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Il primo concorso per il Palazzo di Giustizia a Roma del 1884. Ricostruzione critica del progetto di Ernesto Basile

2019

1. Breve descrizione dell’oggetto di studio Il concorso del Palazzo di Giustizia di Roma si svolge in quattro fasi svolte tra il 1884 e il 1887. Il progetto per il primo concorso, del 1884, redatto dall’allora giovanissimo Ernesto Basile (Palermo 1857-1932), rivela una grande perizia progettuale che trasforma il complesso programma funzionale in un austero edificio in stile neofiorentino. I disegni originari dell’opera, non realizzata, conservati presso la Dotazione Basile del Dipartimento di Architettura dell’Università di Palermo, sono stati oggetto di studio propedeutico alle fasi di analisi, interpretazione e ricostruzione congetturale del modello digitale. 2. Stato dell’arte e riferime…

the spatiality of the great vestibule• elaboration of axonometric and perspective view• choice of interpretation criteria in case of project incongruitiethe vaulted arcades.the space of the main courtyard which Basile outlines in a sketch• elaboration of analytical drawings (modular functional compositional volumetric schemes)• modular study and flat vectorization• application of rendering techniques consistent with the available information. 4. Objectives pursued and achieved Conjectural reconstruction achieved the following results: • formulation of analytical documents which show how the planimetric and altimetric articulation are perfectly consistent with the functional program• definition of the level of uncertainty1. Brief description of the object of study The competition of the Palace of Justice in Rome takes place in four phases between 1884 and 1887. The project for the first competition in 1884 drawn up by the then very young Ernesto Basile (Palermo 1857-1932) reveals a great deal of design expertise that transforms the complex functional program into an austere building in neo-florentine style. The original drawings of the building not realized kept in the Basile Endowment of the Department of Architecture of the University of Palermo have been the subject of preliminary study to the phases of analysis interpretation and conceptual reconstruction of the digital model. 2. State of the art and main bibliographical references The conjectural reconstruction on the basis of drawings and archival documents is a well-established and codified practice thanks to various disciplinary contributions at national and international level. See: F. I. Apollonio Classification Schemes for Visualization of Uncertainty in Digital Hypothetical Reconstruction in M. Sander P. Mieke P. Kuroczyński M. Ioannides 3D Research Challenges in Cultural Heritage II Cham (CH) 2016. G. Antista M. Cannella Ricostruire. Architettura - Storia – Rappresentazione Palermo 2015. For studies related to the examinated project see: E. Mauro E. Sessa I disegni della Collezione Basile Roma 2015. E. Sessa Ernesto Basile. Dall'eclettismo Classicista al Modernismo Palermo 2002. 3. Definition of the methodologies adopted in the research Methodological phases: • historical analysi• survey of the original drawings and dimensional verification of the flat scanSettore ICAR/17 - Disegno• construction of perspective views deduced from the original drawings that highlight: the volumetric hierarchy and the function of the bugnate in the scanning of the masonry ma• three-dimensional modeling
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Di Maio, A

2012

Traduzione di poesie e brani tratti da varie opere di Wole Soyinka, Premio Nobel per la letteratura (1986)

traduzione dell'intervista inedita "La terapia delle parole: conversazione con Wole Soyinka" condotta dalla curatrice del volumeWole SoyinkaLetteratura nigerianatraduzione di un brano dell'autobiografia "You Must Set Forth at Dawn"Traduzione del saggio inedito "Assoluti e relativismi culturali: la dignità e la sacralità della vita umana"Traduzione delle poesie "Conversazione telefonica" e "I figli di questa terra"
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Three-dimensional core-collapse supernovae with complex magnetic structures: I. Explosion dynamics

2021

Magnetic fields can play a major role in the dynamics of outstanding explosions associated to violent events such as GRBs and hypernovae, since they provide a natural mechanism to harness the rotational energy of the central proto-neutron star and power relativistic jets through the stellar progenitor. As the structure of such fields is quite uncertain, most numerical models of MHD-driven core-collapse supernovae consider an aligned dipole as initial magnetic field, while the field's morphology can actually be much more complex. We present three-dimensional simulations of core-collapse supernovae with more realistic magnetic structures, such as quadrupolar fields and, for the first time, an…

transients: supernovaeField (physics)MHDAstrophysics::High Energy Astrophysical Phenomenagamma-ray burst: generalFOS: Physical sciencesAstrophysics01 natural sciencesstars: magnetarsAstrophysical jet0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)relativistic processesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomy and AstrophysicsRotational energyMagnetic fieldDipoleAstrophysics - Solar and Stellar AstrophysicsinstabilitiesSpace and Planetary ScienceMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]HypernovaDynamo
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The impact of non-dipolar magnetic fields in core-collapse supernovae

