Estudo da distribuição de tamanho e composição iônica de aerossóis e seus efeitos na capacidade de nuclear gotas de nuvens

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

Uma análise da proposta de formação técnica para o processo de transição agroecológica na escola José Gomes Da Silva, MST-PR

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Dinâmica de campos escalares fora do equilíbrio

Pós-graduação em Física - IFT

Morfologia do testículo e espermatogênese em Telchin licus (Drury, 1773) (Lepidoptera: Castiniidae)

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Evolução morfológica do Rio do Peixe: estudo de uma avulsão na planície aluvial, a partir de uma análise regional integrada - Oeste Paulista (SP)

Pós-graduação em Geografia - FCT

Morfologia do testículo e espermatogênese em Telchin licus (Drury, 1773) (Lepidoptera: Castiniidae)

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Evolução morfológica do Rio do Peixe: estudo de uma avulsão na planície aluvial, a partir de uma análise regional integrada - Oeste Paulista (SP)

Pós-graduação em Geografia - FCT

Archaeofacies Analysis: Using Depositional Attributes to Identify Anthropic Processes of Deposition in a Monumental Shell Mound of Santa Catarina State, Southern Brazil

In the coast of Santa Catarina State (southern Brazil), a large population of monumental shell mounds characterizes a highly dynamic coastal setting. In this paper, sedimentary facies analysis was adapted for description, sampling, and interpretation of shell mound complex and repetitive archaeostratigraphic successions. Archaeofacies identification in the field, according to depositional attributes, is tested by contrasting field description with multi-element chemical analyses, total carbon and nitrogen determinations, and micromorphological descriptions. Two vertical sequences at the black deposit of Jabuticabeira II shell mound were studied and preliminary results showed that: (1) depositional attributes are a reliable base for archaeofacies identification in the field, (2) the formation process of this site involved a sequence of anthropic depositional processes, where burned refuse was redeposited over the shell mound following a ritual construction pattern, and (3) the black deposit includes a double palimpsest that refers to provenance and meaning of mound construction material. (C) 2009 Wiley Periodicals, Inc.

Processo de formação de tenistas talentosos

O objetivo do presente estudo foi obter informações a respeito do processo de formação de tenistas talentosos e os consequentes fatores que contribuíram para o alcance do profissionalismo. Para tanto, se utilizou uma amostra de cinco tenistas brasileiros profissionais, caracterizados por terem pontos na ATP (Associação dos Tenistas Profissionais). A pesquisa foi constituída através de um delineamento qualitativo, que utilizou como instrumento uma entrevista composta por três perguntas abertas, elaboradas para explorar o contexto de formação do talento. Para a análise dos resultados foi utilizado o “Discurso do Sujeito Coletivo”. De acordo com os resultados, pode-se observar a importância que os professores tiveram no desenvolvimento destes tenistas talentosos, tanto na iniciação como no treinamento. No que se diz respeito ao planejamento dos treinos, o presente estudo demonstra a falta de profissionalismo nas fases iniciais do processo de formação, e a posterior preocupação apenas quando este atleta demonstra possuir algum potencial para seguir carreira profissional.

The influence of both urea and 2,2,2

The influence of external agents on proteins function and structure is essential to elucidate the unfolding pathways and self-assemble properties. The knowledge of the protein amyloid fibril formation process is important due to the fields that this subjected is related, in particular for the neurodegenerative disorders. In the present work we studied the influence of both urea and 2,2,2-Trifluoroethanol (TFE) and temperature on the structure and proteinprotein interactions of Bovine Serum Albumin (BSA), by means of UV-Vis spectroscopy, static fluorescence and small angle X-ray scattering technique. The experiments were performed in samples composed by 10 and 3 mg/ml of BSA at pH 5.8, near the protein pI. First, Thioflavin-T fluorescence measurements indicated that urea, in the absence of TFE, was able to increase the amyloid fibril formation of BSA at 45oC and increasing the urea concentration the rate of amyloid fibril formation also increases. Concerning the presence of TFE, SAXS data suggest that BSA tridimensional structure is not altered by the presence of TFE 5% and 10% v/v in all studied protein concentrations. Interestingly, the presence of TFE on the urea-containing BSA also increases the rate of amyloid fibril formation, as compared to the TFE-free system, indicating that TFE can catalyze the amyloid-fibril formation. The presence of TFE 20% v/v, however, induces the formation of aggregates, but at this time we were not able to infer if such aggregates are amyloidlike or amorphous. Taking together, the results give support to infer that BSA can for fibrils in the presence of urea at 45oC and TFE can act as a stabilizer or as a denaturant agent for BSA.

