9,069 research outputs found

    Reactions of iron and nickel alloy droplets with gases

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    Bosonic and fermionic Weinberg-Joos (j,0)+ (0,j) states of arbitrary spins as Lorentz-tensors or tensor-spinors and second order theory

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    We propose a general method for the description of arbitrary single spin-j states transforming according to (j,0)+(0,j) carrier spaces of the Lorentz algebra in terms of Lorentz-tensors for bosons, and tensor-spinors for fermions, and by means of second order Lagrangians. The method allows to avoid the cumbersome matrix calculus and higher \partial^{2j} order wave equations inherent to the Weinberg-Joos approach. We start with reducible Lorentz-tensor (tensor-spinor) representation spaces hosting one sole (j,0)+(0,j) irreducible sector and design there a representation reduction algorithm based on one of the Casimir invariants of the Lorentz algebra. This algorithm allows us to separate neatly the pure spin-j sector of interest from the rest, while preserving the separate Lorentz- and Dirac indexes. However, the Lorentz invariants are momentum independent and do not provide wave equations. Genuine wave equations are obtained by conditioning the Lorentz-tensors under consideration to satisfy the Klein-Gordon equation. In so doing, one always ends up with wave equations and associated Lagrangians that are second order in the momenta. Specifically, a spin-3/2 particle transforming as (3/2,0)+ (0,3/2) is comfortably described by a second order Lagrangian in the basis of the totally antisymmetric Lorentz tensor-spinor of second rank, \Psi_[ \mu\nu]. Moreover, the particle is shown to propagate causally within an electromagnetic background. In our study of (3/2,0)+(0,3/2) as part of \Psi_[\mu\nu] we reproduce the electromagnetic multipole moments known from the Weinberg-Joos theory. We also find a Compton differential cross section that satisfies unitarity in forward direction. The suggested tensor calculus presents itself very computer friendly with respect to the symbolic software FeynCalc.Comment: LaTex 34 pages, 1 table, 8 figures. arXiv admin note: text overlap with arXiv:1312.581

