130 research outputs found

    Evaluación estadística de la densidad electrónica máxima a -120 de latitud dip

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    Se estudia la distribución de la densidad electrónica máxima de la región F2 de la ionosfera a -12° de latitud dip. En este trabajo se comparan datos experimentales obtenidos por sondadores con valores proporcionados por el SLIM (Modelo Ionosférico Se- miempírico para Bajas Latitudes). El modelo nuestra las densidades electrónicas como una función de la altura, la latitud dip y el tiempo local, resolviendo numéricamente la ecuación de continuidad del O*. No se tiene en cuenta el efecto longitudinal. Los datos experimentales que se analizan provienen de Tucumán y Vanimo. Se ha trabajado con las medianas mensuales de la frecuencia crítica máxima para ambos sois ticios y el equinoccio, realizando un promedio de los meses correspondientes. Se han calculado los coeficientes de correlación p y de regresión y también se han construido rectas de regresión entre los valores experimentales y los determinados por el mcdelo. Para ambas estaciones, existe un buen acuerdo en el equinoccio mientras que en el solsticio de diciembre es cuando se manifiesta el mayor apartamien to entre los valores medidos y los calculados.The ionospheric F2 region maximum electronic density distribution at -12® dip latitude is studied. In this paper sounders experimental data are compared with SLIM ("Semi Empirical Low-Latitude Ionospheric Medel") values. In this model, electron densities as a function of altitude, latitude and local time are calculated by solving the time dependent ion (O+) continuity equation numerically. The longitudinal effect is not taken into account. Experimental data analyzed are from Tucumán and Vanirno. Average maximum critical frequency monthly medians were used for both solsticies and equinox. Correlation and regression coefficients were computed and the regression lines, between experimen tai and inc del data were plotted. There is a good agreement during equinox in both stations while in december solstice an important distance between computed and measured data is observed.Asociación Argentina de Geofísicos y Geodesta

    Tetrads in SU(3) X SU(2) X U(1) Yang-Mills geometrodynamics

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    The relationship between gauge and gravity amounts to understanding underlying new geometrical local structures. These structures are new tetrads specially devised for Yang-Mills theories, Abelian and Non-Abelian in four-dimensional Lorentzian spacetimes. In the present manuscript a new tetrad is introduced for the Yang-Mills SU(3) X SU(2) X U(1) formulation. These new tetrads establish a link between local groups of gauge transformations and local groups of spacetime transformations. New theorems are proved regarding isomorphisms between local internal SU(3) X SU(2) X U(1) groups and local tensor products of spacetime LB1 and LB2 groups of transformations. The new tetrads and the stress-energy tensor allow for the introduction of three new local gauge invariant objects. Using these new gauge invariant objects and in addition a new general local duality transformation, a new algorithm for the gauge invariant diagonalization of the Yang-Mills stress-energy tensor is developed.Comment: There is a new appendix. The unitary transformations by local SU(2) subgroup elements of a local group coset representative is proved to be a new local group coset representative. This proof is relevant to the study of the memory of the local tetrad SU(3) generated gauge transformations. Therefore, it is also relevant to the group theorems proved in the paper. arXiv admin note: substantial text overlap with arXiv:gr-qc/060204

    Présence de métaux lourds et de résidus médicamenteux dans les effluents des établissements de santé de Dakar (Sénégal)