Statistical properties of Radio Halos and the re-acceleration model

Galaxy clusters occupy a special position in the cosmic hierarchy as they are the largest bound structures in the Universe. There is now general agreement on a hierarchical picture for the formation of cosmic structures, in which galaxy clusters are supposed to form by accretion of matter and merging between smaller units. During merger events, shocks are driven by the gravity of the dark matter in the diffuse barionic component, which is heated up to the observed temperature. Radio and hard-X ray observations have discovered non-thermal components mixed with the thermal Intra Cluster Medium (ICM) and this is of great importance as it calls for a “revision” of the physics of the ICM. The bulk of present information comes from the radio observations which discovered an increasing number of Mpcsized emissions from the ICM, Radio Halos (at the cluster center) and Radio Relics (at the cluster periphery). These sources are due to synchrotron emission from ultra relativistic electrons diffusing through µG turbulent magnetic fields. Radio Halos are the most spectacular evidence of non-thermal components in the ICM and understanding the origin and evolution of these sources represents one of the most challenging goal of the theory of the ICM. Cluster mergers are the most energetic events in the Universe and a fraction of the energy dissipated during these mergers could be channelled into the amplification of the magnetic fields and into the acceleration of high energy particles via shocks and turbulence driven by these mergers. Present observations of Radio Halos (and possibly of hard X-rays) can be best interpreted in terms of the reacceleration scenario in which MHD turbulence injected during these cluster mergers re-accelerates high energy particles in the ICM. The physics involved in this scenario is very complex and model details are difficult to test, however this model clearly predicts some simple properties of Radio Halos (and resulting IC emission in the hard X-ray band) which are almost independent of the details of the adopted physics. In particular in the re-acceleration scenario MHD turbulence is injected and dissipated during cluster mergers and thus Radio Halos (and also the resulting hard X-ray IC emission) should be transient phenomena (with a typical lifetime <» 1 Gyr) associated with dynamically disturbed clusters. The physics of the re-acceleration scenario should produce an unavoidable cut-off in the spectrum of the re-accelerated electrons, which is due to the balance between turbulent acceleration and radiative losses. The energy at which this cut-off occurs, and thus the maximum frequency at which synchrotron radiation is produced, depends essentially on the efficiency of the acceleration mechanism so that observations at high frequencies are expected to catch only the most efficient phenomena while, in principle, low frequency radio surveys may found these phenomena much common in the Universe. These basic properties should leave an important imprint in the statistical properties of Radio Halos (and of non-thermal phenomena in general) which, however, have not been addressed yet by present modellings. The main focus of this PhD thesis is to calculate, for the first time, the expected statistics of Radio Halos in the context of the re-acceleration scenario. In particular, we shall address the following main questions: • Is it possible to model “self-consistently” the evolution of these sources together with that of the parent clusters? • How the occurrence of Radio Halos is expected to change with cluster mass and to evolve with redshift? How the efficiency to catch Radio Halos in galaxy clusters changes with the observing radio frequency? • How many Radio Halos are expected to form in the Universe? At which redshift is expected the bulk of these sources? • Is it possible to reproduce in the re-acceleration scenario the observed occurrence and number of Radio Halos in the Universe and the observed correlations between thermal and non-thermal properties of galaxy clusters? • Is it possible to constrain the magnetic field intensity and profile in galaxy clusters and the energetic of turbulence in the ICM from the comparison between model expectations and observations? Several astrophysical ingredients are necessary to model the evolution and statistical properties of Radio Halos in the context of re-acceleration model and to address the points given above. For these reason we deserve some space in this PhD thesis to review the important aspects of the physics of the ICM which are of interest to catch our goals. In Chapt. 1 we discuss the physics of galaxy clusters, and in particular, the clusters formation process; in Chapt. 2 we review the main observational properties of non-thermal components in the ICM; and in Chapt. 3 we focus on the physics of magnetic field and of particle acceleration in galaxy clusters. As a relevant application, the theory of Alfv´enic particle acceleration is applied in Chapt. 