Sintesi di 4-bromo-pirazoli quali precursori di sistemi eterociclici condensati. Sintesi della 3a,4,5,6,7,7a-esaidro-N-metil-1H-1,4,6-(epietano-1,1,2-triil)indeno-4,8-dicarbossimmide e di composti relazionati tramite reazione Diels-Alder intramolecolare.

Il progetto di tesi specialistica svolto durante questo anno accademico si è suddiviso in due parti: un primo periodo, da settembre 2010 a gennaio 2011, presso il dipartimento di Chimica Organica “A. Mangini” della Facoltà di Chimica Industriale dell’Università di Bologna e un secondo periodo in Spagna, da marzo ad agosto 2011, presso la Unitat de Química Farmacèutica de la Facultat de Farmàcia de la Universitat de Barcelona. Nel primo periodo a Bologna mi sono occupato della sintesi di 4-bromo-pirazoli da utilizzare come precursori di composti eterociclici condensati. Inizialmente è stato sintetizzato un pirazolo 1,3,5-trisostituito tramite cicloaddizione 1,3-dipolare tra un acetilene e una nitril immina generata in situ da un idrazonoil cloruro. Il pirazolo è stato poi bromurato facendo uno screening di diversi agenti bromuranti e condizioni di reazione per ottenere la migliore resa e chemoselettività. Infine è stata studiata la ciclizzazione intramolecolare del prodotto bromurato tramite reazione di cross-coupling catalizzata da metalli di transizione. Nel secondo periodo a Barcellona mi sono occupato della sintesi di dicarbossimmidi tricicliche con struttura a gabbia con il fine di creare alcheni altamente piramidalizzati e di studiarne la dimerizzazione ad un derivato del dodecaedrano. La strategia sintetica è stata impostata utilizzando come reagente di partenza una semplice succinimmide per giungere, dopo numerosi passaggi, al precursore del prodotto triciclico, del quale è stata studiata la ciclizzazione tramite reazione Diels-Alder intramolecolare.

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.

Constraining FIR size, dust temperature and dust mass in ALPINE galaxies at redshift 4

The study of galaxies at high redshift plays a crucial role to understand the mechanism of galaxy formation and evolution. At redshifts just after the epoch of re-ionization (4nsform from newly-formed objects to more complex structures. In a few hundred Myrs, galaxies increase their stellar mass, change their morphological type and progressively become more obscured due to increased dust attenuation of the UV light. Therefore, determining physical parameters regarding dust is essential to trace the history of the star formation rate (SFR). The main purpose of this thesis is to determine the spatial extent of the dust emission in high-redshift galaxies and to provide a lower limit on dust temperature, to constrain the dust mass. This is achieved by studying 23 FIR continuum detected main-sequence galaxies of the ALMA Large Program to INvestigate (ALPINE) survey, performed at high redshift (4nt of the dust emission, i.e. the dust size, with the stellar and gas distribution, traced by the UV and [CII] emission, respectively. Finally, we put these results in a broader context, by studying the dust size evolution as a function of cosmic time. We derive dust size measurements via a Gaussian fit in the image and uv plane. Out of the 23 FIR-continuum-detected targets, 20 have been considered in this work since they are isolated systems. Of these 20, 7 are spatially resolved; for each of the remaining 13, we provide an upper limit to the dust size. We find that the gas emission is more extended than the dust spatial scale, by a factor of 1.40±0.29, while the latter appears to be larger than the stellar emission size. Moreover, we do not find any significant trend for dust size as a function of the stellar mass and the redshift. In addition, we provide a minimum dust temperature estimate for the 7 resolved sources, for which we find Tmin∼16−19K. We also derive dust masses for the resolved sources, logMdust∼7−8M⊙.

From 3,3,4,4-Tetraethoxybut-1-yne to furan derivatives

The starting material for this project was the highly functionalized compound 3,3,4,4- tetraethoxybut-1-yne (TEB) and it can be prepared from ethyl vinyl ether by a 4-steps synthesis. The third and the fourth step in TEB synthesis were sensitive to reaction conditions, so it was developed a strategy to try to optimize the third step and obtain TEB with higher yields. An approach, which tries to optimize also the fourth step, will be developed in further works. Several γ-hydroxy-α,β-unsaturated acetylenic ketones can be prepared from 3,3,4,4- tetraethoxybut-1-yne. TEB and γ-hydroxy-α,β-unsaturated acetylenic ketones have been previously synthesized in good yields using various reaction routes. In this work will be shown the synthesis of 1,1-diethoxy-5-hydroxyhex-3-yn-2-one, 1,1-diethoxy-5-hydroxyundec-3-yn-2-one and 1,1-diethoxy-5-hydroxydodec-3-yn-2-one, which will react with ethyl acetoacetate to give, respectively, ethyl 4-(3,3-diethoxy-2-oxopropyl)-2,5-dimethylfuran-3-carboxylate, ethyl 4-(3,3-diethoxy-2-oxopropyl)-5-hexyl-2-methylfuran-3-carboxylate and ethyl 4-(3,3-diethoxy-2-oxopropyl)- 5-heptyl-2-methylfuran-3-carboxylate furan derivatives. This thesis project was carried out during the year 2011, at the Department of Chemistry of the University of Bergen.