104,661 research outputs found
Informazione e adattamento nell'attacco di panico. Una patologia cronica
No full textIl Disturbo di Panico è una patologia psichiatrica
comune, ad alto impatto sociale, a eziopatogenesi complessa
e tendente a cronicizzare.
L'adozione di percorsi diagnostico-terapeutici deve
essere considerata una priorità ed un impegno per tutta
la classe medica sia dal punto di vista deontologico che
etico. Nel Disturbo di Panico è necessaria una strategia
diagnostico-terapeutica razionale che dia la massima
garanzia e deve essere fissata rispettando i bisogni di
ogni singolo individuo, caso per caso senza scelte schematiche.
A seconda della gravità e delle caratteristiche cliniche,
può essere sufficiente l'intervento psicologico limitato
a poche sedute con somministrazione occasionale
di Benzodiazepine, oppure, come avviene nella maggior
parte dei casi, con pazienti che hanno alle spalle una
strategia terapeutica fallimentare, disorientati da anni di
sofferenza e dalle diverse interpretazioni date ai loro disturbi,
è richiesto un intervento più lungo e complesso
di tipo integrato psicologico e farmacologico, basato
sulla riorganizzazione cognitiva e sopratutto sull'informazione.
Noi partiamo dal presupposto che possa scaturire un
buon controllo dei sintomi del disturbo soltanto da una
presa di posizione realistica e da una buona conoscenza
della natura dei sintomi stessi.
Questo tipo di approccio favorisce l'accettazione della
terapia farmacologica, riduce l'ansia e dà modo di
adattarsi e gestire i sintomi residui in un clima di protezione
e di disponibilità competente
Frederick J. Lynch, Joseph Gerald Berry, Giovanni Panico, and Patrick G. Maloney, ca. 1950
No full textdigital photograph (jpeg)Excellent condition.Frederick J. Lynch, Joseph Gerald Berry, Giovanni Panico, and Patrick G. Maloney stand in front of a statue of the Virgin Mary
Measurement of the cosmic rays light component (pHe) primary spectrum with ARGO-YBJ
No full textThe ARGO-YBJ experiment, located at the Yangbajing Cosmic Ray Laboratory (Tibet, 4300 m a.s.l., 606 g/cm 2) has an high segmentation that allows the detection of air showers with greater detail and lower energy threshold (a few hundred GeV) compared to other EAS arrays. The spectrum of the primary cosmic ray light (pHe) component in the energy range ∼10-100TeV is measured selecting quasi-vertical showers (θ<15°) with the reconstructed core position located in a 40×40 m 2 fiducial area. The results are compared with other measurements carried out with direct methods. © 2012 Elsevier B.V
The Electroweak phase transition in models with gauge-Higgs unification
No full textThe dynamics of five dimensional Wilson line phases at finite temperature is studied in the oneloop approximation. We show that at temperatures of order T ∼ 1/L, where L is the length of
the compact space, the gauge symmetry is always restored and the electroweak phase transition
appears to be of first order.
We focus on a specific model where the Wilson line phase is identified with the Higgs field
(gauge-Higgs unification). The transition is of first order even for values of the Higgs mass above
the current experimental limit. If large localized gauge kinetic terms are present, the transition
might be strong enough to give baryogenesis at the electroweak transitio
Nucleon Form Factors from 5D Skyrmions
No full textSeveral aspects of hadron physics are well described by a simple 5D effective field theory, Baryons arise in this scenario as "large" (and therefore calculable) 5D skyrmions. We extend and reline the existing analysis of this 5D soliton, which is fairly non-trivial due to the need of numerical methods. We perform the complete quantization of those collective coordinates which are relevant for computing the static observables like the nucleon form factors. We compare the result with simple expectations about large-N-c QCD and with the experimental data. An agreement within 30% is found. (C) 2009 Elsevier B.V. All rights reserved.S
Measurement of the CR light component primary spectrum with ARGO-YBJ experiment
No full textThe ARGO-YBJ experiment, located at the Yangbajing Cosmic Ray Laboratory (Tibet, 4300 m a.s.l., 606 g/cm2) has an high segmentation that allows the detection of air showers with greater detail and lower energy threshold (a few hundred GeV) compared to other EAS arrays. The spectrum of the primary Cosmic Ray light (p+He) component in the energy range ∼10 - 100 TeV is measured selecting quasi-vertical showers with the reconstructed core position located in a 40×40 m2 fiducial area. The results are compared with other measurements carried out with direct methods
Measurement of the cosmic ray primary spectrum with ARGO-YBJ experiment
No full textThe study of cosmic ray physic of 1012-1015 primary cosmic energy is one of the main goals of ARGO-YBJ experiment. The detector, located at the Yangbajing Cosmic Ray Laboratory (Tibet, 4300 m a.s.l., 606 g/cm2), is an EAS array consisting of a continuous carpet of RPCs. The low energy threshold of the detector allows to study an energy region characterized by the transition from the direct to the indirect measurements. In this talk we will report on the measurement of the cosmic ray energy spectrum at different zenith angles. The phenomenology of horizontal air shower (θ > 70°) will be described and discussed
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