2019

The magnetic field is believed to play an important role in at least some core-collapse supernovae if its magnitude reaches $10^{15}\,\rm{G}$, which is a typical value for a magnetar. In the presence of fast rotation, such a strong magnetic field can drive powerful jet-like explosions if it has the large-scale coherence of a dipole. The topology of the magnetic field is, however, probably much more complex with strong multipolar and small-scale components and the consequences for the explosion are so far unclear. We investigate the effects of the magnetic field topology on the dynamics of core-collapse supernovae and the properties of forming proto-neutron star (PNS) by comparing pre-collap…

transients: supernovaeMHDAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCompact starMagnetar01 natural sciencesstars: magnetars0103 physical sciences010303 astronomy & astrophysicsrelativistic processesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Toroid010308 nuclear & particles physicsgamma-ray burststurbulenceAstronomy and AstrophysicsRotational energyComputational physicsMagnetic fieldSupernovaDipoleSpace and Planetary ScienceMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Monthly Notices of the Royal Astronomical Society
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AI Ethics in Industry: A Research Framework

2019

Artificial Intelligence (AI) systems exert a growing influence on our society. As they become more ubiquitous, their potential negative impacts also become evident through various real-world incidents. Following such early incidents, academic and public discussion on AI ethics has highlighted the need for implementing ethics in AI system development. However, little currently exists in the way of frameworks for understanding the practical implementation of AI ethics. In this paper, we discuss a research framework for implementing AI ethics in industrial settings. The framework presents a starting point for empirical studies into AI ethics but is still being developed further based on its pr…

transparencyFOS: Computer and information sciencesAI developmentComputingMilieux_THECOMPUTINGPROFESSIONresearch frameworkvastuullisuustekoälyartificial intelligenceGeneralLiterature_MISCELLANEOUSComputer Science - Computers and SocietyAI ethicsComputingMethodologies_PATTERNRECOGNITIONaccountabilityComputers and Society (cs.CY)responsibilityetiikkateollisuus
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Recommendations of the LHC Dark Matter Working Group: Comparing LHC searches for dark matter mediators in visible and invisible decay channels and ca…

2019

Physics of the Dark Universe 26, 100377 (2019). doi:10.1016/j.dark.2019.100377

transverse momentum: missing-energyscale: TeVAtomic01 natural sciencesParticle and Plasma Physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]scattering [p p]TeV [scale]010303 astronomy & astrophysicsPhysicsLarge Hadron ColliderCMSPhysicsaxial-vectorMonte Carlo [numerical calculations]ATLASCERN LHC Collinterpretation of experimentsrelic density [dark matter]colliding beams [p p]numerical calculations: Monte CarloAstronomical and Space SciencessignatureParticle physicsp p: scatteringDark matterlepton: couplingdark matter: production5300103 physical sciencesThermalNuclearddc:530Pseudovector010308 nuclear & particles physicsdark matter: relic densityMolecularAstronomy and Astrophysicsmediation [dark matter]dark matter: mediationproduction [dark matter]Space and Planetary Sciencemissing-energy [transverse momentum][PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]invisible decaycoupling [lepton][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]p p: colliding beamsvectorLeptonexperimental results
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Calidad de la farmacoterapia antidiabética en el departamento de salud Valencia Clínico Malvarrosa en 2015-2019 con datos de la vida real

2023

La diabetes mellitus (DM) es una enfermedad crónica caracterizada por un déficit de insulina o de su acción, produciéndose, en ausencia de tratamiento, una elevación de la glucemia. La diabetes mellitus, especialmente del tipo 2 (DM2), se ha convertido en un problema de Salud Pública de primer nivel. Se trata de una enfermedad con una alta prevalencia y a que constituye un factor de riesgo para el sistema circulatorio , que además es previsible que se incremente con el aumento de esperanza de vida y el envejecimiento poblacional. Aunque el inicio del tratamiento farmacológico de la diabetes se inició básicamente en 1921 con el aislamiento de una sustancia insulínica, es en los últimos años …

tratamientodiabetesUNESCO: Ciencia Médicasfarmacoterapia
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The OLYMPUS Experiment

