424 resultados para INTERSTRAND STACKED PYRENES


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Das metastasierende maligne Melanom ist durch eine geringe p53-Mutations-Rate und eine hohe Resistenz gegenüber Chemotherapie mit alkylierenden Agenzien wie Fotemustin (FM) und Temozolomid (TMZ) gekennzeichnet. In der vorliegenden Arbeit wurde die Rolle von p53 in der Resistenz von malignen Melanomzellen gegenüber FM untersucht und Möglichkeiten zur Sensitivierung von Melanomzellen gegenüber TMZ und FM aufgezeigt.rnAusgangspunkt war die Beobachtung, dass p53 Wildtyp (p53wt) Melanomzellen resistenter gegenüber FM sind als p53 mutierte (p53mt) Zellen. In der vorliegenden Arbeit wurde gezeigt, dass eine FM-Behandlung in p53wt Zellen eine Stabilisierung von p53 und eine Induktion des p53-Zielproteins p21 bewirkte. Mithilfe einer p53wt Zelllinie, welche einen p53 Knockdown trägt, konnte gezeigt werden, dass p53 für die geringe Apoptose-Rate nach FM-Behandlung verantwortlich ist. Eine Untersuchung der Interstrang-Crosslink (ICL)-Reparaturkapazität zeigte, dass p53mt Zellen im Gegensatz zu p53wt Zellen nicht in der Lage sind, FM-induzierte ICL zu reparieren. Dies ging mit einer im Vergleich zu p53wt Zellen starken DNA-Schadensantwort einher. Die Gene für die Proteine DDB2 und XPC wurden als durch FM regulierte DNA-Reparatur-Gene identifiziert, deren Induktion p53-abhängig und lang anhaltend (bis zu 144 h) erfolgt. Da XPC Knockdown-Zellen sensitiver als ihre Kontrollzellen gegenüber FM reagierten, konnte die biologische Relevanz von XPC bei der ICL-Reparatur bestätigt werden. Anhand von Xenograft-Tumoren wurde gezeigt, dass FM auch in situ eine Induktion von DDB2 und XPC auslöst. Die Beobachtung, dass DNA-Reparatur-Gene nach FM-Behandlung hochreguliert werden, liefert eine Erklärung für das schlechte Ansprechen von Melanomen auf eine Therapie mit ICL-induzierenden Chemotherapeutika.rnDes Weiteren befasste sich die vorliegende Arbeit mit Möglichkeiten zur Sensitivierung von Melanomzellen gegenüber den Chemotherapeutika TMZ und FM. In diesem Zusammenhang wurde Valproinsäure (VPA), ein in der Epilepsie-Therapie verwendetes Medikament und Histondesacetylase (HDAC)-Hemmer, bezüglich der chemosensitivierenden Wirkung untersucht. Zunächst konnte der in der Literatur häufig beschriebene stabilisierende Effekt von VPA auf „wildtypisches“ p53-Protein und destabilisierende Effekt auf mutiertes p53-Protein bestätigt werden. Zwei der vier untersuchten Zelllinien konnten mithilfe von VPA gegenüber TMZ sensitiviert werden, während nur eine der vier untersuchten Zelllinien gegenüber FM sensitiviert werden konnte. VPA begünstigt die Induktion von Apoptose, während der Effekt auf die Induktion von Nekrose nur gering ausfiel. Eine Wirkung von VPA auf die Aktivität des Resistenz-vermittelnden Enzyms O6-Methylguanin-DNA-Methyltransferase (MGMT) wurde nicht beobachtet. Zudem wurde ausgeschlossen, dass die Sensitivierung gegenüber TMZ und FM, welche S-Phase abhängige Gentoxine sind, auf einer VPA-induzierten Erhöhung der Proliferation beruht. Mithilfe einer Zelllinie, welche stabil dominant-negatives FADD (Fas-associated death domain) exprimiert, konnten keine Hinweise auf eine Beteiligung des extrinsischen Apoptose-Signalwegs an der VPA-vermittelten Sensitivierung gewonnen werden. Gleichzeitig wurde gezeigt, dass VPA keine Induktion der niedrig exprimierten Procaspase-8 verursachte. Mithilfe eines PCR-Arrays wurden transaktivierende und –reprimierende Effekte von VPA auf die Genexpression gezeigt, wobei das proapoptotische Protein BAX (Breakpoint cluster-2-associated x protein) als ein in der Sensitivierung involviertes Kandidatengen identifiziert wurde. Obwohl eine vollständige Aufklärung der dem Sensitivierungseffekt von VPA zu Grunde liegenden Mechanismen nicht erbracht werden konnte, zeigen die in dieser Arbeit erlangten Beobachtungen einen vielversprechenden Weg zur Überwindung der Resistenz von Melanomzellen gegenüber DNA-alkylierenden Zytostatika auf.rn

