Desenvolvimento da mecanizacao agricola no TSA: programa integrado pesquisa/extensao.

Trata da experimentacao de varias maquinas a tracao animal em varios niveis de mecanizacao e de fontes de tracao. Essa experimentacao tem por objetivo conhecer as maquinas ja existentes, fabricadas no Brasil, determinar e sugerir correcoes das eventuais falhas, testar outras maquinas usadas em condicoes semelhantes as do tropico semi-arido do Brasil, adaptar e desenvolver maquinas mais adequadas a fim de uma fabricacao posterior. As maquinas sao classificadas em 3 conjuntos destinados a diversos niveis de produtores. Dois sao a tracao por corrente: SINE e ARIANA, um a tracao por timao (varao ou cambao) TROPICULTOR

Differential Step Response of Unipolar Space-Charge-Limited Current in Solids

The small signal step response of unipolar space‐charge‐limited current in solids is analyzed for planar structures and for media in which the drift velocity of the charge carriers is either proportional to the electric field (thermal charge carriers) or is independent of the electric field (hot charge carriers). Results are reported in analytical and graphical form. Their features are discussed in terms of the underlying physical phenomena, as well as in the perspective of experimental applications. Cylindrical and spherical structures are not accessible to closed‐form solutions by the approach

How to measure the wave-function absolute squared of a moving particle by using mirrors

We consider a slow particle with wave function $\psi_t(\vec{x})$, moving freely in some direction. A mirror is briefly switched on around a time $T$ and its position is scanned. It is shown that the measured reflection probability then allows the determination of $|\psi_T(\vec{x})|^2$. Experimentally available atomic mirrors should make this method applicable to the center-of-mass wave function of atoms with velocities in the cm/s range.Comment: 4 pages, 5 figure

Whispering Gallery States of Antihydrogen

We study theoretically interference of the long-living quasistationary quantum states of antihydrogen atoms, localized near a concave material surface. Such states are an antimatter analog of the whispering gallery states of neutrons and matter atoms, and similar to the whispering gallery modes of sound and electro-magnetic waves. Quantum states of antihydrogen are formed by the combined effect of quantum reflection from van der Waals/Casimir-Polder (vdW/CP) potential of the surface and the centrifugal potential. We point out a method for precision studies of quantum reflection of antiatoms from vdW/CP potential; this method uses interference of the whispering gallery states of antihydrogen.Comment: 13 pages 7 figure

Reading the Spectra of the Most Peculiar Type Ia Supernova 2002cx

In spite of the apparent lack of Si II and S II features in its spectra, SN 2002cx was classified as a peculiar Type Ia supernova (SN Ia) on the basis of its overall photometric and spectroscopic behavior. Spectra obtained near maximum light contained Fe III features, as in SN 1991T-like events, but the blueshifts of the Fe III absorptions were exceptionally low. The luminosity also was low. We use the supernova synthetic--spectrum code SYNOW to study line identifications in SN 2002cx. We find that the maximum-light spectra appear to contain weak features of Si II, S II, Si III, and Ca II, which strengthens the connection with SN 1991T-like events. We show that later spectra, obtained 12, 25, and 56 days after maximum, consist of P-Cygni resonance-scattering features due to permitted Fe II and Co II lines. SN 2002cx had been thought to have made the transition from a permitted-line to a forbidden-line spectrum between 25 and 56 days. Owing to the low expansion velocities the postmaximum spectral features are narrower and easier to identify than they are in other SNe Ia. SN 2002cx will lead to improved line identifications in other SNe Ia and clarify when the transition from a permitted-line to a forbidden-line spectrum occurs. In the context of current SN Ia explosion models, we suggest that the properties of SN 2002cx may be consistent with 3D deflagration models, which are not favored for normal SNe Ia.Comment: 21 pages including 7 figures and 4 tables; accepted by PAS

Preliminary Spectral Analysis of SN 1994I

We present optical spectra of the Type Ic supernova 1994I in M51 and preliminary non-LTE analysis of the spectra. Our models are not inconsistent with the explosions of C+O cores of massive stars. While we find no direct evidence for helium in the optical spectra, our models cannot rule out small amounts of helium. More than 0.1~\msol\ of helium seems unlikely.Comment: LaTeX, MN style, psfig, and natbib substyles, 7 pages, 4 figures, to appear in MNRAS. Postscript file available from http://www.nhn.uoknor.edu/~baro