7,193 research outputs found

    Confrontation Cinema in the Age of Neoliberalism; Where Brazil and the United States Meet

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    Contents: Introduction; The Smell of Revolution and Popcorn; Filling the Gaps: Historical Context; Brazilian Cinema in the Age of Neoliberalism and Political Discourse of the New Brazilian Left; US Films and the Iraq War: This isn’t my America; Epilogu

    Bank capital structure, regulatory capital, and securities innovations

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    Although financial instruments that, in effect, permit corporations to treat preferred stock dividends as tax-deductible interest have been used by nonfinancial corporations since late 1993, bank holding companies (BHCs) did not issue these trust-preferred securities (TPS) until 1996, when the Federal Reserve qualified them as Tier-1 capital. We delineate and test hypotheses with 1) analyses of the stock-market reaction to the Fed’s ruling and to TPS filings and 2) comparisons of BHCs that issued TPS with those that did not. We conclude that regulatory capital requirements, tax savings, and uninsured sources of funds can have significant positive effects on BHCs’ demand for capital; growth and investment opportunities have an inconclusive effect; and transaction costs have a negative effect. Our results are not consistent with the moral-hazard hypothesis.Bank capital ; Bank holding companies ; Bank supervision ; Securities

    Constraints on a scalar-pseudoscalar Higgs mixing at future e+e- colliders: an update

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    We perform an update of our previous analysis on the constraints on possible deviations of Hbb coupling from its Standard Model value, arising from a scalar-pseudoscalar mixing. In this paper we include a complete simulation of the process e+ e- -> b bbar e+ e- and combine it with our previous results to obtain tighter bounds on the deviations of the parameters describing this coupling that could be measured at the Next Linear Collider.Comment: 3 pages, 2 figures, to be submitted to Phys. Rev.

    Three Jet Events and New Strong Couplings at LEP and NLC

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    We study the effects of new dimension--6 operators, resulting from a general SU(3)C⊗SU(2)L⊗U(1)YSU(3)_C \otimes SU(2)_L \otimes U(1)_Y invariant effective Lagrangian, on three jet production at LEP and at the Next Linear Collider. Contributions to the total event rate and to some event shape variables are analysed in order to establish bounds on these operators.Comment: 5 pages, LaTeX, 1 Figur

    Phase behaviour of additive binary mixtures in the limit of infinite asymmetry

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    We provide an exact mapping between the density functional of a binary mixture and that of the effective one-component fluid in the limit of infinite asymmetry. The fluid of parallel hard cubes is thus mapped onto that of parallel adhesive hard cubes. Its phase behaviour reveals that demixing of a very asymmetric mixture can only occur between a solvent-rich fluid and a permeated large particle solid or between two large particle solids with different packing fractions. Comparing with hard spheres mixtures we conclude that the phase behaviour of very asymmetric hard-particle mixtures can be determined from that of the large component interacting via an adhesive-like potential.Comment: Full rewriting of the paper (also new title). 4 pages, LaTeX, uses revtex, multicol, epsfig, and amstex style files, to appear in Phys. Rev. E (Rapid Comm.

    A new approach to the inverse problem for current mapping in thin-film superconductors

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    A novel mathematical approach has been developed to complete the inversion of the Biot-Savart law in one- and two-dimensional cases from measurements of the perpendicular component of the magnetic field using the well-developed Magneto-Optical Imaging technique. Our approach, especially in the 2D case, is provided in great detail to allow a straightforward implementation as opposed to those found in the literature. Our new approach also refines our previous results for the 1D case [Johansen et al., Phys. Rev. B 54, 16264 (1996)], and streamlines the method developed by Jooss et al. [Physica C 299, 215 (1998)] deemed as the most accurate if compared to that of Roth et al. [J. Appl. Phys. 65, 361 (1989)]. We also verify and streamline the iterative technique, which was developed following Laviano et al. [Supercond. Sci. Technol. 16, 71 (2002)] to account for in-plane magnetic fields caused by the bending of the applied magnetic field due to the demagnetising effect. After testing on magneto-optical images of a high quality YBa2Cu3O7 superconducting thin film, we show that the procedure employed is effective

    Can neutrino-assisted early dark energy models ameliorate the H0H_0 tension in a natural way?

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    The idea of neutrino-assisted early dark energy (ν\nuEDE), where a coupling between neutrinos and the scalar field that models early dark energy (EDE) is considered, was introduced with the aim of reducing some of the fine-tuning and coincidence problems that appear in usual EDE models. In order to be relevant in ameliorating the H0H_0 tension, the contribution of EDE to the total energy density (fEDEf_\text{EDE}) should be around 10\% near the redshift of matter-radiation equality. We verify under which conditions ν\nuEDE models can fulfill these requirements for a model with a quartic self-coupling of the EDE field and an exponential coupling to neutrinos. We find that in the situation where the EDE field is frozen initially, the contribution to fEDEf_\text{EDE} can be significant but it is not sensitive to the neutrino-EDE coupling and does not address the EDE coincidence problem. On the other hand, if the EDE field starts already dynamical at the minimum of the effective potential, it tracks this time-dependent minimum that presents a feature triggered by the neutrino transition from relativistic to nonrelativistic particles. This feature generates fEDEf_\text{EDE} in a natural way at around this transition epoch, that roughly coincides with the matter-radiation equality redshift. For the set of parameters that we considered we did not find values that satisfy the requirements on the background cosmological evolution to mitigate the Hubble tension in a natural way in this particular ν\nuEDE model.Comment: 6 pages, 4 figures. New version with more detailed analysi
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