4 where we report the most important results from calculations we have done in the framework of the re-acceleration scenario. In this Chapter we show that a fraction of the energy of fluid turbulence driven in the ICM by the cluster mergers can be channelled into the injection of Alfv´en waves at small scales and that these waves can efficiently re-accelerate particles and trigger Radio Halos and hard X-ray emission. The main part of this PhD work, the calculation of the statistical properties of Radio Halos and non-thermal phenomena as expected in the context of the re-acceleration model and their comparison with observations, is presented in Chapts.5, 6, 7 and 8. In Chapt.5 we present a first approach to semi-analytical calculations of statistical properties of giant Radio Halos. The main goal of this Chapter is to model cluster formation, the injection of turbulence in the ICM and the resulting particle acceleration process. We adopt the semi–analytic extended Press & Schechter (PS) theory to follow the formation of a large synthetic population of galaxy clusters and assume that during a merger a fraction of the PdV work done by the infalling subclusters in passing through the most massive one is injected in the form of magnetosonic waves. Then the processes of stochastic acceleration of the relativistic electrons by these waves and the properties of the ensuing synchrotron (Radio Halos) and inverse Compton (IC, hard X-ray) emission of merging clusters are computed under the assumption of a constant rms average magnetic field strength in emitting volume. The main finding of these calculations is that giant Radio Halos are naturally expected only in the more massive clusters, and that the expected fraction of clusters with Radio Halos is consistent with the observed one. In Chapt. 6 we extend the previous calculations by including a scaling of the magnetic field strength with cluster mass. The inclusion of this scaling allows us to derive the expected correlations between the synchrotron radio power of Radio Halos and the X-ray properties (T, LX) and mass of the hosting clusters. For the first time, we show that these correlations, calculated in the context of the re-acceleration model, are consistent with the observed ones for typical µG strengths of the average B intensity in massive clusters. The calculations presented in this Chapter allow us to derive the evolution of the probability to form Radio Halos as a function of the cluster mass and redshift. The most relevant finding presented in this Chapter is that the luminosity functions of giant Radio Halos at 1.4 GHz are expected to peak around a radio power » 1024 W/Hz and to flatten (or cut-off) at lower radio powers because of the decrease of the electron re-acceleration efficiency in smaller galaxy clusters. In Chapt. 6 we also derive the expected number counts of Radio Halos and compare them with available observations: we claim that » 100 Radio Halos in the Universe can be observed at 1.4 GHz with deep surveys, while more than 1000 Radio Halos are expected to be discovered in the next future by LOFAR at 150 MHz. This is the first (and so far unique) model expectation for the number counts of Radio Halos at lower frequency and allows to design future radio surveys. Based on the results of Chapt. 6, in Chapt.7 we present a work in progress on a “revision” of the occurrence of Radio Halos. We combine past results from the NVSS radio survey (z » 0.05 − 0.2) with our ongoing GMRT Radio Halos Pointed Observations of 50 X-ray luminous galaxy clusters (at z » 0.2−0.4) and discuss the possibility to test our model expectations with the number counts of Radio Halos at z » 0.05 − 0.4. The most relevant limitation in the calculations presented in Chapt. 5 and 6 is the assumption of an “averaged” size of Radio Halos independently of their radio luminosity and of the mass of the parent clusters. This assumption cannot be released in the context of the PS formalism used to describe the formation process of clusters, while a more detailed analysis of the physics of cluster mergers and of the injection process of turbulence in the ICM would require an approach based on numerical (possible MHD) simulations of a very large volume of the Universe which is however well beyond the aim of this PhD thesis. On the other hand, in Chapt.8 we report our discovery of novel correlations between the size (RH) of Radio Halos and their radio power and between RH and the cluster mass within the Radio Halo region, MH. In particular this last “geometrical” MH − RH correlation allows us to “observationally” overcome the limitation of the “average” size of Radio Halos. Thus in this Chapter, by making use of this “geometrical” correlation and of a simplified form of the re-acceleration model based on the results of Chapt. 5 and 6 we are able to discuss expected correlations between the synchrotron power and the thermal cluster quantities relative to the radio emitting region. This is a new powerful tool of investigation and we show that all the observed correlations (PR − RH, PR − MH, PR − T, PR − LX, . . . ) now become well understood in the context of the re-acceleration model. In addition, we find that observationally the size of Radio Halos scales non-linearly with the virial radius of the parent cluster, and this immediately means that the fraction of the cluster volume which is radio emitting increases with cluster mass and thus that the non-thermal component in clusters is not self-similar.

