936 resultados para Shlomo Ben Ami


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Conferencia: Diálogo y Paz en el Mediterráneo

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Para el desarrollo de esta monografía se tratará el tema de las armas nucleares con relación a diferentes países así: en el capítulo 1 Korea del Norte, en el capítulo 2 Israel, en el capítulo 3 China, en el capítulo 4 los países en desarrollo, en el capítulo 5 India y Pakistán

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El objetivo del presente estudio es analizar la forma en la que la prensa italiana de izquierdas construyó la imagen de palestinos e israelíes entre 1947 y 1957. La investigación se ha centrado en el estudio de los artículos publicados por algunos destacados periódicos de la época, con la finalidad de comprender cómo ha ido cambiando el lenguaje empleado por dichos órganos de prensa a la hora de referirse a los moradores de la tierra de Palestina. La tesis de este artículo es que dichos periódicos construyeron múltiples y contradictorias representaciones de judíos y palestinos, representaciones que no tenían nada que ver con la realidad de Oriente Medio, sino que obedecían a cuestiones ideológicas de carácter nacional e internacional (relaciones entre los partidos italianos y evolución de las dinámicas de la guerra fría).

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Correspondence with individuals: Jacob Ben-Ami, Ossip Dymow, Ovsei Liubomirskii, Kalman Marmor, Nachman Meisel, Melech Ravitch, Dov Sadan, Michael Weichert and Zalman Zylbercweig. Correspondence with organizations: Hebrew Actors' Union, IKUF, YIVO. Manuscripts of plays collected by Mestel as director, including adaptations by Mestel. Mestel's writings: manuscripts of poems, plays, essays, articles, notes, translations. Theater production materials: scripts with Mestel's direction notes, prop and set design notes. Miscellaneous theater materials, including course notes, theater programs. Clippings: Mestel's writings, biographical articles, reviews of performances. Family correspondence and personal papers including papers of Sara Kindman-Mestel. Photographs relating to Yiddish theater in New York, 1930s-1950s.

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A detailed study is presented of the expected performance of the ATLAS detector. The reconstruction of tracks, leptons, photons, missing energy and jets is investigated, together with the performance of b-tagging and the trigger. The physics potential for a variety of interesting physics processes, within the Standard Model and beyond, is examined. The study comprises a series of notes based on simulations of the detector and physics processes, with particular emphasis given to the data expected from the first years of operation of the LHC at CERN.

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PTF11iqb was initially classified as a TypeIIn event caught very early after explosion. It showed narrow Wolf-Rayet (WR) spectral features on day 2, but the narrow emission weakened quickly and the spectrum morphed to resemble those of Types II-L and II-P. At late times, Halpha emission exhibited a complex, multipeaked profile reminiscent of SN1998S. In terms of spectroscopic evolution, we find that PTF11iqb was a near twin of SN~1998S, although with weaker interaction with circumstellar material (CSM) at early times, and stronger CSM interaction at late times. We interpret the spectral changes as caused by early interaction with asymmetric CSM that is quickly (by day 20) enveloped by the expanding SN ejecta photosphere, but then revealed again after the end of the plateau when the photosphere recedes. The light curve can be matched with a simple model for weak CSM interaction added to the light curve of a normal SN~II-P. This plateau requires that the progenitor had an extended H envelope like a red supergiant, consistent with the slow progenitor wind speed indicated by narrow emission. The cool supergiant progenitor is significant because PTF11iqb showed WR features in its early spectrum --- meaning that the presence of such WR features in an early SN spectrum does not necessarily indicate a WR-like progenitor. [abridged] Overall, PTF11iqb bridges SNe~IIn with weaker pre-SN mass loss seen in SNe II-L and II-P, implying a continuum between these types.

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On 2011 May 31 UT a supernova (SN) exploded in the nearby galaxy M51 (the Whirlpool Galaxy). We discovered this event using small telescopes equipped with CCD cameras and also detected it with the Palomar Transient Factory survey, rapidly confirming it to be a Type II SN. Here, we present multi-color ultraviolet through infrared photometry which is used to calculate the bolometric luminosity and a series of spectra. Our early-time observations indicate that SN 2011dh resulted from the explosion of a relatively compact progenitor star. Rapid shock-breakout cooling leads to relatively low temperatures in early-time spectra, compared to explosions of red supergiant stars, as well as a rapid early light curve decline. Optical spectra of SN 2011dh are dominated by H lines out to day 10 after explosion, after which He I lines develop. This SN is likely a member of the cIIb (compact IIb) class, with progenitor radius larger than that of SN 2008ax and smaller than the eIIb (extended IIb) SN 1993J progenitor. Our data imply that the object identified in pre-explosion Hubble Space Telescope images at the SN location is possibly a companion to the progenitor or a blended source, and not the progenitor star itself, as its radius (~1013 cm) would be highly inconsistent with constraints from our post-explosion spectra.

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The nearby Type Ia supernova SN 2011fe in M101 (cz=241 km s^-1) provides a unique opportunity to study the early evolution of a "normal" Type Ia supernova, its compositional structure, and its elusive progenitor system. We present 18 high signal-to-noise spectra of SN 2011fe during its first month beginning 1.2 days post-explosion and with an average cadence of 1.8 days. This gives a clear picture of how various line-forming species are distributed within the outer layers of the ejecta, including that of unburned material (C+O). We follow the evolution of C II absorption features until they diminish near maximum light, showing overlapping regions of burned and unburned material between ejection velocities of 10,000 and 16,000 km s^-1. This supports the notion that incomplete burning, in addition to progenitor scenarios, is a relevant source of spectroscopic diversity among SNe Ia. The observed evolution of the highly Doppler-shifted O I 7774 absorption features detected within five days post-explosion indicate the presence of O I with expansion velocities from 11,500 to 21,000 km s^-1. The fact that some O I is present above C II suggests that SN 2011fe may have had an appreciable amount of unburned oxygen within the outer layers of the ejecta.

