Estudi medi ambiental del centre de mecanitzat Kondia HS1000 quan s'utilitza com a màquina d'ISF

Aproximadament deu anys enrere, es va començar a desenvolupar un nou procés industrial de deformació de xapa anomenat conformació incremental de xapa, Incremental Sheet Forming (ISF) en anglès. En aquest procés, una làmina de xapa és subjectada per un suport i conformada per una eina que normalment és un punxó amb punta semiesfèrica que es mou segons les directrius d’un software de control numèric. Aquest moviment de l’eina es fa en el pla, i un cop ja s’ha realitzat un contorn, l’eina baixa per realitzar-ne un altre i així successivament fins a la realització de la peça desitjada. Aquest procés de conformat de xapa està considerat com una alternativa al procés d’embotició, i la seva principal avantatge és que es pot considerar una gran alternativa al procés d’embotició per a la fabricació de petits lots de producte. La diferència més destacable és que en el procés de conformació incremental de xapa no es necessiten grans matrius ni punxons, que són molt costosos ja que han de garantir unes precisions molt elevades. A l’actualitat, aquest sistema encara es troba en fase d’investigació, no hi ha estudis definitius que aportin resultats fiables sobre la viabilitat del procés en aplicacions industrials, però cada vegada hi ha més equips de treball universitaris que es dediquen a estudiar-lo i més empreses que l’estan introduint en els seus departaments de I+D per tal d’adaptar els seus processos de fabricació a aquesta nova tecnologia. Un dels equips de treball que estan investigant aquest procés es el Grup de Recerca d’Enginyeria de Producte, Procés i Producció (GREP) situat al parc científic i tecnològic de l’Universitat de Girona. Disposen d’un centre de mecanitzat CNC de la marca Kondia model HS1000 que actualment es troba en període d’adaptació per tal de desenvolupar una màquina híbrida en la qual es duran a terme processos de conformació de xapa i sinterització per làser. Per tal d’adaptar la màquina, una part dels estudis que s’han de realitzar és la investigació sobre el consum i emissions de CO2 generades durant el procés de fabricació. Així doncs, aquest projecte final de carrera és aquest estudi de forma experimental i teòrica sobre el consum energètic del centre de mecanitzat, quan s’utilitza amb la tècnica de Incremental Sheet Forming (ISF). Es pretén estudiar el consum energètic de la tecnologia tenint en compte paràmetres de procés com ara el material, geometries, energia elèctrica consumida i programació de la trajectòria de l’eina, paràmetres relacionats amb l’origen de l’energia i aspectes relacionats amb els costos de producció

Disseny dels elements constitutius per adaptar un centre de mecanitzat de control numèric a la tecnologia Incremental Sheet Forming (ISF)

Un dels processos tradicionals de conformació de xapa més utilitzats a nivell industrial, degut a la seva rapidesa d’operació i la seva maduresa del procés, és l’embotició. Per a dur a terme aquest procés és necessària la construcció d’uns utillatges (matriu i punxó) per a cada tipus de producte. Aquests utillatges estan fabricats amb materials altament resistents ja que han de poder suportar càrregues molt importants durant la deformació. A més, s’han de garantir unes precisions dimensionals molt bones per tal d’evitar el xoc entre les dues parts de l’utillatge i per a assegurar que la peça obtinguda tingui les dimensions desitjades. Aquest fet implica que el procés d’obtenció de les matrius i punxons tingui un cost molt elevat i per a amortitzar-lo és necessari que la producció sigui en massa.L’objecte d’aquest projecte és adaptar el centre de mecanitzat Kondia HS1000 per tal de poder dur a terme recerca bàsica de la tecnologia de conformat incremental de xapa (ISF) en el Grup de Recerca en Enginyeria del Producte, Procés i Producció (GREP)

La Federación Internacional del Deporte Escolar (ISF).