Kontrollierte Fällung von amorphem Calciumcarbonat durch homogene Carbonatfreisetzung

In der Vergangenheit haben Untersuchung an biologischen und Modell-Systemen gezeigt, dass amorphes Calciumcarbonat als instabiles Zwischenprodukt bei der Bildung kristalliner Strukturen aus CaCO3 auftritt. Über dessen Rolle im Fällungsprozess von CaCO3 ist nicht viel bekannt und es wird davon ausgegangen, dass es als CaCO3-Speicher für die nachfolgenden kristallinen Produkte dient. Der genaue Reaktionsablauf, der zur Bildung von amorphem Calciumcarbonat (ACC) führt, ist nicht bekannt. Ziel dieser Arbeit war die Entwicklung einer Fällungstechnik, die die Beobachtung der Bildungskinetik von ACC durch Lichtstreuung ermöglicht. In Fällungsexperimenten wird gezeigt, dass die Fällung unter nicht-turbulenten Bedingungen zur Bildung von amorphem Calciumcarbonat führt. Hinsichtlich der Basen- und Alkylcarbonatmenge, die äquivalent oder im Überschuss zur Calciumionenkonzentration eingesetzt wird, entstehen zwei verschiedene Fällungsprodukte. In Bezug auf ihre chemische Zusammensetzung, thermische und mechanische Eigenschaften werden diese charakterisiert. In beiden Fällen wird ein amorphes CaCO3 mit einem Wassergehalt von 0,5 mol/L pro Mol CaCO3 erhalten. Die in situ Generierung von Carbonat führt zur Bildung von sphärischem amorphem Calciumcarbonat, das eine gewisse Tendenz zur Koazervation zeigt. Die bei gleichem Reaktionsumsatz beobachtete Temperaturabhängigkeit des Partikelradius konnten wir unter Annahme einer Mischungslücke mit unterer kritischer Mischungstemperatur interpretieren. Für die Bildung von amorphem Calciumcarbonat schlagen wir daher einen Mechanismus via binodaler flüssig-flüssig Entmischung vor. Nach einer kurzen Keimbildungsperiode können flüssige Tröpfchen aus wasserhaltigem CaCO3 wachsen und dann infolge von stetigem Wasserverlust glasartig erstarren und so amorphes Calciumcarbonat bilden. Bekräftigt wird dieses Modell durch die Wachstumskinetik, die mittels Lichtstreuung und SAXS verfolgt worden ist. In den Fällungsversuchen sind je nach Reaktionsbedingungen, zwei verschiedene Zeitgesetze des Teilchenwachstums erkennbar: Bei schneller Freisetzung von Carbonat liegt ein parabolischer Verlauf des Radienwachstums vor; hingegen führt eine langsame Freisetzung von Carbonat zu einem linearen Wachstum der Radien. Diese Abhängigkeiten lassen sich im Rahmen der bekannten Kinetik einer flüssig-flüssig Entmischung deuten. Ferner wird der Einfluss von doppelthydrophilen Blockcopolymeren (PEO-PMAA) auf die Teilchengröße und die Kinetik der Bildung von amorphem Calciumcarbonat untersucht. Zum Einsatz kommen zwei verschiedene Blockcopolymere, die sich in der Länge des PEO-Blocks unterscheiden. Im Fällungsexperiment führt das in sehr kleinen Konzentrationen vorliegende Blockcopolymere zur Stabilisierung von kleineren Partikeln. Das Blockcopolymer mit der längeren PEO-Einheit weist eine größere Effizienz auf. Die Ergebnisse lassen sich durch Annahme von Adsorption des Polymers an der Oberfläche interpretieren. Der Einfluss der doppelthydrophilen Blockcopolymere auf die Bildung von ACC deutet darauf, dass amorphes Calciumcarbonat eine komplexere Rolle als lediglich die eines Calciumcarbonatspeichers für das spätere Wachstum kristalliner Produkte einnimmt. Für die Wirkung von Polymerzusätzen muss somit nicht nur die Wechselwirkung mit den gegen Ende gebildeten Kristalle betrachtet werden, sondern auch der Einfluss, den das Polymer auf die Bildung des amorphen Calciumcarbonats hat. Die hier neu entwickelte Methode bietet die Möglichkeit, auch für komplexere Polymere, wie z.B. extrahierte Proteine, den Einfluss auf die Bildung der amorphen Vorstufe zu untersuchen.

