Study on the Radiation Shielding Performance of an Assembly of Concrete Blocks

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New Particles from Belle

I report recent results on hidden charm spectroscopy from Belle. These include: observation of a near-threshold enhancement in the omega-J/psi invariant mass distribution for exclusive B-->K omega J/psi decays; evidence for the decay X(3872)-->pi+pi-pi0 J/psi, where the pi+pi-pi0 invariant mass distribution has a strong peak between 750 MeV and the kinematic limit of 775 MeV, suggesting that the process is dominated by the sub-threshold decay X-->omega J/psi; and the observation of a peak near 3940 MeV in the J/psi recoil mass spectrum for the inclusive continuum process e+e- --> J/psi X. The results are based on a study of a 287 fb-1 sample of e+e- annihilation data collected at center- of-mass energies around the Upsilon(4S) in the Belle detector at the KEKB collider.Comment: 10 pages 12 figures. Invited talk at the 1st meeting of the APS Topical Group on Hadronic Physics, Fermilab, October 24-26, 2004; revised to correct some reference

Infrared study of spin crossover Fe-picolylamine complex

Infrared (IR) absorption spectroscopy has been used to probe the evolution of microscopic vibrational states upon the temperature- and photo-induced spin crossovers in [Fe(2-picolylamine)3]Cl2EtOH (Fe-pic). To overcome the small sizes and the strong IR absorption of the crystal samples used, an IR synchrotron radiation source and an IR microscope have been used. The obtained IR spectra of Fe-pic show large changes between high-spin and low-spin states for both the temperature- and the photo- induced spin crossovers. Although the spectra in the temperature- and photo-induced high-spin states are relatively similar to each other, they show distinct differences below 750 cm-1. This demonstrates that the photo-induced high-spin state involves microscopically different characters from those of the temperature-induced high-spin state. The results are discussed in terms of local pressure and structural deformations within the picolylamine ligands, and in terms of their possible relevance to the development of macroscopic photo-induced phase in Fe-pic.Comment: 6 pages (text) and 6 figures,submitted to J. Phys. Soc. Jp

Parâmetros biológicos de Heliothis virescens (Lepidoptera: Noctuidae) em folha e vagem de feijão.

Heliothis virescens (Fabricius, 1781) (Lepidoptera: Noctuidae) é uma praga polífaga, e recentemente tem sido relatada atacando a cultura do feijão. O inseto é capaz de se alimentar de estruturas vegetativas e reprodutivas da planta, porém são escassas as informações a respeito do desenvolvimento da praga nessas estruturas. Desse modo, este trabalho objetivou avaliar parâmetros biológicos de H. virescens alimentada com folhas e vagens verdes de feijão. O estudo foi realizado em delineamento inteiramente casualizado, com 10 repetições (n=7 espécimes / repetição). A cultivar utilizada no trabalho foi a BRS Ametista Carioca, sendo que o material foi coletado no estádio R8, em plantas com 90 dias de idade. As folhas ofertadas foram obtidas do terço superior da planta. Os tratamentos (folha e vagem) foram ofertados ad libitum para as lagartas recém-eclodidas, em condições controladas de temperatura 25±2°C, UR 70±10% e fotofase de 14 hs. A partir do 5° instar larval foi avaliado o consumo de alimento. Após a emergência dos adultos, foram formados casais para posterior avaliação dos parâmetros reprodutivos das mariposas. De forma geral, foi observado que os indivíduos alimentados somente com folhas de feijão não conseguiram completar a fase jovem. Entretanto, quando alimentadas com vagens de feijão, as lagartas apresentaram longevidade média de 12 dias, com viabilidade de 56%. Os insetos consumiram 3,57g de feijão vagem, e o peso de pupa foi de 0,21g. Durante a fase adulta, as fêmeas apresentaram fecundidade média de 240 ovos, com viabilidade em torno de 40%. Esses resultados demonstram que embora H. virescens possa se alimentar de folhas de feijão, o seu desempenho biológico é maior quando se alimenta das vagens da planta. Desse modo, é fundamental o monitoramento populacional da praga durante o estádio reprodutivo da cultura, pois é o momento em que a praga encontra o alimento mais apropriado para o seu desenvolvimento, e desse modo pode ser necessária a adoção de estratégias de controle