    Tracing the magnetic field of IRDC G028.23-00.19 using NIR polarimetry

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    The importance of the magnetic (B) field in the formation of infrared dark clouds (IRDCs) and massive stars is an ongoing topic of investigation. We studied the plane-of-sky B field for one IRDC, G028.23-00.19, to understand the interaction between the field and the cloud. We used near-IR background starlight polarimetry to probe the B field and performed several observational tests to assess the field importance. The polarimetric data, taken with the Mimir instrument, consisted of H-band and K-band observations, totaling 17,160 stellar measurements. We traced the plane-of-sky B-field morphology with respect to the sky-projected cloud elongation. We also found the relationship between the estimated B-field strength and gas volume density, and we computed estimates of the normalized mass-to-magnetic flux ratio. The B-field orientation with respect to the cloud did not show a preferred alignment, but it did exhibit a large-scale pattern. The plane-of-sky B-field strengths ranged from 10 to 165 ÎŒG, and the B-field strength dependence on density followed a power law with an index consistent with 2/3. The mass-to-magnetic flux ratio also increased as a function of density. The relative orientations and relationship between the B field and density imply that the B field was not dynamically important in the formation of the IRDC. The increase in mass-to-flux ratio as a function of density, though, indicates a dynamically important B field. Therefore, it is unclear whether the B field influenced the formation of G28.23. However, it is likely that the presence of the IRDC changed the local B-field morphology.We thank J. Montgomery, T. Hogge, and I. Stephens for constructive discussions on the analysis. We are grateful to R. Crutcher for permission to include his Zeeman data. This research was conducted in part using the Mimir instrument, jointly developed at Boston University and Lowell Observatory and supported by NASA, NSF, and the W.M. Keck Foundation. This research made use of the NASA/IPAC Infrared Science Archive, which is operated by the Jet Propulsion Laboratory, California Institute of Technology (Caltech), under contract with NASA. This publication made use of data products from the Two Micron All Sky Survey, which was a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/Caltech, funded by NASA and NSF. This work is based in part on data obtained as part of the UKIRT Infrared Deep Sky Survey. The ATLAS-GAL project is a collaboration between the Max-PlanckGesellschaft, the European Southern Observatory (ESO), and the Universidad de Chile. It includes projects E-181.C-0885, E-078.F-9040(A), M-079.C-9501(A), M-081.C-9501(A), and Chilean data. This publication makes use of molecular line data from the Boston University-FCRAO Galactic Ring Survey (GRS). The GRS is a joint project of Boston University and Five College Radio Astronomy Observatory, funded by the National Science Foundation under grants AST-9800334, 0098562, 0100793, 0228993, and. 0507657. A.E.G. acknowledges support from FONDECYT 3150570. This work was supported under NSF grants AST 09-07790 and 14-12269 and NASA grant NNX15AE51G to Boston University. We thank the anonymous referee for valuable feedback, which improved the quality of this work. (NASA; NSF; W.M. Keck Foundation; E-181.C-0885 - Max-Planck-Gesellschaft; E-078.F-9040(A) - Max-Planck-Gesellschaft; M-079.C-9501(A) - Max-Planck-Gesellschaft; M-081.C-9501(A) - Max-Planck-Gesellschaft; E-181.C-0885 - European Southern Observatory (ESO); E-078.F-9040(A) - European Southern Observatory (ESO); M-079.C-9501(A) - European Southern Observatory (ESO); M-081.C-9501(A) - European Southern Observatory (ESO); E-181.C-0885 - Universidad de Chile; E-078.F-9040(A) - Universidad de Chile; M-079.C-9501(A) - Universidad de Chile; M-081.C-9501(A) - Universidad de Chile; AST-9800334 - National Science Foundation; 0098562 - National Science Foundation; 0100793 - National Science Foundation; 0228993 - National Science Foundation; 0507657 - National Science Foundation; 3150570 - FONDECYT; AST 09-07790 - NSF; 14-12269 - NSF; NNX15AE51G - NASA