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    L’objectif de cette étude est de quantifier les concentrations en métaux lourds et de rechercher la présence de résidus de molécules médicamenteuses des effluents de trois hôpitaux de Dakar (Sénégal). C’est ainsi que la collecte des effluents a été réalisée chaque jour sur une période de trois semaines à l’entrée du déversoir des services de radiologie, de médecine interne et d’odontologie. Ensuite, des échantillons composites par semaine ont été constitués pour rechercher leur composition en métaux lourds et en résidus médicamenteux. Le transport a été effectué à +4 °C et à l'obscurité pour assurer une conservation satisfaisante. Les métaux lourds ont été dosés par ICP-MS et les résidus de médicaments ont été recherchés par UPLCMS/ MS. Les médicaments identifiés dans les effluents sont essentiellement des analgésiques et des psychotropes. La concentration en métaux lourds des effluents des trois hôpitaux est inférieure aux normes sénégalaises et de celles de L’OMS fixant les conditions de rejet de métaux dans les eaux usées. Cependant, bien que les taux retrouvés soient tolérables, leur introduction continuelle en milieu aquatique pourrait être à l’origine d’effets néfastes sur les organismes marins par des phénomènes de bioaccumulation et de biomagnification. D’où l’importance et la nécessité des stations d’épuration pour une bonne gestion et une réduction des risques écotoxicologiques liés aux effluents liquides hospitaliers.Mots clés : Effluents hospitaliers, métaux lourds, résidus médicamenteux, toxicité

    Can Schwarzschildean gravitational fields suppress gravitational waves?

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    Gravitational waves in the linear approximation propagate in the Schwarzschild spacetime similarly as electromagnetic waves. A fraction of the radiation scatters off the curvature of the geometry. The energy of the backscattered part of an initially outgoing pulse of the quadrupole gravitational radiation is estimated by compact formulas depending on the initial energy, the Schwarzschild radius, and the location and width of the pulse. The backscatter becomes negligible in the short wavelength regime.Comment: 18 pages, Revtex. Added three references; a new comment in Sec. 7; several misprints corrected. To appear in the Phys. Rev.

    Initial data for two Kerr-like black holes

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    We prove the existence of a family of initial data for the Einstein vacuum equation which can be interpreted as the data for two Kerr-like black holes in arbitrary location and with spin in arbitrary direction. When the mass parameter of one of them is zero, this family reduces exactly to the Kerr initial data. The existence proof is based on a general property of the Kerr metric which can be used in other constructions as well. Further generalizations are also discussed.Comment: revtex, 5 pages, no figure

    The Trypanosoma cruzi nucleic acid binding protein Tc38 presents changes in the intramitochondrial distribution during the cell cycle

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    Background: Tc38 of Trypanosoma cruzi has been isolated as a single stranded DNA binding protein with high specificity for the poly [dT-dG] sequence. It is present only in Kinetoplastidae protozoa and its sequence lacks homology to known functional domains. Tc38 orthologues present in Trypanosoma brucei and Leishmania were proposed to participate in quite different cellular processes. To further understand the function of this protein in Trypanosoma cruzi, we examined its in vitro binding to biologically relevant [dT-dG] enriched sequences, its expression and subcellular localization during the cell cycle and through the parasite life stages.Results: By using specific antibodies, we found that Tc38 protein from epimastigote extracts participates in complexes with the poly [dT-dG] probe as well as with the universal minicircle sequence (UMS), a related repeated sequence found in maxicircle DNA, and the telomeric repeat. However, we found that Tc38 predominantly localizes into the mitochondrion. Though Tc38 is constitutively expressed through non-replicating and replicating life stages of T. cruzi, its subcellular localization in the unique parasite mitochondrion changes according to the cell cycle stage. in epimastigotes, Tc38 is found only in association with kDNA in G1 phase. From the S to G2 phase the protein localizes in two defined and connected spots flanking the kDNA. These spots disappear in late G2 turning into a diffuse dotted signal which extends beyond the kinetoplast. This later pattern is more evident in mitosis and cytokinesis. Finally, late in cytokinesis Tc38 reacquires its association with the kinetoplast. in non-replicating parasite stages such as trypomastigotes, the protein is found only surrounding the entire kinetoplast structure.Conclusions: the dynamics of Tc38 subcellular localization observed during the cell cycle and life stages support a major role for Tc38 related to kDNA replication and maintenance.FIRCAFondo Clemente Estable (DICyT)FAPESConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)PROSULPEDECIBAAMSUD-PasteurFac Ciencias, Lab Interacc Mol, Montevideo, UruguayFac Med, Dept Genet, Montevideo, UruguayFac Ciencias, Dept Biol Celular & Mol, Montevideo, UruguayInst Invest Biol Clemente Estable Montevideo Urug, Dept Neurobiol Celular & Mol, Montevideo, UruguayUniv Nacl Gen San Martin, CONICET, INTECH, Inst Invest Biotecnol, Buenos Aires, DF, ArgentinaUniversidade Federal de São Paulo, Dept Microbiol Imunol & Parasitol, São Paulo, BrazilSUNY Buffalo, Dept Microbiol & Immunol, Buffalo, NY 14260 USAInst Biol Mol Parana, Curitiba, Parana, BrazilUniversidade Federal de São Paulo, Dept Microbiol Imunol & Parasitol, São Paulo, BrazilFIRCA: R03 TW05665-01Fondo Clemente Estable (DICyT): 7109Web of Scienc

