Fabrication of 2D and 3D microelectrode arrays for amperometric dopamine sensing: towards a metal free approach to bioelectronics

Dopamine is a neurotransmitter which has a role in several psychiatric and neurological disorders. In-vivo detection of its concentration at the microscopic scale would benefit the study of these conditions and help in the development of therapies. The ideal sensor would be biocompatible, able to probe concentrations in microscopic volumes and sensitive to the small physiological concentrations of this molecule (10 nM - 1 μM). The ease of oxidation of dopamine makes it possible to detect it by electrochemical methods. An additional requirement in this kind of experiments when run in water, though, is to have a large potential window inside which no redox reactions with water take place. A promising class of materials which are being explored is the one of pyrolyzed photoresists. Photoresists can be lithographically patterned with micrometric resolution and after pyrolysis leave a glassy carbon material which is conductive, biocompatible and has a large electrochemical water window. In this work I developed a fabrication procedure for microelectrode arrays with three dimensional electrodes, making the whole device using just a negative photoresist called SU8. Making 3D electrodes could be a way to enhance the sensitivity of the electrodes without occupying a bigger footprint on the device. I characterized the electrical, morphological, and electrochemical properties of these electrodes, in particular their sensitivity to dopamine. I also fabricated and tested a two dimensional device for comparison. The three dimensional devices fabricated showed inferior properties to their two dimensional counter parts. I found a possible explanation and suggested some ways in which the fabrication could be improved.

Synthesis and Characterization of Double Metal Hexacyanoferrates

Manganese Hexacyanoferrate (MnHCF) and nickel doped manganese hexacyanoferrate were synthesized by simple co-precipitation method. The water content and chemical formula was obtained by TGA and MP-AES measurements, functional groups by FT-IR analysis, the crystal structure by PXRD and a local geometry by XAS. Elemental species of cycled samples were further investigated by TXM and 2D XRF. Electrochemical tests were performed in the glass cell. With addition of nickel, vacancies and water content increased in the sample. Crystal structure changed from monoclinic to cubic. Ni disturbed the local structure of Mn, site, however, almost no change was observed in Fe site. After charge/discharge cycling of MnHCF intercalation was already found in the peripheries of charged species after 20 cycle in 2D XRF analysis and randomly distributed intercalated regions after 50 cycles in TXM analysis. Cyclic voltammetry showed that peak-to-peak separation is increasing in case of the addition of Ni to MnHCF.

Catalytic reduction of organic pollutants using supported metal nanoparticles

Metal nanoparticle catalysts have in the last decades been extensively researched for their enhanced performance compared to their bulk counterpart. Properties of nanoparticles can be controlled by modifying their size and shape as well as adding a support and stabilizing agent. In this study, preformed colloidal gold nanoparticles supported on activated carbon were tested on the reduction of 4-nitrophenol by NaBH4, a model reaction for evaluating catalytic activity of metal nanoparticles and one with high significance in the remediation of industrial wastewaters. Methods of wastewater remediation are reviewed, with case studies from literature on two major reactions, ozonation and reduction, displaying the synergistic effects observed with bimetallic and trimetallic catalysts, as well as the effects of differences in metal and support. Several methods of preparation of nanoparticles are discussed, in particular, the sol immobilization technique, which was used to prepare the supported nanoparticles in this study. Different characterization techniques used in this study to evaluate the materials and spectroscopic techniques to analyze catalytic activities of the catalyst are reviewed: ultraviolet-visible (UV-Vis) spectroscopy, dynamic light scattering (DLS) analysis, X-ray diffraction (XRD) analysis and transmission electron microscopy (TEM) imaging. Optimization of catalytic parameters was carried out through modifications in the reaction setup. The effects of the molar ratio of reactants, stirring, type and amount of stabilizing agent are explored. Another important factor of an effective catalyst is its reusability and long-term stability, which was examined with suggestions for further studies. Lastly, a biochar support was newly tested for its potential as a replacement for activated carbon.

Abbondanze chimiche in un campione di stelle metal-poor della galassia nana del Sagittario

Lo scenario oggi più accreditato per spiegare la formazione delle galassie è quello del merging gerarchico: Sgr è una delle prove più importanti a favore di questo scenario. Sgr è una galassia satellite della MW ed è il caso migliore di processo di distruzione mareale in corso dalla MW. La sua distruzione ha contribuito alla costituzione dell'alone della Via Lattea. Di Sgr si osserva solo ciò che ne rimane del corpo principale, i suoi streams ed il suo nucleo, dominato dall'ammasso metal-poor M54. È la presenza di M54 che rende complessa la selezione di stelle metal-poor di Sgr: il main-body di Sgr è rarefatto e fortemente contaminato da stelle galattiche ed il suo nucleo si sovrappone con M54 rendendo quasi impossibile identificare stelle di Sagittario metal-poor non appartenenti ad M54. Fino ad ora l'unico metodo utilizzato per selezionare i targets per studiare la chimica di Sgr ha fatto uso della loro posizione sul CMD: questo metodo introduce un bias, selezionando solo le stelle metal-rich di Sgr. In questo lavoro sono state studiate 23 stelle metal-poor appartenenti al main-body di Sgr ma fuori dal raggio mareale di M54 selezionate grazie ai moti propri dalla missione GAIA. Gli spettri analizzati sono stati ottenuti con lo spettrografo UVES-FLAMES del VLT (ESO)da cui è stata ottenuta l'abbondanza di 17 elementi sia di stelle di Sgr che in 12 stelle di M54. Questo campione di abbondanze chimiche permette per la prima volta: (a) di comprendere la storia di arricchimento chimico di Sgr in un ampio range di metallicità (mai studiato finora) e (b) di confrontare la chimica di Sgr con quella di M54. Tali abbondanze dimostrano come Sgr abbia avuto un'evoluzione chimica diversa da quella della MW, con un contributo inferiore da parte di stelle massive, probabilmente a causa del suo basso SFR. Inoltre è stato possibile determinare la forte somiglianza chimica tra Sgr e M54, confermando che i due sistemi condividono la stessa storia di arricchimento chimico.