Nuclear reactions leading to energy levels of Ar37 and K37

In view of recent interest in the Cl³⁷ (ʋ solar’^e-)Ar³⁷ reaction cross section, information on some aspects of mass 37 nuclei has been obtained using the K³⁹ (d, ∝) Ar³⁷ and Cl³⁵ (He³, p) Ar³⁷ reactions. Ar³⁷ levels have been found at 0, 1.41, 1.62, 2.22, 2.50, 2.80, 3.17, 3.27, 3.53, 3.61, 3.71, (3.75), (3.90), 3.94, 4.02, (4.21), 4.28, 4.32, 4.40, 4.45, 4.58, 4.63, 4.74, 4.89, 4.98, 5.05, 5.10, 5.13, 5.21, 5.35, 5.41, 5.44, 5.54, 5.58, 5.67, 5.77, and 5.85 MeV (the underlined values correspond to previously tabulated levels). The nuclear temperature calculated from the Ar³⁷ level density is 1.4 MeV. Angular distributions of the lowest six levels with the K³⁹ (d, ∝) Ar³⁷ reaction at E_d = 10 MeV indicate a dominant direct interaction mechanism and the inapplicability of the 2I + 1 rule of the statistical model. Comparison of the spectra obtained with the K³⁹ (d, ∝) Ar³⁷ and Cl³⁵ (He³, p) Ar³⁷ reactions leads to the suggestion that the 5.13-MeV level is the T = 3/2 Cl³⁷ ground state analog. The ground state Q-value of the Ca⁴⁰ (p, ∝) K³⁷ reaction has been measured: -5179 ± 9 keV. This value implies a K³⁷ mass excess of -24804 ± 10 keV. Description of a NMR magnetometer and a sixteen-detector array used in conjunction with a 61-cm double-focusing magnetic spectrometer are included in appendices.

Isotope shift measurements using k x-rays in Sn, Sm, and W

Electronic Kαl x-ray isotope shifts have been measured for Sn 116-124, Sm 148-154, W 182-184, W 184-186, and W 182-186 using a curved crystal Cauchois spectrometer. The analysis of the measurements has included the electrostatic volume effect, screening by the transition electron as well as the non-transition electrons, normal and specific mass shifts, dynamical nuclear qudrupole polarization, and a radiative correction effect of the electron magnetic moment in the nuclear charge radii are obtained. Where other experimental data are available, the agreement with the present measurements is satisfactory. Comparisons with several nuclear model predictions yield only partial agreement.

Experimental study study of antiproton-proton annihilation into a pair of charged Pi-Mesons or K-Mesons for incident antiproton mementa in the range from 0.72 GeV/c to 2.62 GeV/c

The cross sections for the two antiproton-proton annihilation-in-flight modes,

ˉp + p → π⁺ + π^-

ˉp + p → k⁺ + k^-

were measured for fifteen laboratory antiproton beam momenta ranging from 0.72 to 2.62 GeV/c. No magnets were used to determine the charges in the final state. As a result, the angular distributions were obtained in the form [dσ/dΩ (Θ_C.M.) + dσ/dΩ (π – Θ_C.M.)] for 45 ≲ Θ_C.M. ≲ 135°.

A hodoscope-counter system was used to discriminate against events with final states having more than two particles and antiproton-proton elastic scattering events. One spark chamber was used to record the track of each of the two charged final particles. A total of about 40,000 pictures were taken. The events were analyzed by measuring the laboratory angle of the track in each chamber. The value of the square of the mass of the final particles was calculated for each event assuming the reaction

ˉp + p → a pair of particles with equal masses.

About 20,000 events were found to be either annihilation into π ^±-pair or k ^±-pair events. The two different charged meson pair modes were also distinctly separated.

The average differential cross section of ˉp + p → π⁺ + π^- varied from ~ 25 µb/sr at antiproton beam momentum 0.72 GeV/c (total energy in center-of-mass system, √s = 2.0 GeV) to ~ 2 µb/sr at beam momentum 2.62 GeV/c (√s = 2.64 GeV). The most striking feature in the angular distribution was a peak at Θ_C.M. = 90° (cos Θ_C.M. = 0) which increased with √s and reached a maximum at √s ~ 2.1 GeV (beam momentum ~ 1.1 GeV/c). Then it diminished and seemed to disappear completely at √s ~ 2.5 GeV (beam momentum ~ 2.13 GeV/c). A valley in the angular distribution occurred at cos Θ_C.M. ≈ 0.4. The differential cross section then increased as cos Θ_C.M. approached 1.

