Et certe opera Deus facit mediantibus causis secundis : Fray Luis de León y la determinación del derecho

Luis de León es una de las figuras más importantes de la llamada Escolástica salmantina. En su obra, que marca el culmen de la escuela agustina del siglo XVI, se reúnen los más diversos oficios (jurista, prosista, teólogo, poeta, etc.) y las más distintas tradiciones de pensamiento (tomismo, nominalismo, humanismo, etc.). Su trabajo como teórico del derecho, que es el que aquí se procura destacar, se ha visto ensombrecido, aparentemente, por su renombre como literato y místico. Esto, sin embargo, no significa que su reflexión iusfilosófica sea de poca entidad. Todo lo contrario, las ideas jurídicas del pensador español representan una de las piezas más importantes de la Escuela teológica de Salamanca

Discovery of τ Neutrino Appearance in the CNGS Neutrino Beam with the OPERA Experiment

The OPERA experiment was designed to search for νµ → ντ oscillations in appearance mode, i.e. by detecting the τ leptons produced in charged current ντ interactions. The experiment took data from 2008 to 2012 in the CERN Neutrinos to Gran Sasso beam. The observation of the νµ → ντ appearance, achieved with four candidate events in a subsample of the data, was previously reported. In this Letter, a fifth ντ candidate event, found in an enlarged data sample, is described. Together with a further reduction of the expected background, the candidate events detected so far allow us to assess the discovery of νµ → ντ oscillations in appearance mode with a significance larger than 5 σ.

Limits on muon-neutrino to tau-neutrino oscillations induced by a sterile neutrino state obtained by OPERA at the CNGS beam

The OPERA experiment, exposed to the CERN to Gran Sasso νµ beam, collected data from 2008 to 2012. Four oscillated ντ Charged Current interaction candidates have been detected in appearance mode, which are consistent with νµ → ντ oscillations at the atmospheric ∆m^2 within the “standard” three-neutrino framework. In this paper, the OPERA ντ appearance results are used to derive limits on the mixing parameters of a massive sterile neutrino.

The OPERA experiment

The OPERA experiment was designed to study νμ→ντ oscillations in appearance mode using the CERN to Gran Sasso high energy neutrino beam. From 2008 to 2012, 19505 CNGS neutrino interactions were recorded in the OPERA detector. At the present status of the analysis, 4 ντ candidate events have been observed, establishing the oscillation mechanism in the atmospheric sector with a significance of 4.2 σ. The oscillation analysis will be presented in detail and the candidate events will be described. The final measurement of the atmospheric muon charge ratio in the TeV region will be also reported.

Opera D. Gregorii Papæ, huius nominis primi, cognomento Magni, omnia quæ extant / accuratissima diligentia à mendis multis ... maximè in libris Epistolarum, repurgata ... ; cum indice duplici ...

Marca tip. en port. y en 2P8v

Opera / D. Gregorii Papæ, huius nominis primi, cognomento Magni, omnia quæ extant accuratissima diligentia à mendis multis ... maximè in libris Epistolarum, repurgata ... ; cum indice duplici ...

Marca tip. en port. y en 2P8v

Dn. Cornelii Iansenii ... Commentariorum in suam concordiam, ac totam historiam Euangelicam epitome / opera, & industria F. Matthaei à Castro Insulensis...

Marca tip. en port. (Vandeweghe y Beeck, p. 91, merk 2)