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Metastasierender Krebs ist bei Erwachsenen in der Regel nicht heilbar. Eine Ausnahme stellen testikuläre Keimzelltumoren (TKZT) dar, da über 75 % der Patienten mit fortgeschrittenen metastasierenden TKZT mit einer auf Cisplatin basierenden Kombinations-Chemotherapie geheilt werden können. Zelllinien, die aus TKZT isoliert wurden, behalten diese Cisplatin-Sensitivität in vitro bei. Somit spiegeln Testistumorzelllinien die klinische Situation wider und sind deswegen ein gutes Modellsystem um zu untersuchen, welche Faktoren der Cisplatin-Sensitivität zugrunde liegen. Die Ursachen der Cisplatin-Sensitivität in Testistumoren sind nicht bekannt. Es wurde bereits gezeigt, dass Testistumorzellen eine geringe Kapazität für die Entfernung von Cisplatin-induzierten DNA-Platinierungen aufweisen. Dieser Defekt in der DNA-Reparatur könnte ein Faktor für die beobachtete Cisplatin-Sensitivität sein. Cisplatin induziert sowohl Intrastrang-Vernetzungen als auch Interstrang-Vernetzungen (ICLs). Die Bildung und Reparatur der Cisplatin-induzierten Intrastrang-Vernetzungen wurde mittels DNA-Slot-Blot, die Bildung und Entfernung von Interstrang-Vernetzungen wurde mithilfe des Comet-Assays untersucht. In der vorliegenden Arbeit wurde gezeigt, dass die Reparatur von Intrastrang-Vernetzungen in Testis- und Blasentumorzelllinien vergleichbar ist. Somit sind Testistumorzellen in diesem Reparaturweg nicht beeinträchtigt. Im Unterschied dazu zeigte sich, dass Testistumorzellen die ICLs nicht oder nur mit einer reduzierten Kapazität entfernen können.Da die ICL-Reparatur über die Bildung von DNA-Doppelstrangbrüchen (DSB) mit anschließender DSB-Reparatur verläuft, wurde die Kinetik der DSB-Reparatur anhand der Immundetektion der Histon-Variante γH2AX, die zur Visualisierung von DSB verwendet wird, verfolgt. γH2AX Foci wurden nach Behandlung mit Cisplatin in Testistumorzellen und Blasentumorzellen gebildet. Anders als in Blasentumorzellen blieb der Prozentsatz an γH2AX-positiven Zellen in Testistumorzellen bestehen. Offensichtlich konnten die Testistumorzellen die Cisplatin-induzierten ICLs nicht korrekt prozessieren, was dazu führte, dass γH2AX Foci persistierten. Da unreparierte DNA-Läsionen eine DNA-schadensabhängige Antwort einleiten können, wurde die Aktivierung der Hauptfaktoren dieser Signalwege untersucht. In den Testistumorzellen zeigte sich eine Erhöhung der p53 Proteinmenge nach Cisplatin-Behandlung. Des Weiteren wurde die durch Cisplatin induzierte Aktivierung von ATM/ATR, Chk1/Chk2, Bax und Noxa in Testis- und Blasentumorzellen vergleichend untersucht. Es wurde bereits gezeigt, dass der Reparaturfaktor ERCC1-XPF in Testistumorzelllinien reduziert vorliegt. Um eine mögliche Rolle von ERCC1-XPF für die Reparatur-Defizienz der ICLs und Cisplatin-Sensitivität in Testistumorzellen zu analysieren, wurde ERCC1-XPF in der Testistumorenzelllinie 833K mithilfe eines Expressionsvektors überexprimiert, und der Einfluss von ERCC1-XPF auf ICL-Reparatur sowie Cisplatin-Sensitivität wurde ermittelt. Überexpression von ERCC1-XPF führte zur Reparatur der ICLs in 833K-Zellen und verminderte die Cisplatinsensitivität. Somit scheint die Cisplatinsensitivität der Testistumorzellen, zumindest zum Teil, auf einer verminderten ICL-Reparatur zu beruhen. Des Weiteren wurde in „proof of principle“ Experimenten ERCC1-XPF in der Cisplatin-resistenten Blasentumorzelllinie MGH-U1 mittels siRNA herunterreguliert, und die Auswirkung der Herunterregulation auf die ICL-Reparatur und die Cisplatinsensitivität wurde geprüft. RNA-Interferenz-vermittelte Herunterregulierung von ERCC1-XPF reduzierte die Prozessierung der Cisplatin-induzierten ICLs und verstärkte die Cisplatinsensitivität in MGH-U1 Zellen. Somit wurde in dieser Arbeit zum ersten Mal gezeigt, dass die Testistumorzellen in Vergleich zu Blasentumorzellen in der Reparatur von ICLs defizient sind, wobei die verminderte ICL-Reparatur auf die geringe Expression von ERCC1-XPF zurückgeführt werden konnte. Diese ICL-Reparatur-Defizienz könnte, zumindest zu einem Teil, für die Sensitivität der Testistumoren gegenüber Cisplatin verantwortlich sein.