    The political organization of sugarcane production in Western Mexico

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    The strike of CNC sugarcane producers and the immediate response by the refinery administration are a good example of the ongoing political negotiations between the main actors involved in the organization of sugarcane production in the Valley of AutlĂĄn-El Grullo. I introduced in Chapter I the protagonists of sugarcane production participating in the social drama of confrontation and negotiation. I have described in Chapters 3, 4 and 5 the socio-economic conditions in which local peasants and farmers have evolved their decision to grow sugarcane. These social actors disclosed a wide range of skills and acute understanding of social institutions. This holds true among all producers from the smallest to the largest. The ways in which these different actors have got involved in sugarcane production defy the images of powerless reactive peasants and farmers that abound in the social analyses on Mexico.Sugarcane producers in the valley successfully lobbied the Mexican Government to attract public investment into the region, which arrived as a sugar refinery with the financial resources to build access roads and improve the conditions of the irrigation canals which had been neglected. The reconstruction of how these peasants and farmers brought to the region public investment to build a refinery and how they have developed, with the encouragement of the refinery, their own organizations to deal with the refinery administration, was covered in Chapter 6. In Chapter 7, the last chapter, I have closed the circle with a description of a negotiation between producers and refinery administration which reached a satisfactory agreement to all parts involved, this negotiation highlights the shifting alliances and interests among participants.The methodological approach to the subjects of study was a down-up actor- oriented approach. Although I would not claim I was a tabula rasa when I started the research I would certainly emphasise that this approach allowed me to immerse myself in the different individual perspectives which were, in spite of their contradictions, complementary to grasp the ethos of the organization of sugarcane production in the region. The individual cases illustrated their complex structuring of institutional arrangements. As North (1993) describes, individual decision-making follows guides provided by the institutions which shape human interaction in historically contexts. These structures provide social actors with incentives and guidance in the political, social and economic arenas which they apply and develop in their organizations. Sugarcane producers assume institutional constrains to diminish the uncertainty in their everyday life. On the one hand their participation in local economic and political organizations have repercussions beyond their region as on the other the national organizations impinge on their activities. My study has focused on the ways how these different levels of political and economic organization at national and local level are brought together by the social actors involved in sugarcane production.Some of these local peasants and farmers participated in the initial negotiations to bring the refinery into the valley, others had to be lured to grow sugarcane. Their decision-making, in contrast with sugarcane producers in other regions, was based on the pursue of their own interest. As I described in Chapter 2, this was possible because they could make their decision when the state direct intervention in sugarcane production was trying to boost a steady supply of sugar for the domestic market; after several private refinery owners had gone into bankruptcy precipitating the crisis of sugar production at the end of the 1960s (Purcell, 1981: 224-225). These national conditions provided local peasants and farmers with room for manoeuvre. They could join forces with sugarcane producers in other regions and ask for better terms of production. Thus, they did not have to overturn archaic structures of exploitation as sugarcane producers in other regions in Mexico did (see Ronfeldt, 1975). These conditions were propitious for an organization of production where all the parts involved may have an equal participation. However, these propitious conditions only provide the institutional arena where social actors have to negotiate and implement the agreed plans for the organization of production. In other regions, sugarcane producers have not been able to seize as much control over production as the producers in the Valley of AutlĂĄn-El Grullo.The possible explanations to the type of organization of production agreed by sugarcane producers and refinery administrators in the valley have to be extracted from the specific historical conditions in which these social actors were immersed and how they not only rely on the hegemonic social, economic and political institutions but transform them to fulfil their need and aspirations. In the case of local peasants and farmers, they have learned how to deal with the dominant political party, which pervades in a corporatist way the negotiations between the governmental institutions and the civil society (see Jessop, 1990). Each local peasant or farmer has found a way to deal with the refinery employees. As I discussed in Chapter 7, the refinery administrators have a different agenda to the producers, they look up to the national echelons of public administration, which is their line of command and where they would like to secure a place. These administrators have to reconcile the producers' demands with the national policies they have to implement and their careers, which is an extremely difficult task.However all parts involved in the organization of production seemed to have been able to work out a modusvivendi where they have conciliated their differences and run efficiently the organization of production in the Valley of AutlĂĄn-EI Grullo, which made the refinery Melchor Ocampo one of the most efficient in the country. As it was transparent in most comments, this was not achieved easily but the results have been worthwhile the effort. And these results provide an example of a successful cooperation between public administrators and local producers.The sound financial record and good level of productivity made this refinery an attractive investment when the privatising wave reached the sugar refineries in the early 1990s. As it could have been expected, the Ingenio Melchor Ocampo was one of the first refineries to be sold to CNC. How this change of ownership has affected all parts involved in the organization of sugarcane production in the valley must be assessed in a re-study

    Shape evolution and shape coexistence in Pt isotopes: comparing interacting boson model configuration mixing and Gogny mean-field energy surfaces

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    The evolution of the total energy surface and the nuclear shape in the isotopic chain 172−194^{172-194}Pt are studied in the framework of the interacting boson model, including configuration mixing. The results are compared with a self-consistent Hartree-Fock-Bogoliubov calculation using the Gogny-D1S interaction and a good agreement between both approaches shows up. The evolution of the deformation parameters points towards the presence of two different coexisting configurations in the region 176 ≀\leq A ≀\leq 186.Comment: Submitted to PR