The average differential cross section for ˉp + p → k⁺ + k^- was about one third of that of the π^±-pair mode throughout the energy range of this experiment. At the lower energies, the angular distribution, unlike that of the π^±-pair mode, was quite isotropic. However, a peak at Θ_C.M. = 90° seemed to develop at √s ~ 2.37 GeV (antiproton beam momentum ~ 1.82 GeV/c). No observable change was seen at that energy in the π^±-pair cross section.

The possible connection of these features with the observed meson resonances at 2.2 GeV and 2.38 GeV, and its implications, were discussed.

Studies of noble gases in meteorites and in the earth

The isotopic and elemental abundances of noble gases in the solar system are investigated, using simple mixing models and mass-spectrometric measurements of the noble gases in meteorites and terrestrial rocks and minerals.

Primordial neon is modeled by two isotopically distinct components from the interstellar gas and dust. Neon from the gas dominates solar neon, which contains about ten times more ²⁰Ne than ²²Ne. Neon from the dust is represented in meteorites by neon-E, with ²⁰Ne/²²Ne less than 0.6. Isotopic variations in meteorites require neon from both dust and gas to be present. Mixing dust and gas without neon loss generates linear correlation lines on three-isotope and composition-concentration diagrams. A model for solar wind implantation predicts small deviations from linear mixing, due to preferential sputtering of the lighter neon isotopes.

Neon in meteorites consists of galactic cosmic ray spallation neon and at least two primordial components, neon-E and neon-S. Neon was measured in several meteorites to investigate these end- members. Cosmogenic neon produced from sodium is found to be strongly enriched in ²²Ne. Neon measurements on sodium-rich samples must be interpreted with care so not to confuse this source of ²²Ne with neon-E, which is also rich in ²²Ne.

Neon data for the carbonaceous chondrite Mokoia show that the end member composition of neon-Si in meteorites is ²⁰Ne/²²Ne = 13.7, the same as the present solar wind. The solar wind composition evidently has remained constant since before the compaction of Mokoia.

Ca, Al-rich inclusions from the Allende meteorite were examined for correlation between neon-E and oxygen or magnesium isotopic anomalies. ²²Ne and ³⁶Ar enrichments found in some inclusions are attributed to cosmic- ray-induced reactions on Na and Cl, not to a primordial component. Neon-E is not detectably enriched in Allende.

Measurements were made to determine the noble gas contents of various terrestrial rocks and minerals, and to investigate the cycling of noble gases between different terrestrial reservoirs. Beryl crystals contain a characteristic suite of magmatic gases including nucleogenic ²¹Ne and ²²Ne from (α,n) reactions, radiogenic ⁴⁰Ar, and fissiogenic ^131-136Xe from the decay of K and U in the continental crust. Significant concentrations of atmospheric noble gases are also present in beryl.

Both juvenile and atmospheric noble gases are found in rocks from the Skaergaard intrusion. The ratio ⁴⁰Ar/³⁶Ar (corrected for in situ decay of ⁴⁰K) correlates with δ¹⁸O in plagioclase. Atmospheric argon has been introduced into samples that have experienced oxygen-isotope exchange with circulating meteoric hydrothermal fluids. Unexchanged samples contain juvenile argon with ⁴⁰Ar/³⁶Ar greater than 6000 that was trapped from the Skaergaard magma.

Juvenile and atmospheric gases have been measured in the glassy rims of mid-ocean ridge (MOR) pillow basalts. Evidence is presented that three samples contain excess radiogenic ¹²⁹Xe and fission xenon, in addition to the excess radiogenic ⁴⁰Ar found in all samples. These juvenile gases are being outgassed from the upper-mantle source region of the MOR magma. No isotopic evidence has been found here for juvenile primordial noble gases accompanying the juvenile radiogenic gases in the MOR glasses. Large argon isotopic variations in a single specimen provide a clear indication of the late-stage addition of atmospheric argon, probably from seawater.

The Skaergaard data demonstrate that atmospheric noble gases dissolved in ground water can be transferred into crustal rocks. Subduction of oceanic crust altered by seawater can transport atmospheric noble gases into the upper mantle. A substantial portion of the noble gases in mantle derived rocks may represent subducted gases, not a primordial component as is often assumed.

Thermodynamic and kinetic behavior of an argon plasma jet. Decomposition of nitric oxide between 1300 - 1750 degrees K in an argon plasma

In the first part of the study, an RF coupled, atmospheric pressure, laminar plasma jet of argon was investigated for thermodynamic equilibrium and some rate processes.

Improved values of transition probabilities for 17 lines of argon I were developed from known values for 7 lines. The effect of inhomogeneity of the source was pointed out.

