El mar y la mediterraneidad en la narrativa de Elsa Morante

This doctoral Thesis aims to approach the philosophical significance of the Italian author Elsa Morante, expressed through poetic narrative of her second great novel L'isola di Arturo (1957). For this reason, the inductive knowledge has been opted, which can be reached through the symbolic study of the sea and the mediterranean. From the philosophical and psychoanalytical research from such authors as Mircea Eliade, Gaston Bachelard and Carl Jung, linked to the circle of the Eranos Foundation in Switzerland, where the most rigorous multidisciplinary science theories of nature and man converged, and the Grenoble imaginary Center of Research, driven by anthropologist Gilbert Durand in 1966, a revealing investigation of aquatic and marine image has been carried out. In this context of convergence, the work Las estructuras antropológicas del imaginario by Durand, has fulfilled the important catalytic role, of both the Renaissance conception that wants to observe certain universal components in the symbolic vision that nourishes literary expression, as well as the compilation of large images that illuminate the human imaginary of all time. Objectives and results In this regard, it has been considered that the appropriate approach to morantiano imaginary, could only be done thoroughly, based on a repertoire of images as complete as possible, which, if performed from the anthropological compendium of people and civilization of the world, it is offered as a study backed by profound consistency which is the basis of the method. Therefore, it is said, the imaginary is studied and understood through itself. Thus, the internal coherence of this method is seen to be configured as a form of knowledge of human thought because research, from the symbolic point of view, dissects reality in various ways, however, the most seductive is to consider the possibility of an internal coherence between them to converge at a common conclusion which includes all of them. This fact determines the systematization which is shown in the first part of this thesis, as the image and symbol have a close homogeneity between the signifier and the meaning, so that metaphorical expression is established as the structuring element of the human imaginary and the literary representation...

Are long gamma-ray bursts biased tracers of star formation? Clues from the host galaxies of the Swift/BAT6 complete sample of bright LGRBs II. Star formation rates and metallicities at z < 1

Aims. Long gamma-ray bursts (LGRBs) are associated with the deaths of massive stars and might therefore be a potentially powerful tool for tracing cosmic star formation. However, especially at low redshifts (z< 1.5) LGRBs seem to prefer particular types of environment. Our aim is to study the host galaxies of a complete sample of bright LGRBs to investigate the effect of the environment on GRB formation. Methods. We studied host galaxy spectra of the Swift/BAT6 complete sample of 14 z< 1 bright LGRBs. We used the detected nebular emission lines to measure the dust extinction, star formation rate (SFR), and nebular metallicity (Z) of the hosts and supplemented the data set with previously measured stellar masses M_*. The distributions of the obtained properties and their interrelations (e.g. mass-metallicity and SFR-M_* relations) are compared to samples of field star-forming galaxies. Results. We find that LGRB hosts at z< 1 have on average lower SFRs than if they were direct star formation tracers. By directly comparing metallicity distributions of LGRB hosts and star-forming galaxies, we find a good match between the two populations up to 12 +log (O/H)~8.4−8.5, after which the paucity of metal-rich LGRB hosts becomes apparent. The LGRB host galaxies of our complete sample are consistent with the mass-metallicity relation at similar mean redshift and stellar masses. The cutoff against high metallicities (and high masses) can explain the low SFR values of LGRB hosts. We find a hint of an increased incidence of starburst galaxies in the Swift/BAT6 z< 1 sample with respect to that of a field star-forming population. Given that the SFRs are low on average, the latter is ascribed to low stellar masses. Nevertheless, the limits on the completeness and metallicity availability of current surveys, coupled with the limited number of LGRB host galaxies, prevents us from investigating more quantitatively whether the starburst incidence is such as expected after taking into account the high-metallicity aversion of LGRB host galaxies.