Resumen del autor. Resumen en castellano e inglés. Este artículo se incluye en el monográfico 'Educación y Deporte'

Disseny dels elements constitutius per adaptar un centre de mecanitzat de control numèric a la tecnologia Incremental Sheet Forming (ISF)

Un dels processos tradicionals de conformació de xapa més utilitzats a nivell industrial, degut a la seva rapidesa d’operació i la seva maduresa del procés, és l’embotició. Per a dur a terme aquest procés és necessària la construcció d’uns utillatges (matriu i punxó) per a cada tipus de producte. Aquests utillatges estan fabricats amb materials altament resistents ja que han de poder suportar càrregues molt importants durant la deformació. A més, s’han de garantir unes precisions dimensionals molt bones per tal d’evitar el xoc entre les dues parts de l’utillatge i per a assegurar que la peça obtinguda tingui les dimensions desitjades. Aquest fet implica que el procés d’obtenció de les matrius i punxons tingui un cost molt elevat i per a amortitzar-lo és necessari que la producció sigui en massa.L’objecte d’aquest projecte és adaptar el centre de mecanitzat Kondia HS1000 per tal de poder dur a terme recerca bàsica de la tecnologia de conformat incremental de xapa (ISF) en el Grup de Recerca en Enginyeria del Producte, Procés i Producció (GREP)

Microstructures of ISF sinters in air

The microstructures of industrial ISF and synthetic sinters were examined. The principle phases present were found to consist of zincite, spinel and glass. The morphologies of the zincite phase in these complex multiphase materials were shown to relate directly to the bulk chemical compositions and thermal histories of the sinters. The conditions favouring the formation of plate-like zincite, essential for the development of refractory networks in the ISF sinters, were identified. The proportion of framework zincite present in the sinters was found to increase with increasing peak bed temperature and an increasing CaO/SiO2 ratio. The aspect ratio of the zincite increases by increasing iron in the solid solution in zincite.

Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars IV. Two bulge populations

Based on high-resolution (R approximate to 42 000 to 48 000) and high signal-to-noise (S/N approximate to 50 to 150) spectra obtained with UVES/VLT, we present detailed elemental abundances (O, Na, Mg, Al, Si, Ca, Ti, Cr, Fe, Ni, Zn, Y, and Ba) and stellar ages for 12 new microlensed dwarf and subgiant stars in the Galactic bulge. Including previous microlensing events, the sample of homogeneously analysed bulge dwarfs has now grown to 26. The analysis is based on equivalent width measurements and standard 1-D LTE MARCS model stellar atmospheres. We also present NLTE Li abundances based on line synthesis of the (7)Li line at 670.8 nm. The results from the 26 microlensed dwarf and subgiant stars show that the bulge metallicity distribution (MDF) is double-peaked; one peak at [Fe/H] approximate to -0.6 and one at [Fe/H] approximate to +0.3, and with a dearth of stars around solar metallicity. This is in contrast to the MDF derived from red giants in Baade's window, which peaks at this exact value. A simple significance test shows that it is extremely unlikely to have such a gap in the microlensed dwarf star MDF if the dwarf stars are drawn from the giant star MDF. To resolve this issue we discuss several possibilities, but we can not settle on a conclusive solution for the observed differences. We further find that the metal-poor bulge dwarf stars are predominantly old with ages greater than 10 Gyr, while the metal-rich bulge dwarf stars show a wide range of ages. The metal-poor bulge sample is very similar to the Galactic thick disk in terms of average metallicity, elemental abundance trends, and stellar ages. Speculatively, the metal-rich bulge population might be the manifestation of the inner thin disk. If so, the two bulge populations could support the recent findings, based on kinematics, that there are no signatures of a classical bulge and that the Milky Way is a pure-disk galaxy. Also, recent claims of a flat IMF in the bulge based on the MDF of giant stars may have to be revised based on the MDF and abundance trends probed by our microlensed dwarf stars.

Transiting exoplanets from the CoRoT space mission XI. CoRoT-8b: a hot and dense sub-Saturn around a K1 dwarf

Aims. We report the discovery of CoRoT-8b, a dense small Saturn-class exoplanet that orbits a K1 dwarf in 6.2 days, and we derive its orbital parameters, mass, and radius. Methods. We analyzed two complementary data sets: the photometric transit curve of CoRoT-8b as measured by CoRoT and the radial velocity curve of CoRoT-8 as measured by the HARPS spectrometer**. Results. We find that CoRoT-8b is on a circular orbit with a semi-major axis of 0.063 +/- 0.001 AU. It has a radius of 0.57 +/- 0.02 R(J), a mass of 0.22 +/- 0.03 M(J), and therefore a mean density of 1.6 +/- 0.1 g cm(-3). Conclusions. With 67% of the size of Saturn and 72% of its mass, CoRoT-8b has a density comparable to that of Neptune (1.76 g cm(-3)). We estimate its content in heavy elements to be 47-63 M(circle plus), and the mass of its hydrogen-helium envelope to be 7-23 M(circle plus). At 0.063 AU, the thermal loss of hydrogen of CoRoT-8b should be no more than similar to 0.1% over an assumed integrated lifetime of 3 Ga.