Photonen-Aufkonversion in Nanokapseln

Die vorliegende Dissertation zeigt eine erfolgreiche Verknüpfung der Triplett-Triplett-Annihilations-Aufkonversion (TTA-UC) mit möglichen biologischen Anwendungen. Die Grundlage für solche Anwendungen ist ein Transfer der TTA-UC aus seinem üblicherweise verwendeten organischen Medium in eine wässrige Umgebung. Um diesen Transfer zu realisieren, wurden, unter Anwendung der Technik des Miniemulsionsprozesses, in Wasser dispergierte Nanokapseln herstellt. Der Kern dieser Nanokapseln besteht aus einem flüssigen hydrophoben Medium (meist Hexadekan oder Phenylheptadekan), in dem die zur TTA-UC notwendigen Farbstoffe gelöst sind. Dieser flüssige Kern ist vollständig von einer festen Polymerhülle umschlossen und somit isoliert von seiner wässrigen Umgebung. Es wurden insgesamt drei Generationen solcher Nanokapseln hergestellt, die sich hauptsächlich im Herstellungsprozess, aber auch beim Material von Kern und Hülle unterscheiden. Mittels dieser Variationen konnten die Nanokapseln in Bezug auf Effizienz, Anregungswellenlänge und Sauerstoffempfindlichkeit optimiert werden. Bei der ersten Generation wurde die radikalische Miniemulsionspolymerisation zur Kapselbildung verwendet. Die zweite Generation wurde durch die Kombination des Lösungsmittelverdampfungsprozesses mit dem Miniemulsionsprozess entwickelt und liefert somit eine alternative Möglichkeit der Kapselbildung unter milden Reaktionsbedingungen, was eine uneingeschränkte Auswahl der UC-Farbstoffpaare ermöglicht. Durch den Einsatz unterschiedlicher Sensitizer konnte die Anregungswellenlänge der TTA-UC in den roten und in den nahen Infrarot-Bereich des sichtbaren Spektrums verschoben werden. Diese Verschiebung ist im biologischen Anwendungsbereich von enormer Bedeutung, da dort eine Überlappung mit dem natürlichen optischen Fenster von menschlicher Haut und Gewebe stattfindet. Dies reduziert die Streuung der Anregungsquelle im zu untersuchende Medium und ermöglicht hohe Eindringtiefen. Mit den Kapseln der zweiten Generation wurde zum ersten Mal TTA-UC in lebenden HeLa-Zellen (Krebszellen) und MSCs (Mesenchymale Stammzellen) nachgewiesen. Die verzögerte Fluoreszenz aus den Zellen wurde mit biologischen Standardverfahren, sowohl mit der Durchflusszytometrie (FACS) als auch am cLSM nachgewiesen. Besondere Vorteile gegenüber direkter Fluoreszenz konnten bei der Bildgebung von Zellen erreicht werden. Die relativ energiearme Anregungswellenlänge und die dazu anti-Stokes verschobene, detektierte verzögerte UC-Fluoreszenz lieferte eine bessere Bildqualität und eine sehr geringe Phototoxizität der Zellen. Die Kapseln der dritten Generation zeichnen sich durch ihre anorganische, tetraedrisch verknüpfte SiO2-Hülle aus und wurden mittels einer Grenzflächenreaktion (Sol-Gel-Prozess) in Miniemulsion hergestellt. Diese Kapseln weisen im Vergleich zu den Polymernanokapseln eine bessere UC-Effizienz auf und sind zusätzlich stabiler und robuster.