Wet and dry deposition of mineral dust particles in Japan: factors related to temporal variation and spatial distribution

Recent ground networks and satellite remote-sensing observations have provided useful data related to spatial and vertical distributions of mineral dust particles in the atmosphere. However, measurements of temporal variations and spatial distributions of mineral dust deposition fluxes are limited in terms of their duration, location, and processes of deposition. To ascertain temporal variations and spatial distributions of mineral dust deposition using wet and dry processes, weekly deposition samples were obtained at Sapporo, Toyama, Nagoya, Tottori, Fukuoka, and Cape Hedo (Okinawa) in Japan during October 2008–December 2010 using automatic wet and dry separating samplers. Mineral dust weights in water-insoluble residue were estimated from Fe contents measured using an X-ray fluorescence analyser. Wet and dry deposition fluxes of mineral dusts were both high in spring and low in summer, showing similar seasonal variations to frequency of aeolian dust events (Kosa) in Japan. For wet deposition, highest and lowest annual dust fluxes were found at Toyama (9.6 g m⁻² yr⁻¹) and at Cape Hedo (1.7 g m⁻² yr⁻¹) as average values in 2009 and 2010. Higher wet deposition fluxes were observed at Toyama and Tottori, where frequent precipitation (> 60% days per month) was observed during dusty seasons. For dry deposition among Toyama, Tottori, Fukuoka, and Cape Hedo, the highest and lowest annual dust fluxes were found respectively at Fukuoka (5.2 g m⁻² yr⁻¹) and at Cape Hedo (2.0 g m⁻² yr⁻¹) as average values in 2009 and 2010. The average ratio of wet and dry deposition fluxes was the highest at Toyama (3.3) and the lowest at Hedo (0.82), showing a larger contribution of the dry process at western sites, probably because of the distance from desert source regions and because of the effectiveness of the wet process in the dusty season. <br><br> Size distributions of refractory dust particles were obtained using four-stage filtration: > 20, > 10, > 5, and > 1 μm diameter. Weight fractions of the sum of > 20 μm and 10–20 μm (giant fraction) were higher than 50% for most of the event samples. Irrespective of the deposition type, the giant dust fractions generally decreased with increasing distance from the source area, suggesting the selective depletion of larger giant particles during atmospheric transport. Based on temporal variations of PM_c (2.5 < <i>D</i> < 10 μm), ground-based lidar, backward air trajectories, and vertical profiles of potential temperatures, transport processes of dust particles are discussed for events with high-deposition and low-deposition flux with high PM_c. Low dry dust depositions with high PM_c concentrations were observed under stronger (5 K km⁻¹) stratification of potential temperature with thinner and lower (< 2 km) dust distributions because the PM_c fraction of dust particles only survived after depletion of giant dust particles by rapid gravitational settling at the time they reach Japan. In contrast, transport through a thicker (> 2 km) dust layer with weak vertical gradient of potential temperature carry more giant dust particles to Japan. Because giant dust particles are an important mass fraction of dust accumulation, especially in the North Pacific, which is known as a high-nutrient, low-chlorophyll (HNLC) region, the transport height and fraction of giant dust particles are important factors for studying dust budgets in the atmosphere and their role in biogeochemical cycles

A major star formation region in the receding tip of the stellar Galactic bar

We present an analysis of the optical spectroscopy of 58 stars in the Galactic plane at $l=27$\arcdeg, where a prominent excess in the flux distribution and star counts have been observed in several spectral regions, in particular in the Two Micron Galactic Survey (TMGS) catalog. The sources were selected from the TMGS, to have a $K$ magnitude brighter than +5 mag and be within 2 degrees of the Galactic plane. More than 60% of the spectra correspond to stars of luminosity class I, and a significant proportion of the remainder are very late giants which would also be fast evolving. This very high concentration of young sources points to the existence of a major star formation region in the Galactic plane, located just inside the assumed origin of the Scutum spiral arm. Such regions can form due to the concentrations of shocked gas where a galactic bar meets a spiral arm, as is observed at the ends of the bars of face-on external galaxies. Thus, the presence of a massive star formation region is very strong supporting evidence for the presence of a bar in our Galaxy.Comment: 13 pages (latex) + 4 figures (eps), accepted in ApJ Let