Description of the immature and mature larvae of Bocchus scobiolae Nagy (Hymenoptera: Dryinidae).

The last immature instar and the mature larva of Bocchus scobiolae are described and illustrated for the first time. The affinities of both immature and mature larvae of Bocchus scobiolae and Mystrophorus formicaeformis are discussed to define larval characters of the subfamily Bocchinae.

Tailoring the hexagonal boron nitride nanomesh on Rh(111) with gold.

It is known that the hexagonal boron nitride (h-BN) monolayer has a periodically corrugated structure on Rh(111), termed "nanomesh", while the h-BN layer is planar on the close packed surfaces of coinage metals (Cu, Ag, Au) due the weak interactions. Our studies are aimed at understanding the metal-h-BN interaction, when both Rh and Au are present. On the one hand, the growth and thermal properties of gold deposited on h-BN nanomesh prepared on Rh(111) were studied. On the other hand, the formation of h-BN was examined on Au/Rh surface alloys prepared by the deposition of Au on Rh(111) and subsequent annealing at 1000 K. In each case, the h-BN was prepared by the decomposition of borazine at about 1000 K. Low energy ion scattering (LEIS), X-ray photoelectron spectroscopy (XPS) and scanning tunneling microscopy (STM) measurements revealed that the growth of Au on h-BN/Rh(111) at room temperature leads to the formation of mainly three dimensional (3D) gold nanoparticles, although at low coverages (<0.2 ML) 2D particles formed as well. Stepwise annealing to higher temperatures induces the intercalation of Au below the nanomesh, which was complete at around 1050 K. Some agglomeration and desorption of Au also took place. Interestingly, the nanomesh structure was observable after intercalation up to relatively large Au coverages. Measurements performed in the reverse order, namely exposing a Au/Rh(111) surface alloy to borazine, revealed that Rh atoms get covered by h-BN (or by its precursors) at significantly smaller borazine exposures than Au atoms. The nanomesh structure was essentially present up to a gold coverage of 0.9 ML, but with a smaller pore diameter, while it gradually disappeared at higher gold amounts. In this way the application of surface alloy supports provides a key for gradual tuning of the mesh morphology. Density functional theory calculations confirmed the decreased pore diameter of the BN layer upon the formation of a surface Rh-Au alloy layer.

LEIS and XPS investigation into the growth of cerium and cerium dioxide on Cu(111).

The controlled growth of Ce and CeO2 on Cu(111) was investigated applying low energy ion scattering spectroscopy (LEIS) and X-ray photoelectron spectroscopy (XPS). Previous LEIS studies on metallic and oxidised cerium deposits using other metallic substrates reported serious difficulties related to the neutralization of noble gas ions. For this reason, special attention was paid here to reveal possible matrix effects for the neutralization ("neutralization effects"), which would severely hinder quantitative evaluation of the LEIS data. The adsorption of O2 on Cu(111) induced no neutralization effects either with He(+) or Ne(+). Similarly, no neutralization effects were identified using He(+) upon the deposition of metallic Ce on Cu(111), but it arises for the Ce peak monitored with Ne(+). The initial growth of Ce is two dimensional up to ΘCe ∼ 0.5 ML, while almost complete coverage of Cu(111) is achieved at ΘCe = 2 ML. CeO2(111) was deposited evaporating Ce in a background of O2 at a sample temperature of 523 K. No neutralization effects were observed either with He(+) or Ne(+). In harmony with literature data, the growth mode is three dimensional. Here it was demonstrated that the continuity of the film, which could be efficiently checked by LEIS, is influenced by the applied oxygen pressure in the range of 5 × 10(-7)-3 × 10(-6) mbar. At pO2 = 3 × 10(-6) mbar the film was not completely closed even at relatively large coverages (16 ML), and a significant part of copper atoms were oxidized to Cu(1+). Deposition of CeO2 at pO2 = 5 × 10(-7) mbar was characterized by a nearly perfect wetting, with metallic copper atoms at the interface, and with a slightly more reduced ceria layer.