Aerosol-cloud interactions studied with a chemistry-climate model

This study aims at a comprehensive understanding of the effects of aerosol-cloud interactions and their effects on cloud properties and climate using the chemistry-climate model EMAC. In this study, CCN activation is regarded as the dominant driver in aerosol-cloud feedback loops in warm clouds. The CCN activation is calculated prognostically using two different cloud droplet nucleation parameterizations, the STN and HYB CDN schemes. Both CDN schemes account for size and chemistry effects on the droplet formation based on the same aerosol properties. The calculation of the solute effect (hygroscopicity) is the main difference between the CDN schemes. The kappa-method is for the first time incorporated into Abdul-Razzak and Ghan activation scheme (ARG) to calculate hygroscopicity and critical supersaturation of aerosols (HYB), and the performance of the modied scheme is compared with the osmotic coefficient model (STN), which is the standard in the ARG scheme. Reference simulations (REF) with the prescribed cloud droplet number concentration have also been carried out in order to understand the effects of aerosol-cloud feedbacks. In addition, since the calculated cloud coverage is an important determinant of cloud radiative effects and is influencing the nucleation process two cloud cover parameterizations (i.e., a relative humidity threshold; RH-CLC and a statistical cloud cover scheme; ST-CLC) have been examined together with the CDN schemes, and their effects on the simulated cloud properties and relevant climate parameters have been investigated. The distinct cloud droplet spectra show strong sensitivity to aerosol composition effects on cloud droplet formation in all particle sizes, especially for the Aitken mode. As Aitken particles are the major component of the total aerosol number concentration and CCN, and are most sensitive to aerosol chemical composition effect (solute effect) on droplet formation, the activation of Aitken particles strongly contribute to total cloud droplet formation and thereby providing different cloud droplet spectra. These different spectra influence cloud structure, cloud properties, and climate, and show regionally varying sensitivity to meteorological and geographical condition as well as the spatiotemporal aerosol properties (i.e., particle size, number, and composition). The changes responding to different CDN schemes are more pronounced at lower altitudes than higher altitudes. Among regions, the subarctic regions show the strongest changes, as the lower surface temperature amplifies the effects of the activated aerosols; in contrast, the Sahara desert, where is an extremely dry area, is less influenced by changes in CCN number concentration. The aerosol-cloud coupling effects have been examined by comparing the prognostic CDN simulations (STN, HYB) with the reference simulation (REF). Most pronounced effects are found in the cloud droplet number concentration, cloud water distribution, and cloud radiative effect. The aerosol-cloud coupling generally increases cloud droplet number concentration; this decreases the efficiency of the formation of weak stratiform precipitation, and increases the cloud water loading. These large-scale changes lead to larger cloud cover and longer cloud lifetime, and contribute to high optical thickness and strong cloud cooling effects. This cools the Earth's surface, increases atmospheric stability, and reduces convective activity. These changes corresponding to aerosol-cloud feedbacks are also differently simulated depending on the cloud cover scheme. The ST-CLC scheme is more sensitive to aerosol-cloud coupling, since this scheme uses a tighter linkage of local dynamics and cloud water distributions in cloud formation process than the RH-CLC scheme. For the calculated total cloud cover, the RH-CLC scheme simulates relatively similar pattern to observations than the ST-CLC scheme does, but the overall properties (e.g., total cloud cover, cloud water content) in the RH simulations are overestimated, particularly over ocean. This is mainly originated from the difference in simulated skewness in each scheme: the RH simulations calculate negatively skewed distributions of cloud cover and relevant cloud water, which is similar to that of the observations, while the ST simulations yield positively skewed distributions resulting in lower mean values than the RH-CLC scheme does. The underestimation of total cloud cover over ocean, particularly over the intertropical convergence zone (ITCZ) relates to systematic defficiency of the prognostic calculation of skewness in the current set-ups of the ST-CLC scheme.rnOverall, the current EMAC model set-ups perform better over continents for all combinations of the cloud droplet nucleation and cloud cover schemes. To consider aerosol-cloud feedbacks, the HYB scheme is a better method for predicting cloud and climate parameters for both cloud cover schemes than the STN scheme. The RH-CLC scheme offers a better simulation of total cloud cover and the relevant parameters with the HYB scheme and single-moment microphysics (REF) than the ST-CLC does, but is not very sensitive to aerosol-cloud interactions.

Fabrication of cone-shaped boron doped diamond and gold nanoelectrodes for AFM-SECM

We demonstrate a reliable microfabrication process for a combined atomic force microscopy (AFM) and scanning electrochemical microscopy (SECM) measurement tool. Integrated cone-shaped sensors with boron doped diamond (BDD) or gold (Au) electrodes were fabricated from commercially available AFM probes. The sensor formation process is based on mature semiconductor processing techniques, including focused ion beam (FIB) machining, and highly selective reactive ion etching (RIE). The fabrication approach preserves the geometry of the original AFM tips resulting in well reproducible nanoscaled sensors. The feasibility and functionality of the fully featured tips are demonstrated by cyclic voltammetry, showing good agreement between the measured and calculated currents of the cone-shaped AFM-SECM electrodes.