"Lavinia" de Úrsula K. Le Guin, una novela virgiliana

Análisis de las dependencias y novedades que, respecto al argumento de la Eneida de Virgilio, ofrece la reciente novela Lavinia (2009), de la escritora norteamericana Úrsula K. Le Guin.

Análisis comparativo de los principales aspectos reproductivos de Octopus mimus GOULD, 1852 (CEPHALOPODA: OCTOPODIDAE) entre dos áreas del Litoral Peruano en el año 2014

Se realizó el análisis comparativo de los principales aspectos reproductivos del pulpo Octopus mimus Gould, 1852 entre las áreas de Callao y Chiclayo; utilizando bases de datos correspondientes a los muestreos quincenales de las capturas de la pesquería artesanal durante el año 2014. Se muestrearon 604 individuos (244 hembras y 360 machos) en Callao y 411 individuos (152 hembras y 259 machos) en Chiclayo. Este estudio tiene como objetivo aumentar el conocimiento sobre la biología reproductiva de la especie, y cómo se ve influenciada por las condiciones oceanográficas propias de un área. Se determinó que ambas poblaciones no siguen los parámetros de una distribución normal, y que son estadísticamente diferentes con relación a la longitud del manto. Callao muestra una talla media anual mayor que Chiclayo. La proporción anual de sexos fue a favor de los machos. Resalta el predominio de individuos hembras y machos maduros durante todo el año. La talla de madurez obtenida, confirma que los machos maduran a tallas menores que las hembras. La talla de desove mantiene la tendencia. El peso de madurez en ambos sexos se encontró por debajo del peso mínimo de captura (1 kg), pero el peso de desove de las hembras fue mayor a éste. El grado en que la condición del individuo se ve afectada por la reproducción, es más evidente y determinante en hembras. La especie muestra un crecimiento alométrico negativo. En machos está mejor definido el aumento del peso de la gónada en función de la longitud del manto. La influencia de los factores ambientales sobre el ciclo reproductivo es particular en cada área, lo que explica las diferencias en el biotipo y la estacionalidad de los eventos reproductivos.

Ecología trófica del pulpo Octopus mimus Gould 1852 (Cephalopoda: Octopodidae) invierno 2013-2014 en la bahía del Callao

El pulpo Octopus mimus es un importante recurso de la pesquería artesanal bentónica, que se distribuye desde el norte del Perú a San Vicente, Chile. Se analizaron contenidos gástricos de 741 ejemplares obtenidos de la captura comercial en la bahía del Callao, durante agosto 2013-agosto 2014. Se determinó que las presas más importantes fueron crustáceos Decapoda: Petrolisthes desmarestii (%FO=24,13; %P=21,29%; N=27,10), Cycloxanthops sexdecimdentatus (%FO=16,35; %P=12,16%; N=15,99) y Allopetrolisthes angulosus (%FO=6,17; %P=6,05; %N=25,20). No hubo diferencias en la dieta entre machos y hembras en %FO y %P (Mann -Whitney U-test, p>0,05). Se observaron diferencias en el IR asociado a las fases de desarrollo gonadal en hembras, ejemplares madurantes/maduros mostraron mayor IR (0,17±0,17) que los desovados (0,08± 0,06), en machos no se observaron diferencias. El IR fue mayor en otoño (0,21±0,17) (Kruskal-Wallis test, p < 0,05). Los índices ecológicos mostraron que O. mimus es un depredador generalista (B’>3), observándose traslapo entre la dieta de machos y hembras (Cλ>0,6), por lo que se concluye que su alimentación está influenciada por una combinación de factores fisiológicos y ambientales.

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.

Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars III. Detection of lithium in the metal-poor bulge dwarf MOA-2010-BLG-285S

Context. To study the evolution of Li in the Galaxy it is necessary to observe dwarf or subgiant stars. These are the only long-lived stars whose present-day atmospheric chemical composition reflects their natal Li abundances according to standard models of stellar evolution. Although Li has been extensively studied in the Galactic disk and halo, to date there has only been one uncertain detection of Li in an unevolved bulge star. Aims. Our aim with this study is to provide the first clear detection of Li in the Galactic bulge, based on an analysis of a dwarf star that has largely retained its initial Li abundance. Methods. We performed a detailed elemental abundance analysis of the bulge dwarf star MOA-2010-BLG-285S using a high-resolution and high signal-to-noise spectrum obtained with the UVES spectrograph at the VLT when the object was optically magnified during a gravitational microlensing event (visual magnification A similar to 550 during observation). The Li abundance was determined through synthetic line profile fitting of the (7)Li resonance doublet line at 670.8 nm. The results have been corrected for departures from LTE. Results. MOA-2010-BLG-285S is, at [Fe/H] = -1.23, the most metal-poor dwarf star detected so far in the Galactic bulge. Its old age (12.5 Gyr) and enhanced [alpha/Fe] ratios agree well with stars in the thick disk at similar metallicities. This star represents the first unambiguous detection of Li in a metal-poor dwarf star in the Galactic bulge. We find an NLTE corrected Li abundance of log epsilon(Li) = 2.16, which is consistent with values derived for Galactic disk and halo dwarf stars at similar metallicities and temperatures. Conclusions. Our results show that there are no signs of Li enrichment or production in the Galactic bulge during its earliest phases. Observations of Li in other galaxies (omega Cen) and other components of the Galaxy suggest further that the Spite plateau is universal.

