (FY) equations, which confirm a previous conjecture on a four-body scale dependence. In the present contribution, within a discussion on our numerical results obtained for the binding energies of two consecutive tetramer states, we are analyzing the relative relevance of the two possible configurations of the four-body system. © 2013 Springer-Verlag Wien.