    Binary black holes in circular orbits. II. Numerical methods and first results

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    We present the first results from a new method for computing spacetimes representing corotating binary black holes in circular orbits. The method is based on the assumption of exact equilibrium. It uses the standard 3+1 decomposition of Einstein equations and conformal flatness approximation for the 3-metric. Contrary to previous numerical approaches to this problem, we do not solve only the constraint equations but rather a set of five equations for the lapse function, the conformal factor and the shift vector. The orbital velocity is unambiguously determined by imposing that, at infinity, the metric behaves like the Schwarzschild one, a requirement which is equivalent to the virial theorem. The numerical scheme has been implemented using multi-domain spectral methods and passed numerous tests. A sequence of corotating black holes of equal mass is calculated. Defining the sequence by requiring that the ADM mass decrease is equal to the angular momentum decrease multiplied by the orbital angular velocity, it is found that the area of the apparent horizons is constant along the sequence. We also find a turning point in the ADM mass and angular momentum curves, which may be interpreted as an innermost stable circular orbit (ISCO). The values of the global quantities at the ISCO, especially the orbital velocity, are in much better agreement with those from third post-Newtonian calculations than with those resulting from previous numerical approaches.Comment: 27 pages, 20 PostScript figures, improved presentation of the regularization procedure for the shift vector, new section devoted to the check of the momentum constraint, references added + minor corrections, accepted for publication in Phys. Rev.

    Acoplamiento de la alta y baja ionosfera durante la tormenta geomagnética del 26 de marzo de 1976

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    Se realiza el análisis comparativo del comportamiento dé diferentes parámetros de las regiones D, E y F para Tucumán durante la tormenta del 26 de marzo de 1976. Para el estudio de las capas E y F se trabajo con registros del sondador vertical. Para la región D se infiere el comportamiento de la misma a través de registros de fase y amplitud en señales de muy baja frecuencia emitidas por la estación NAA. El rasgo más saliente del presente estudio indica que la perturbación ionosférica que, iniciada en la zona auroral de la región F y propagada hacia bajas latitudes en camino horizontal, también mostraría una componente vertical que llega a afectar la región D. En la comparación de parámetros indicadores de concentración electrónica se observa comportamiento tanto en fase como en contrafase.A comparative analysis of the behaviour of the D,E and F regions physical parameters over Tucumán for the 26 of march, 1976 storm, has been realized. Tucumán vertical sounder records were used for the E and F regions data. The behaviour of D region has been inferred through phase and amplitude records of VLF signals emitted by the NAA station. One important feature of the present study indicates that the ionospheric perturbation, with origin in the auroral zone and propagating equatorward in a horizontal way, would also show a vertical component reaching the D-region. After comparing parameters indicating electron concentration changes a behaviour in phase as well as in counterphase has been observed.Asociación Argentina de Geofísicos y Geodesta
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