Cold Nuclear Matter Effects on J/psi Yields as a Function of Rapidity and Nuclear Geometry in d plus A Collisions at root S(NN)=200 GeV

We present measurements of J/psi yields in d + Au collisions at root S(NN) = 200 GeV recorded by the PHENIX experiment and compare them with yields in p + p collisions at the same energy per nucleon-nucleon collision. The measurements cover a large kinematic range in J/psi rapidity (-2.2 < y < 2.4) with high statistical precision and are compared with two theoretical models: one with nuclear shadowing combined with final state breakup and one with coherent gluon saturation effects. In order to remove model dependent systematic uncertainties we also compare the data to a simple geometric model. The forward rapidity data are inconsistent with nuclear modifications that are linear or exponential in the density weighted longitudinal thickness, such as those from the final state breakup of the bound state.

Azimuthal correlations of electrons from heavy-flavor decay with hadrons in p plus p and Au plus Au collisions at root s(NN)=200 GeV

Measurements of electrons from the decay of open-heavy-flavor mesons have shown that the yields are suppressed in Au+Au collisions compared to expectations from binary-scaled p+p collisions. These measurements indicate that charm and bottom quarks interact with the hot dense matter produced in heavy-ion collisions much more than expected. Here we extend these studies to two-particle correlations where one particle is an electron from the decay of a heavy-flavor meson and the other is a charged hadron from either the decay of the heavy meson or from jet fragmentation. These measurements provide more detailed information about the interactions between heavy quarks and the matter, such as whether the modification of the away-side-jet shape seen in hadron-hadron correlations is present when the trigger particle is from heavy-meson decay and whether the overall level of away-side-jet suppression is consistent. We statistically subtract correlations of electrons arising from background sources from the inclusive electron-hadron correlations and obtain two-particle azimuthal correlations at root s(NN) = 200 GeV between electrons from heavy-flavor decay with charged hadrons in p+p and also first results in Au+Au collisions. We find the away-side-jet shape and yield to be modified in Au+Au collisions compared to p+p collisions.

Measurement of neutral mesons in p plus p collisions at root s=200 GeV and scaling properties of hadron production

The PHENIX experiment at the Relativistic Heavy Ion Collider has measured the invariant differential cross section for production of K(S)(0), omega, eta', and phi mesons in p + p collisions at root s 200 GeV. Measurements of omega and phi production in different decay channels give consistent results. New results for the omega are in agreement with previously published data and extend the measured p(T) coverage. The spectral shapes of all hadron transverse momentum distributions measured by PHENIX are well described by a Tsallis distribution functional form with only two parameters, n and T, determining the high-p(T) and characterizing the low-p(T) regions of the spectra, respectively. The values of these parameters are very similar for all analyzed meson spectra, but with a lower parameter T extracted for protons. The integrated invariant cross sections calculated from the fitted distributions are found to be consistent with existing measurements and with statistical model predictions.

Nuclear modification factors of phi mesons in d plus Au, Cu plus Cu, and Au plus Au collisions at root s(NN)=200 GeV

The PHENIX experiment at the Relativistic Heavy Ion Collider has performed systematic measurements of phi meson production in the K(+)K(-) decay channel at midrapidity in p + p, d + Au, Cu + Cu, and Au + Au collisions at root s(NN) = 200 GeV. Results are presented on the phi invariant yield and the nuclear modification factor R(AA) for Au + Au and Cu + Cu, and R(dA) for d + Au collisions, studied as a function of transverse momentum (1 < p(T) < 7 GeV/c) and centrality. In central and midcentral Au + Au collisions, the R(AA) of phi exhibits a suppression relative to expectations from binary scaled p + p results. The amount of suppression is smaller than that of the pi(0) and the. in the intermediate p(T) range (2-5 GeV/c), whereas, at higher p(T), the phi, pi(0), and. show similar suppression. The baryon (proton and antiproton) excess observed in central Au + Au collisions at intermediate p(T) is not observed for the phi meson despite the similar masses of the proton and the phi. This suggests that the excess is linked to the number of valence quarks in the hadron rather than its mass. The difference gradually disappears with decreasing centrality, and, for peripheral collisions, the R(AA) values for both particle species are consistent with binary scaling. Cu + Cu collisions show the same yield and suppression as Au + Au collisions for the same number of N(part). The R(dA) of phi shows no evidence for cold nuclear effects within uncertainties.