Twisted quantum affine superalgebra Uq[gl(m|n)(2)] and new Uq[osp(m|n)] invariant R-matrices

The minimal irreducible representations of U-q[gl(m|n)], i.e. those irreducible representations that are also irreducible under U-q[osp(m|n)] are investigated and shown to be affinizable to give irreducible representations of the twisted quantum affine superalgebra U-q[gl(m|n)((2))]. The U-q[osp(m|n)] invariant R-matrices corresponding to the tensor product of any two minimal representations are constructed, thus extending our twisted tensor product graph method to the supersymmetric case. These give new solutions to the spectral-dependent graded Yang-Baxter equation arising from U-q[gl(m|n)((2))], which exhibit novel features not previously seen in the untwisted or non-super cases.

Elliptic Gaudin models and elliptic KZ equations

The Gaudin models based on the face-type elliptic quantum groups and the XYZ Gaudin models are studied. The Gaudin model Hamiltonians are constructed and are diagonalized by using the algebraic Bethe ansatz method. The corresponding face-type Knizhnik–Zamolodchikov equations and their solutions are given.

On Quasi-Hopf Superalgebras

In this work we investigate several important aspects of the structure theory of the recently introduced quasi-Hopf superalgebras (QHSAs), which play a fundamental role in knot theory and integrable systems. In particular we introduce the opposite structure and prove in detail (for the graded case) Drinfeld's result that the coproduct Delta ' =_ (S circle times S) (.) T (.) Delta (.) S-1 induced on a QHSA is obtained from the coproduct Delta by twisting. The corresponding "Drinfeld twist" F-D is explicitly constructed, as well as its inverse, and we investigate the complete QHSA associated with Delta '. We give a universal proof that the coassociator Phi ' = (S circle times S circle times S) Phi (321) and canonical elements alpha ' = S(beta), beta ' = S(alpha) correspond to twisting, the original coassociator Phi = Phi (123) and canonical elements alpha, beta with the Drinfeld twist F-D. Moreover in the quasi-tri angular case, it is shown algebraically that the R-matrix R ' = (S circle times S)R corresponds to twisting the original R-matrix R with F-D. This has important consequences in knot theory, which will be investigated elsewhere.

Algebraic Bethe ansatz method for the exact calculation of energy spectra and form factors: applications to models of Bose-Einstein condensates and metallic nanograins

In this review we demonstrate how the algebraic Bethe ansatz is used for the calculation of the-energy spectra and form factors (operator matrix elements in the basis of Hamiltonian eigenstates) in exactly solvable quantum systems. As examples we apply the theory to several models of current interest in the study of Bose-Einstein condensates, which have been successfully created using ultracold dilute atomic gases. The first model we introduce describes Josephson tunnelling between two coupled Bose-Einstein condensates. It can be used not only for the study of tunnelling between condensates of atomic gases, but for solid state Josephson junctions and coupled Cooper pair boxes. The theory is also applicable to models of atomic-molecular Bose-Einstein condensates, with two examples given and analysed. Additionally, these same two models are relevant to studies in quantum optics; Finally, we discuss the model of Bardeen, Cooper and Schrieffer in this framework, which is appropriate for systems of ultracold fermionic atomic gases, as well as being applicable for the description of superconducting correlations in metallic grains with nanoscale dimensions.; In applying all the above models to. physical situations, the need for an exact analysis of small-scale systems is established due to large quantum fluctuations which render mean-field approaches inaccurate.

Ladder operator for the one-dimensional Hubbard model

The one-dimensional Hubbard model is integrable in the sense that it has an infinite family of conserved currents. We explicitly construct a ladder operator which can be used to iteratively generate all of the conserved current operators. This construction is different from that used for Lorentz invariant systems such as the Heisenberg model. The Hubbard model is not Lorentz invariant, due to the separation of spin and charge excitations. The ladder operator is obtained by a very general formalism which is applicable to any model that can be derived from a solution of the Yang-Baxter equation.