α-alchilazione di aldeidi, via organocatalisi: un approccio sintetico e computazionale

During this internship, the α-alkylation of branched aldehydes was taken into consideration. An enantiopure Betti’s base derivative was used as catalyst, applying a new concept in catalysis: organocatalysis. The Betti’s base may be of particular interest for organic chemists working in the field of “reactions catalysed by enantiopure small organic molecules”, in particular for the ones interested in enantiopure primary amines. The potential of secondary amines as catalysts has certainly been known for years. It is indeed more innovative to conduct reactions using primary amine derivatives as catalyst. In this work, the efficacy of the primary amine was checked first. Then, the focus was set on finding optimal reaction conditions. Finally, to have a more complete picture of the structure of the compounds used in the project, experimental and computational IR spectra were compared, after the method was validated. Durante il periodo di tirocinio è stata presa in esame la reazione di α-alchilazione di aldeidi branched, utilizzando un derivato dell’ammina di Betti come catalizzatore enantiopuro ed applicando un nuovo tipo di catalisi: l’organocatalisi. Questi composti possono essere di particolare interesse per lavori in chimica organica, nel campo delle reazioni catalizzate da “piccole” molecole organiche, in particolare da ammine primarie a chiralità definita; la potenzialità delle ammine secondarie chirali come catalizzatori è certamente nota da anni, ma innovativo è condurre il tutto con l’impiego di un derivato amminico primario. Altri aspetti significativi sono gli apparenti e innumerevoli vantaggi, dal punto di vista economico ed ambientale, oltre che operativo e sintetico, derivanti dal nuovo tipo di catalisi. In un primo momento è stata verificata l’efficacia dell’ammina primaria sintetizzata nella reazione in progetto, quindi sono state individuate le condizioni di reazione ottimali. Infine, per un’analisi più completa di alcune molecole organiche e dopo un’opportuna validazione del metodo utilizzato, sono stati ottenuti a livello computazionale gli spettri IR delle molecole di sintesi prodotto e catalizzatore.

High precision radial velocities with giano spectra

Radial velocities measured from near-infrared (NIR) spectra are a potential tool to search for extrasolar planets around cool stars. High resolution infrared spectrographs now available reach the high precision of visible instruments, with a constant improvement over time. GIANO is an infrared echelle spectrograph and it is a powerful tool to provide high resolution spectra for accurate radial velocity measurements of exo-planets and for chemical and dynamical studies of stellar or extragalactic objects. No other IR instruments have the GIANO's capability to cover the entire NIR wavelength range. In this work we develop an ensemble of IDL procedures to measure high precision radial velocities on a few GIANO spectra acquired during the commissioning run, using the telluric lines as wevelength reference. In Section 1.1 various exoplanet search methods are described. They exploit different properties of the planetary system. In Section 1.2 we describe the exoplanet population discovered trough the different methods. In Section 1.3 we explain motivations for NIR radial velocities and the challenges related the main issue that has limited the pursuit of high-precision NIR radial velocity, that is, the lack of a suitable calibration method. We briefly describe calibration methods in the visible and the solutions for IR calibration, for instance, the use of telluric lines. The latter has advantages and problems, described in detail. In this work we use telluric lines as wavelength reference. In Section 1.4 the Cross Correlation Function (CCF) method is described. This method is widely used to measure the radial velocities.In Section 1.5 we describe GIANO and its main science targets. In Chapter 2 observational data obtained with GIANO spectrograph are presented and the choice criteria are reported. In Chapter 3 we describe the detail of the analysis and examine in depth the flow chart reported in Section 3.1. In Chapter 4 we give the radial velocities measured with our IDL procedure for all available targets. We obtain an rms scatter in radial velocities of about 7 m/s. Finally, we conclude that GIANO can be used to measure radial velocities of late type stars with an accuracy close to or better than 10 m/s, using telluric lines as wevelength reference. In 2014 September GIANO is being operative at TNG for Science Verification and more observational data will allow to further refine this analysis.

Towards NIR emission: 2-(1H-tetrazol-1-yl)pyridine as versatile ligand for the synthesis of two new families of cationic and neutral Ir(III) complexes.

In the last decades, cyclometalated Ir(III) complexes have drawn a large interest for their unique properties: they are excellent triplet state emitters, thus the emission is phosphorescent in nature; typically high quantum yields and good stability make them good candidates for luminescent materials. Moreover, through an opportune choice of the ligands, it is possible to tune the emission along the whole visible spectra. Thanks to these interesting features, Ir(III) complexes have found different applications in several areas of applied science, from OLEDs to bioimaging. In particular, regarding the second application, a remarkable red-shift in the emission is required, in order to minimize the problem of the tissue penetration and the possible damages for the organisms. With the aim of synthesizing a new family of NIR emitting Ir(III) complexes, we envisaged the possibility to use for the first time 2-(1H-tetrazol-1-yl)pyridine as bidentate ligand able to provide the required red-shift of the emission of the final complexes. Exploiting the versatility of the ligand, I prepared two different families of heteroleptic Ir(III) complexes. In detail, in the first case the 2-(1H-tetrazol-1-yl)pyridine was used as bis-chelating N^N ligand, leading to cationic complexes, while in the second case it was used as cyclometalating C^N ligand, giving neutral complexes. The structures of the prepared molecules have been characterised by NMR spectroscopy and mass spectrometry. Moreover, the neutral complexes’ emissive properties have been measured: emission spectra have been recorded in solution at both room temperature and 77K, as well as in PMMA matrix. DFT calculation has then been performed and the obtained results have been compared to experimental ones.