18,048 research outputs found

    A sectoral analysis of Italy's development : 1861 -2010

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    Italy‘s economic growth over its 150 years of unified history did not occur at a steady pace nor was it balanced across sectors. Relying on an entirely new input (labour and capital) database by us built and presented in the Appendix, together with new Banca d‘Italia estimates of GDP by sector, this paper evaluates the different labour productivity growth trends within the Italian economy‘s sectors, as well as the contribution of structural change to productivity growth. Italy‘s performance is then set in an international context: a comparison of sectoral labour productivity growth rates and levels within a selected sample of countries (UK, US, Germany, Japan, India) allows us to better time, quantify and gauge the causes of Italy‘s catching-up process and subsequent more recent slowdown. Finally, the paper analyses the proximate sources of Italy‘s growth, relative to the other countries, in a standard growth accounting framework, in an attempt also to disentangle the contribution of both total factor productivity growth and capital deepening to the country‘s labour productivity dynamics

    Monte Carlo simulations of single polymer force-extension relations

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    We present Monte Carlo simulations for studying the statistical mechanics of arbitrarily long single molecules under stretching. In many cases in which the thermodynamic limit is not satisfied, different statistical ensembles yield different macroscopic force-displacement curves. In this work we provide a description of the Monte Carlo simulations and discuss in details the assumptions adopted

    Scaling relations of the colour-detected cluster RzCS 052 at z=1.016 and of some other high redshift clusters

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    We report on the discovery of the z=1.016 cluster RzCS 052 using a modified red sequence method, followup spectroscopy and X-ray imaging. This cluster has a velocity dispersion of 710+-150 km/s, a virial mass of 4.0e14 Msol (based on 21 spectroscopically confirmed members) and an X-ray luminosity of (0.68+- 0.47)e44 ergs/s in the [1-4] keV band. This optically selected cluster appears to be of richness class 3 and to follow the known L_X-sigma_v relation for high redshift X-ray selected clusters. Using these data, we find that the halo occupation number for this cluster is only marginally consistent with what expected assuming a self-similar evolution of cluster scaling relations, suggesting perhaps a break of them at z~1. We also rule out a strong galaxy merging activity between z=1 and today. Finally, we present a Bayesian approach to measuring cluster velocity dispersions and X-ray luminosities in the presence of a background: we critically reanalyze recent claims for X-ray underluminous clusters using these techniques and find that the clusters can be accommodated within the existing L_X -sigma_v relation.Comment: MNRAS, in pres

    Rare diseases of the anterior segment of the eye: update on diagnosis and management

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    This special issue is focused on the current approaches used to identify and manage rare diseases of the anterior segment of the eye, which range from congenital to acquired disorders that are caused by ocular or systemic conditions and often have consequences that extend beyond the anterior segment of the eye

    Identification of the Coronal Sources of the Fast Solar Wind

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    The present spectroscopic study of the ultraviolet coronal emission in a polar hole, detected on April 6-9, 1996 with the Ultraviolet Coronagraph Spectrometer aboard the SOHO spacecraft, identifies the inter-plume lanes and background coronal hole regions as the channels where the fast solar wind is preferentially accelerated. In inter-plume lanes, at heliocentric distance 1.7 \rsun, the corona expands at a rate between 105 km/s and 150 km/s, that is, much faster than in plumes where the outflow velocity is between 0 km/s and 65 km/s. The wind velocity is inferred from the Doppler dimming of the O VI λλ\lambda\lambda 1032, 1037 \AA lines, within a range of values, whose lower and upper limit corresponds to anisotropic and isotropic velocity distribution of the oxygen coronal ions, respectively.Comment: 14 pages, 4 figures, 3 tables, Accepted by ApJ Letter
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