2014

Nuclear instruments & methods in physics research / A 741, 1 - 17 (2014). doi:10.1016/j.nima.2013.12.035

two-photon [exchange]Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsHadronluminosity: monitoringRecoil4-MOMENTUM TRANSFERSNuclear Experiment (nucl-ex)Nuclear ExperimentInstrumentationNuclear ExperimentPhysicsElastic scatteringLuminosity (scattering theory)ELECTROMAGNETIC FORM-FACTORSInstrumentation and Detectors (physics.ins-det)elastic scattering [cross section]positron p: elastic scatteringAntimatterdrift chamberelastic scattering [electron p]target [hydrogen]proportional chamberCROSS-SECTIONNuclear and High Energy PhysicsELECTRON-PROTONDESY DORIS StorFOS: Physical sciencesmonitoring [luminosity]time-of-flight530electron p: elastic scatteringNuclear physicsCross section (physics)RATIO(GEV/C)(2)p: form factor: ratiocalorimeterddc:530cross section: elastic scatteringactivity reporthydrogen: targetexchange: two-photonScatteringPOSITRONSDESYelastic scattering [positron p]magnetic spectrometerELECTROMAGNETIC FORM-FACTORS; PROTON ELASTIC-SCATTERING; 4-MOMENTUM TRANSFERS; ELECTRON-PROTON; CROSS-SECTION; RATIO; (GEV/C)(2); POSITRONSform factor: ratio [p]gas electron multiplierPhysics::Accelerator PhysicsPROTON ELASTIC-SCATTERINGHigh Energy Physics::Experiment
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Search for photons with energies above 1018 eV using the hybrid detector of the Pierre Auger Observatory

2017

A search for ultra-high energy photons with energies above 1 EeV is performed using nine years of data collected by the Pierre Auger Observatory in hybrid operation mode. An unprecedented separation power between photon and hadron primaries is achieved by combining measurements of the longitudinal air-shower development with the particle content at ground measured by the fluorescence and surface detectors, respectively. Only three photon candidates at energies 1-2 EeV are found, which is compatible with the expected hadron-induced background. Upper limits on the integral flux of ultra-high energy photons of 0.027, 0.009, 0.008, 0.008 and 0.007 km-2 sr-1 yr-1 are derived at 95% C.L. for ener…

ultra high energy cosmic rays cosmic ray experimentsPhoton[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]AstronomyHadronFluxultra high energy cosmic rays; cosmic ray experiments7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)energy: thresholdCosmic ray experiments[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsphoton: productionconstraint: energyCOSMIC-RAYSAugerobservatoryContent (measure theory)ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearfluorescenceAstrophysics - High Energy Astrophysical PhenomenalongitudinalAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesCosmic rayultra high energy cosmic raysdark matterUltra high energy cosmic rays Cosmic ray experiments Astronomy and Astrophysics.Nuclear physics[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesultra high energy cosmic rays; cosmic ray experiments; Astronomy and Astrophysicscosmic radiation: UHEHigh Energy PhysicsCiencias ExactasPierre Auger ObservatorySPECTRUMhybridbackgrounddetector: surface010308 nuclear & particles physicsFísicaUltra high energy cosmic raysAstronomy and AstrophysicsASTROFÍSICAULTRA-HIGH ENERGYfluxExperimental High Energy PhysicsHigh Energy Physics::Experimentcosmic ray experimentshadron[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)
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Adecuación del uso de los servicios médicos de urgencias por parte del paciente adolescente

2021

Objetivo: Comparar la adecuación de las consultas a urgencias del paciente adolescente que está siendo atendido por el pediatra (12 a 14 años) y los que ya no lo están (15 a 18 años). Métodos: Estudio transversal con pacientes en edades entre 12 y 18 años que acudieron al Servicio de Urgencias del Hospital La Salud de Valencia durante el 2018. Los criterios de adecuación se basaron en el Protocolo de Adecuación de Urgencias Hospitalarias. Las variables de adecuación se describieron mediante frecuencias y como método de comparación se utilizó el test exacto de Fisher y la razón de momios. En todos los casos los contrastes de hipótesis fueron bilaterales, con un nivel de confianza de 95 % y l…

urgencias médicasmal uso de los servicios de saludpediatría: estudio comparativopediatríaUNESCO::CIENCIAS MÉDICASestudio comparativoadolescenteUrgències en pediatria:CIENCIAS MÉDICAS [UNESCO]PediatricsRJ1-570Salut pública Planificació
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