0000000000413962

AUTHOR

Ana Beatriz Alvarez Perez

The earth Mantle-Core effect in charge-asymmetries for atmospheric neutrino oscillations

Earth medium effects in the three-neutrino oscillations of atmospheric neutrinos are observable under appropriate conditions. This paper generalizes the study of the medium effects and the possibility of their observation in the atmospheric neutrino oscillations from the case of neutrinos traversing only the Earth mantle, where the density is essentially constant, to the case of atmospheric neutrinos crossing also the Earth core. In the latter case new resonance-like effects become apparent. We calculate the CPT-odd asymmetry for the survival probability of muon neutrinos and the observable muon-charge asymmetry, taking into account the different atmospheric neutrino fluxes, and show the de…

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Plasma effects on neutrino-antineutrino synchrotron radiation in dense matter

Abstract We consider plasma effects on ν ν synchroton radiation from ultrarelativistic, degenerate electrons in neutron stars with strong magnetic fields. Under typical conditions for such stars, a semiclassical calculation can be performed, in which electrons are considered to move along classical paths. We show that collective effects in the plasma lead to an essential enhancement (about three times) of the vector weak-current contributions to neutrino pair emissivity.

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Neutrino Bremsstrahlung from electrons in neutron star crusts

The process of v (v) over bar Bremsstrahlung via electron scattering off nuclei in the crust of a cooling neutron star is studied within the Random Phase Approximation. We show that the electromagnetic plasma screens the vector weak coupling of electrons with the neutrino field. This screening effect takes place in both the crystalline and liquid phase of the neutron star crust, when the momentum carried out by the neutrino pair is smaller than the inverse Debye screening distance of the electrons. This condition holds in the crust volume at temperatures and densities where the electron Bremsstrahlung dominates the neutrino production. As a result, the vector weak current contribution to th…

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Erratum to: “Relativistic direct Urca processes in cooling neutron stars”

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Biofilm formation byCandida albicansmutants for genes coding fungal proteins exhibiting the eight-cysteine-containing CFEM domain

Several features and functions of a Candida albicans gene, PGA10 (also designated as RBT51), coding for a putative polypeptide species belonging to a subset of fungal proteins containing an eight-cysteine domain referred as CFEM (Common in several Fungal Extracellular Membrane proteins), are described. The ORF of the gene (ORF19.5674) encoded a protein of 250 amino acids, with a predicted molecular mass of 25.17 kDa. The product of the PGA10 gene also exhibited some features reminiscent of a class II-type hydrophobin. Deletion of PGA10 resulted in a cascade of pleiotropic effects, mostly affecting cell-surface-related properties. Thus, the null pga10Delta mutant displayed an increased sensi…

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Some biological features of Candida albicans mutants for genes coding fungal proteins containing the CFEM domain

Several biological features of Candida albicans genes (PGA10, RBT5 and CSA1) coding for putative polypeptide species belonging to a subset of fungal proteins containing an eight-cysteine domain referred as common in several fungal extracellular membrane (CFEM) are described. The deletion of these genes resulted in a cascade of pleiotropic effects. Thus, mutant strains exhibited higher cell surface hydrophobicity levels and an increased ability to bind to inert or biological substrates. Confocal scanning laser microscopy using concanavalin A-Alexafluor 488 (which binds to mannose and glucose residues) and FUN-1 (a cytoplasmic fluorescent probe for cell viability) dyes showed that mutant stra…

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