The temperatures, T, and the electron densities, n_e , were determined spectroscopically from the population densities of the higher excited states assuming the Saha-Boltzmann relationship to be valid for these states. The axial velocities, v_z, were measured by tracing the paths of particles of boron nitride using a three-dimentional mapping technique. The above quantities varied in the following ranges: 10¹² ˂ n_e ˂ 10¹⁵ particles/cm³, 3500 ˂ T ˂ 11000 °K, and 200 ˂ v_z ˂ 1200 cm/sec.

The absence of excitation equilibrium for the lower excitation population including the ground state under certain conditions of T and n_e was established and the departure from equilibrium was examined quantitatively. The ground state was shown to be highly underpopulated for the decaying plasma.

Rates of recombination between electrons and ions were obtained by solving the steady-state equation of continuity for electrons. The observed rates were consistent with a dissociative-molecular ion mechanism with a steady-state assumption for the molecular ions.

In the second part of the study, decomposition of NO was studied in the plasma at lower temperatures. The mole fractions of NO denoted by x_NO were determined gas-chromatographically and varied between 0.0012 ˂ x_NO ˂ 0.0055. The temperatures were measured pyrometrically and varied between 1300 ˂ T ˂ 1750°K. The observed rates of decomposition were orders of magnitude greater than those obtained by the previous workers under purely thermal reaction conditions. The overall activation energy was about 9 kcal/g mol which was considerably lower than the value under thermal conditions. The effect of excess nitrogen was to reduce the rate of decomposition of NO and to increase the order of the reaction with respect to NO from 1.33 to 1.85. The observed rates were consistent with a chain mechanism in which atomic nitrogen and oxygen act as chain carriers. The increased rates of decomposition and the reduced activation energy in the presence of the plasma could be explained on the basis of the observed large amount of atomic nitrogen which was probably formed as the result of reactions between excited atoms and ions of argon and the molecular nitrogen.

An investigation of the reaction negative K¯p → K¯π⁺ at P_(lab) = 2 Gev/c

The reaction K^-p→K^-π⁺n has been studied for incident kaon momenta of 2.0 GeV/c. A sample of 19,881 events was obtained by a measurement of film taken as part of the K-63 experiment in the Berkeley 72 inch bubble chamber.

Based upon our analysis, we have reached four conclusions. (1) The magnitude of the extrapolated Kπ cross section differs by a factor of 2 from the P-wave unitarity prediction and the K⁺n results; this is probably due to absorptive effects. (2) Fits to the moments yield precise values for the Kπ S-wave which agree with other recent statistically accurate experiments. (3) An anomalous peak is present in our backward K^-p→(π+n) K^- u-distribution. (4) We find a non-linear enhancement due to interference similiar to the one found by Bland et al. (Bland 1966).

Inelastic K+p reactions at incident momenta from 1.37 GeV/c to 2.17 GeV/c

A number of recent experiments have suggested the possibility of a highly inelastic resonance in K⁺p scattering. To study the inelastic K⁺p reactions, a 400 K exposure has been taken at the L.R.L. 25 inch bubble chamber. The data are spread over seven K⁺ momenta between 1.37 and 2.17 GeV/c.

Cross-sections have been measured for the reaction K⁺p → pK°π+ which is dominated by the quasi-two body channels K∆ and K*N. Both these channels are strongly peripheral, as at other momenta. The decay of the ∆ is in good agreement with the predictions of the rho-photon analogy of Stodolsky and Sakurai. The data on the K*p channel show evidence of both pseudo scalar and vector exchange.

Cross-sections for the final state pK⁺π+π- shows a strong contribution from the quasi-two body channel K*∆. This reaction is also very peripheral even at threshold. The decay angular distributions indicate the reaction is dominated as at higher momenta by a pion exchange mechanism. The data are also in good agreement with the quark model predictions of Bialas and Zalewski for the K* and ∆ decay.

CP and the three pion decay of the K°

The time distribution of the decays of an initially pure K° beam into π+π-π° has been analyzed to determine the complex parameter W (also known as Ƞ^+-° and (x + iy)). The K° beam was produced in a brass target by the interactions of a 2.85 GeV/c π- beam which was generated on an internal target in the Lawrence Radiation Laboratory (LRL) Bevatron. The counters and hodoscopes in the apparatus selected for events with a neutral (K°) produced in the brass target, two charged secondaries passing through a magnet spectrometer and a ɣ-ray shower in a shower hodoscope.