    PAH Formation in O-rich Planetary Nebulae

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    Polycyclic aromatic hydrocarbons (PAHs) have been observed in O-rich planetary nebulae towards the Galactic Bulge. This combination of oxygen-rich and carbon-rich material, known as dual-dust or mixed chemistry, is not expected to be seen around such objects. We recently proposed that PAHs could be formed from the photodissociation of CO in dense tori. In this work, using VISIR/VLT, we spatially resolved the emission of the PAH bands and ionised emission from the [SIV] line, confirming the presence of dense central tori in all the observed O-rich objects. Furthermore, we show that for most of the objects, PAHs are located at the outer edge of these dense/compact tori, while the ionised material is mostly present in the inner parts of these tori, consistent with our hypothesis for the formation of PAHs in these systems. The presence of a dense torus has been strongly associated with the action of a central binary star and, as such, the rich chemistry seen in these regions may also be related to the formation of exoplanets in post-common-envelope binary systems.Comment: 14, accepted for publication in the MNRAS Journa

    Dependence of the Fundamental Plane Scatter on Galaxy Age

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    The fundamental plane (FP) has an intrinsic scatter that can not be explained purely by observational errors. Using recently available age estimates for nearby early type galaxies, we show that a galaxy's position relative to the FP depends on its age. In particular, the mean FP corresponds to ellipticals with an age of ~10 Gyr. Younger galaxies are systematically brighter with higher surface brightness relative to the mean relation. Old ellipticals form an `upper envelope' to the FP. For our sample of mostly non-cluster galaxies, age can account for almost half of the scatter in the B band FP. Distance determinations based on the FP may have a systematic bias, if the mean age of the sample varies with redshift. We also show that fundamental plane residuals, B-V colors and Mg_2 line strength are consistent with an ageing central burst superposed on an old stellar population. This reinforces the view that these age estimates are tracing the last major episode of star formation induced by a gaseous merger event. We briefly discuss the empirical `evolutionary tracks' of merger-remnants and young ellipticals in terms of their key observational parameters.Comment: 14 pages, Latex, 2 figures, accepted by ApJ Letter

    The bias-extension test for the analysis of in-plane shear properties of textile composite reinforcements and prepregs: a review

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    The bias-extension test is a rather simple experiment aiming to determine in-plane shear properties of textile composite reinforcements. However the mechanics during the test involves fibrous material at large shear strains and large rotations of the fibres. Several aspects are still being studied and are not yet modeled in a consensual manner. The standard analysis of the test is based on two assumptions: inextensibility of the fibers and rotations at the yarn crossovers without slippage. They lead to the development of zones with constant fibre orientations proper to the bias-extension test. Beyond the analysis of the test within these basic assumptions, the paper presents studies that have been carried out on the lack of verification of these hypothesis (slippage, tension in the yarns, effects of fibre bending). The effects of temperature, mesoscopic modeling and tension locking are also considered in the case of the bias-extension test

    Trade-offs Between Water Transport Capacity and Drought Resistance in Neotropical Canopy Liana and Tree Species

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    In tropical forest canopies, it is critical for upper shoots to efficiently provide water to leaves for physiological function while safely preventing loss of hydraulic conductivity due to cavitation during periods of soil water deficit or high evaporative demand. We compared hydraulic physiology of upper canopy trees and lianas in a seasonally dry tropical forest to test whether trade-offs between safety and efficiency of water transport shape differences in hydraulic function between these two major tropical woody growth forms. We found that lianas showed greater maximum stem-specific hydraulic conductivity than trees, but lost hydraulic conductivity at less negative water potentials than trees, resulting in a negative correlation and trade-off between safety and efficiency of water transport. Lianas also exhibited greater diurnal changes in leaf water potential than trees. The magnitude of diurnal water potential change was negatively correlated with sapwood capacitance, indicating that lianas are highly reliant on conducting capability to maintain leaf water status, whereas trees relied more on stored water in stems to maintain leaf water status. Leaf nitrogen concentration was related to maximum leaf-specific hydraulic conductivity only for lianas suggesting that greater water transport capacity is more tied to leaf processes in lianas compared to trees. Our results are consistent with a trade-off between safety and efficiency of water transport and may have implications for increasing liana abundance in neotropical forests
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