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Las infecciones de vías urinarias (IVU) son frecuentes en la comunidad, existe un incremento progresivo en los mecanismos de resistencia de las enterobacterias, conocer los factores de riesgo representa un interés en la investigación actual. Objetivo: identificar los factores de riesgo para IVU adquirida en la comunidad por enterobacterias productoras de β-lactamasas de espectro extendido (BLEE) o AmpC positivas. Diseño: estudio observacional analítico tipo casos y controles, 50 casos y 100 controles Medición: análisis de las variables de interés para la determinación de las asociaciones en los respectivos Odd ratios (OR). Resultados: se obtuvo un total de 25 casos y 50 controles, en el análisis univariado el uso previo de antibióticos (OR, 6.68; CI 95%, 2-22.32; P 0.001) y los procedimientos previos de la vía urinaria (OR, 3.45; CI 95%, 1.102-10.83; P 0.028) son factores de riesgo para IVU por BLEE o AmpC, en el análisis multivariado el uso previo de antibiótico represento el principal factor de riesgo (OR, 7.36; CI 95%, 1.76-30.77; P 0.006), las quinolonas fueron el antibiótico de uso previo más frecuente. Conclusiones: El uso previo de antibióticos es el principal factor de riesgo para adquirir IVU por enterobacterias productoras de BLEE o AmpC, es necesario ampliar el tamaño de la muestra actual para determinar el impacto que puedan tener las otras variables a estudio.

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Con el fin de la Guerra Fría, la disolución de la Unión Soviética y el comienzo del proceso de Globalización, nuevos factores de amenaza no había recibido la trascendencia necesaria, pero muy silenciosamente iban cobrando vitalidad dentro del amplio concepto de seguridad. Este es el caso de la proliferación nuclear, que ha dejado de ser exclusivo de las grandes potencias, como herramienta fundamental de contención entre ambos bloques durante la Guerra Fría, para estar al alcance de países de menor importancia o grupo de personas, que quieran satisfacer su ambición de convertirse en una potencia nuclear, dejando incluso de lado o simplemente olvidando una serie de necesidades básicas de su población.

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This Letter presents a measurement of the W+ W- production cross section in sqrt(s) = 7  TeV pp collisions by the ATLAS experiment, using 34  pb(-1) of integrated luminosity produced by the Large Hadron Collider at CERN. Selecting events with two isolated leptons, each either an electron or a muon, 8 candidate events are observed with an expected background of 1.7 ± 0.6 events. The measured cross section is 41(-16)(+20)(stat) ± 5(syst)±1(lumi)  pb, which is consistent with the standard model prediction of 44 ± 3  pb calculated at next-to-leading order in QCD.

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This Letter presents the first search for a heavy particle decaying into an e ± μ(-/+) final state in sqrt[s] = 7 TeV pp collisions at the LHC. The data were recorded by the ATLAS detector during 2010 and correspond to a total integrated luminosity of 35 pb(-1). No excess above the standard model background expectation is observed. Exclusions at 95% confidence level are placed on two representative models. In an R-parity violating supersymmetric model, tau sneutrinos with a mass below 0.75 TeV are excluded, assuming all R-parity violating couplings are zero except λ(311)' = 0.11 and λ312 = 0.07. In a lepton flavor violating model, a Z'-like vector boson with masses of 0.70-1.00 TeV and corresponding cross sections times branching ratios of 0.175-0.183 pb is excluded. These results extend to higher mass R-parity violating sneutrinos and lepton flavor violating Z's than previous constraints from the Tevatron.

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Azimuthal decorrelations between the two central jets with the largest transverse momenta are sensitive to the dynamics of events with multiple jets. We present a measurement of the normalized differential cross section based on the full data set (∫Ldt=36  pb(-1)) acquired by the ATLAS detector during the 2010 sqrt(s)=7  TeV proton-proton run of the LHC. The measured distributions include jets with transverse momenta up to 1.3 TeV, probing perturbative QCD in a high-energy regime.

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This Letter presents the first search for supersymmetry in final states containing one isolated electron or muon, jets, and missing transverse momentum from √s=7  TeV proton-proton collisions at the LHC. The data were recorded by the ATLAS experiment during 2010 and correspond to a total integrated luminosity of 35  pb(-1). No excess above the standard model background expectation is observed. Limits are set on the parameters of the minimal supergravity framework, extending previous limits. Within this framework, for A(0)=0 GeV, tanβ=3, and μ>0 and for equal squark and gluino masses, gluino masses below 700 GeV are excluded at 95% confidence level.

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A search for diphoton events with large missing transverse energy is presented. The data were collected with the ATLAS detector in proton-proton collisions at √s=7 TeV at the CERN Large Hadron Collider and correspond to an integrated luminosity of 3.1 pb⁻¹. No excess of such events is observed above the standard model background prediction. In the context of a specific model with one universal extra dimension with compactification radius R and gravity-induced decays, values of 1/R<729 GeV are excluded at 95% C. L., providing the most sensitive limit on this model to date.