From the 275K apparatus triggers, 148 K → π+π-π° events were isolated. The presence of a ɣ-ray shower in the optical shower chambers and a two-prong vee in the optical spark chambers were devices used to isolate the events. The backgrounds were further reduced by reconstructing the momenta of the two charged secondaries and applying kinematic constraints.

The best fit to the final sample of 148 events distributed between .3 and 7.0 K_S lifetimes gives:

ReW = -.05 ±.17

ImW = +.39 +.35/-.37

This result is consistent with both CPT invariance (ReW = 0) and CP invariance (W = 0). Backgrounds are estimated to be less than 10% and systematic effects have also been estimated to be negligible.

An analysis of the present data on CP violation in this decay mode and other K° decay modes has estimated the phase of ɛ to be 45.3 ± 2.3 degrees. This result is consistent with the super weak theories of CP violation which predicts the phase of ɛ to be 43°. This estimate is in turn used to predict the phase of Ƞ°° to be 48.0 ± 7.9 degrees. This is a substantial improvement on presently available measurements. The largest error in this analysis comes from the present limits on W from the world average of recent experiments. The K → πuʋ mode produces the next largest error. Therefore further experimentation in these modes would be useful.

Qualidade do ar e atendimentos médicos de emergência por sintomas respiratórios em crianças residentes em Jacarepaguá, Rio de Janeiro

Apesar da cidade do Rio de Janeiro ser uma das mais importantes metrópoles brasileiras são muito pouco conhecidos os efeitos da exposição aos poluentes atmosféricos na saúde da população carioca. Este trabalho foi idealizado para suprir uma parte desta carência. Os poluentes investigados foram PM10, SO2, NO2, CO e O3 e os desfechos envolveram os atendimentos pediátricos de emergência por sintomas respiratórios em três unidades públicas de saúde de Jacarepaguá, entre abril de 2002 e março de 2003. As variáveis de confusão foram a tendência temporal, sazonalidade, temperatura, umidade relativa do ar, precipitação de chuva e infecções respiratórias. Também foram ajustados os efeitos do calendário, isto é, determinados dias do ano que apresentaram comportamentos anormais como feriados e finais de semana. Houve inúmeras falhas no monitoramento de todos os poluentes e devido ao reduzido volume de dados, optou-se por não incluir o SO2 nas análises. Uma vez que os determinantes e as conseqüências clínicas das exposições aos poluentes atmosféricos são bastante distintos nas vias aérias superiores e nas vias aéreas inferiores, um dos estudos verificou a associação dos poluentes do ar com transtornos nestes dois segmentos. Embora de pequena magnitude, somente o O3 apresentou resultado positivo e estatisticamente significativo, tanto com todos os atendimentos de emergência por queixas respiratórias como com os atendimentos motivados por sintomas nas vias aéreas inferiores. O efeito foi no mesmo dia da exposição (lag 0). No outro estudo, investigou-se a associação dos poluentes do ar com os atendimentos de emergência por sintomas de obstrução brônquica. Neste caso, as crianças foram categorizadads em três faixas etárias. Somente as crianças com idades menores que 2 anos tiveram um resultado positivo e estatisticamente significativo, de expressiva magnitude com PM10. Semelhante efeito foi visto com o O3, embora com significado estatístico limítrofe (p<0,06). Também neste estudo o efeito ocorreu no mesmo dia da exposição. Apesar das falhas no monitoramento, nos dois estudos, os parâmetros da poluição ambiental estiveram associados ao aumento do número de atendimentos pediátricos de emergência por motivos respiratórios em Jacarepaguá. Durante o período de estudos, os níveis de todos os poluentes monitorados permaneceram abaixo dos limites recomendados.

Impacto das motocicletas na qualidade do ar das grandes cidades

O crescimento do número de motocicletas nas grandes cidades, em função de fatores como o baixo custo e a alta mobilidade nos centros urbanos, tem sido considerado um importante fator de deterioração da qualidade do ar. Nesse contexto, o monitoramento das emissões gasosas provenientes do escapamento desses veículos é fundamental para o conhecimento da contribuição dessa classe de transporte no agravamento da poluição atmosférica. A partir dessas informações tornam-se possíveis o monitoramento e o controle da qualidade do ar. Para tanto, amostras das emissões de diferentes motocicletas foram coletadas, por meio de dinamômetro, e analisadas por cromatografia gasosa. As emissões das motocicletas foram utilizadas em conjunto com dados meteorológicos utilizando o modelo de trajetória OZIPR e o mecanismo químico SAPRC para demonstrar o impacto na formação do ozônio troposférico na região. As simulações indicam que a concentração de ozônio na troposfera poderá ultrapassar o padrão nacional estabelecido pela Resolução CONAMA 03/90 em até três anos. Além disso, acrescenta-se que as taxas de emissões de compostos legislados emitidos pelas motocicletas utilizadas neste estudo (HC, CO e NOx) já atendem aos níveis preconizados em todas as fases do PROMOT. Assim, além da adoção do PROMOT, se fazem necessárias medidas adicionais para o gerenciamento da emissão de poluentes provindos de fontes móveis. A alteração do tipo de combustível ou até mesmo da fonte de energia, elétrica, por exemplo, seria uma alternativa para o controle da poluição atmosférica

Charge and spin transport in graphene devices

170 p.