Cross Section and Parity-Violating Spin Asymmetries of W(+/-) Boson Production in Polarized p plus p Collisions at root s=500 Gev

Large parity-violating longitudinal single-spin asymmetries A(L)(e+) = 0.86(-0.14)(+0.30) and Ae(L)(e-) = 0.88(-0.71)(+0.12) are observed for inclusive high transverse momentum electrons and positrons in polarized p + p collisions at a center-of-mass energy of root s = 500 GeV with the PHENIX detector at RHIC. These e(+/-) come mainly from the decay of W(+/-) and Z(0) bosons, and their asymmetries directly demonstrate parity violation in the couplings of the W(+/-) to the light quarks. The observed electron and positron yields were used to estimate W(+/-) boson production cross sections for the e(+/-) channels of sigma(pp -> W(+)X) X BR(W(+) -> e(+) nu(e)) = 144.1 +/- 21.2(stat)(-10.3)(+3.4)(syst) +/- 21.6(norm) pb, and sigma(pp -> W(-)X) X BR(W(-) -> e(-) (nu) over bar (e)) = 3.17 +/- 12.1(stat)(-8.2)(+10.1)(syst) +/- 4.8(norm) pb.

Cross section and double helicity asymmetry for eta mesons and their comparison to pi(0) production in p plus p collisions at root s=200 GeV

Measurements of double-helicity asymmetries in inclusive hadron production in polarized p + p collisions are sensitive to helicity-dependent parton distribution functions, in particular, to the gluon helicity distribution, Delta g. This study focuses on the extraction of the double-helicity asymmetry in eta production ((p) over right arrow + (p) over right arrow -> eta + X), the eta cross section, and the eta/pi(0) cross section ratio. The cross section and ratio measurements provide essential input for the extraction of fragmentation functions that are needed to access the helicity-dependent parton distribution functions.

Measurement of transverse single-spin asymmetries for J/psi production in polarized p plus p collisions at root s=200 GeV

We report the first measurement of transverse single-spin asymmetries in J/psi production from transversely polarized p + p collisions at root s = 200 GeV with data taken by the PHENIX experiment in 2006 and 2008. The measurement was performed over the rapidity ranges 1.2 < vertical bar y vertical bar < 2.2 and vertical bar y vertical bar < 0.35 for transverse momenta up to 6 GeV/c. J/psi production at the Relativistic Heavy Ion Collider is dominated by processes involving initial-state gluons, and transverse single-spin asymmetries of the J/psi can provide access to gluon dynamics within the nucleon. Such asymmetries may also shed light on the long-standing question in QCD of the J/psi production mechanism. Asymmetries were obtained as a function of J/psi transverse momentum and Feynman-x, with a value of -0.086 +/- 0.026(stat) +/- 0.003(syst) in the forward region. This result suggests possible nonzero trigluon correlation functions in transversely polarized protons and, if well defined in this reaction, a nonzero gluon Sivers distribution function.

Azimuthal Anisotropy of pi(0) Production in Au plus Au Collisions at root s(NN)=200 GeV: Path-Length Dependence of Jet Quenching and the Role of Initial Geometry

We have measured the azimuthal anisotropy of pi(0) production for 1 < p(T) < 18 GeV/c for Au + Au collisions at root s(NN) = 200 GeV. The observed anisotropy shows a gradual decrease for 3 less than or similar to p(T) less than or similar to 7-10 GeV/c, but remains positive beyond 10 GeV/c. The magnitude of this anisotropy is underpredicted, up to at least similar to 10 GeV/c, by current perturbative QCD (PQCD) energy-loss model calculations. An estimate of the increase in anisotropy expected from initial-geometry modification due to gluon saturation effects and fluctuations is insufficient to account for this discrepancy. Calculations that implement a path-length dependence steeper than what is implied by current PQCD energy-loss models show reasonable agreement with the data.