Control de vuelo de un cuadricóptero AR-Drone

[ES]En este TFG se obtendrá un algoritmo de generación de trayectorias para el cuadricóptero AR-Drone capaz de conseguir trazados lo más rápidos posibles teniendo en cuenta la dinámica del modelo y las limitaciones del entorno. Así mismo se propondrá un control primitivo para la detección de obstáculos. Mediante las comunicaciones con el cuadricóptero y el control de los parámetros característicos del medio, se establecerá usando el lenguaje C# los bucles de programación necesarios para discriminar todas las trayectorias desfavorables y obtener una que se adecue a nuestros criterios.

Reprodução de peixes de riachos: uma abordagem comparativa entre as estratégias r e K

No presente trabalho, objetivou-se caracterizar a estratégia reprodutiva, enfatizando o investimento energético, de duas espécies de peixe do rio Ubatiba, Maricá, Rio de Janeiro: Parotocinclus maculicauda (K-estrategista) e Astyanax hastatus (r-estrategista). Foram realizadas coletas bimestrais de Junho de 2010 a Abril de 2011 totalizando 236 exemplares amostrados de A. hastatus e 234 de P. maculicauda. Para cada exemplar foram registrados os dados de comprimento padrão (Cp, cm), peso total (Pt, g), peso gonadal (Pg, g), sexo e estádio de maturação. Através da estrutura de tamanho, observamos que as fêmeas atingem maior comprimento, em relação aos machos, para as duas espécies. A relação peso/ comprimento evidenciou para ambas as espécies, crescimento alométrico negativo (inferior a 3), demonstrando crescimento mais longelíneo. Para a proporção sexual, o teste χ2 foi aplicado e indicou que, para as duas espécies, há significativamente mais fêmeas. A distribuição sexual no ano mostrou que as fêmeas se mantêm em maioria durante todo o ano para P. maculicauda. Para A. hastatus este padrão também se mantém, porém com exceção do bimestre Novembro/Dezembro, quando o número de machos torna-se um pouco maior. O tamanho de primeira maturação mostrou-se o mesmo para ambas as espécies (2,5 a 3,0 cm). A variação temporal da freqüência de indivíduos reprodutivos e não reprodutivos juntamente com a distribuição temporal dos valores individuais de IGS mostrou que P. maculicauda se reproduz com maior intensidade nas estações chuvosas (Setembro a Abril), reduzindo sua atividade reprodutiva de maneira significativa nas estações secas (Maio a Agosto). Já A. hastatus demonstrou regular atividade reprodutiva durante todo o ano com pequeno pico no bimestre Novembro/ Dezembro. Desova do tipo total foi registrada para Astyanax, enquanto que para Parotocinclus registrou-se desova parcelada em três lotes. Em ambas as espécies foi observada relação inversa entre volume e a quantidade de ovócitos produzidos, com A. hastatus produzindo muitos ovócitos (fecundidade: 463 + 213 ovócitos/grama de peixe) de reduzido volume (diâmetro = 800 μm e volume = 0,26 mm3) e P. maculicauda produzindo número bem inferior (fecundidade: 47 + 13 ovócitos/grama de peixe), porém com volume superior (diâmetro = 1.600 μm e volume = 2,14 mm3). Com isso o valor energético relativo também se mostrou superior, com A. hastaus produzindo ovócitos vitelogênicos com 0,4+ 0,08 cal/unidade e P. maculicauda produzindo os mesmos ovócitos com 1,8+ 1,1 cal/unidade. Para a produção energética total investida na produção de gametas, foi considerado o tipo de desova de cada espécie, com Astyanax investindo 50,5 + 24 calorias/grama/grama de peixe e Parotocinclus investindo 88,4 + 72,46 cal/grama/grama de peixe, porém sem diferenças significativas (Mann-Whitney; U =235,0, p=0,08), indicando, portanto que independente da estratégia adotada (r ou K), o gasto energético na produção de ovócitos é a mesma.