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Holding the major share of stellar mass in galaxies and being also old and passively evolving, early-type galaxies (ETGs) are the primary probes in investigating these various evolution scenarios, as well as being useful means to provide insights on cosmological parameters. In this thesis work I focused specifically on ETGs and on their capability in constraining galaxy formation and evolution; in particular, the principal aims were to derive some of the ETGs evolutionary parameters, such as age, metallicity and star formation history (SFH) and to study their age-redshift and mass-age relations. In order to infer galaxy physical parameters, I used the public code STARLIGHT: this program provides a best fit to the observed spectrum from a combination of many theoretical models defined in user-made libraries. the comparison between the output and input light-weighted ages shows a good agreement starting from SNRs of ∼ 10, with a bias of ∼ 2.2% and a dispersion 3%. Furthermore, also metallicities and SFHs are well reproduced. In the second part of the thesis I performed an analysis on real data, starting from Sloan Digital Sky Survey (SDSS) spectra. I found that galaxies get older with cosmic time and with increasing mass (for a fixed redshift bin); absolute light-weighted ages, instead, result independent from the fitting parameters or the synthetic models used. Metallicities, instead, are very similar from each other and clearly consistent with the ones derived from the Lick indices. The predicted SFH indicates the presence of a double burst of star formation. Velocity dispersions and extinctiona are also well constrained, following the expected behaviours. As a further step, I also fitted single SDSS spectra (with SNR∼ 20), to verify that stacked spectra gave the same results without introducing any bias: this is an important check, if one wants to apply the method at higher z, where stacked spectra are necessary to increase the SNR. Our upcoming aim is to adopt this approach also on galaxy spectra obtained from higher redshift Surveys, such as BOSS (z ∼ 0.5), zCOSMOS (z 1), K20 (z ∼ 1), GMASS (z ∼ 1.5) and, eventually, Euclid (z 2). Indeed, I am currently carrying on a preliminary study to estabilish the applicability of the method to lower resolution, as well as higher redshift (z 2) spectra, just like the Euclid ones.

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Organic electronics is an emerging field with a vast number of applications having high potential for commercial success. Although an enormous progress has been made in this research area, many organic electronic applications such as organic opto-electronic devices, organic field effect transistors and organic bioelectronic devices still require further optimization to fulfill the requirements for successful commercialization. The main bottle neck that hinders large scale production of these devices is their performances and stability. The performance of the organic devices largely depends on the charge transport processes occurring at the interfaces of various material that it is composed of. As a result, the key ingredient needed for a successful improvement in the performance and stability of organic electronic devices is an in-depth knowledge of the interfacial interactions and the charge transport phenomena taking place at different interfaces. The aim of this thesis is to address the role of the various interfaces between different material in determining the charge transport properties of organic devices. In this framework, I chose an Organic Field Effect Transistor (OFET) as a model system to carry out this study as it An OFET offers various interfaces that can be investigated as it is made up of stacked layers of various material. In order to probe the intrinsic properties that governs the charge transport, we have to be able to carry out thorough investigation of the interactions taking place down at the accumulation layer thickness. However, since organic materials are highly instable in ambient conditions, it becomes quite impossible to investigate the intrinsic properties of the material without the influence of extrinsic factors like air, moisture and light. For this reason, I have employed a technique called the in situ real-time electrical characterization technique which enables electrical characterization of the OFET during the growth of the semiconductor.

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21 cm cosmology opens an observational window to previously unexplored cosmological epochs such as the Epoch of Reionization (EoR), the Cosmic Dawn and the Dark Ages using powerful radio interferometers such as the planned Square Kilometer Array (SKA). Among all the other applications which can potentially improve the understanding of standard cosmology, we study the promising opportunity given by measuring the weak gravitational lensing sourced by 21 cm radiation. We performed this study in two different cosmological epochs, at a typical EoR redshift and successively at a post-EoR redshift. We will show how the lensing signal can be reconstructed using a three dimensional optimal quadratic lensing estimator in Fourier space, using single frequency band or combining multiple frequency band measurements. To this purpose, we implemented a simulation pipeline capable of dealing with issues that can not be treated analytically. Considering the current SKA plans, we studied the performance of the quadratic estimator at typical EoR redshifts, for different survey strategies and comparing two thermal noise models for the SKA-Low array. The simulation we performed takes into account the beam of the telescope and the discreteness of visibility measurements. We found that an SKA-Low interferometer should obtain high-fidelity images of the underlying mass distribution in its phase 1 only if several bands are stacked together, covering a redshift range that goes from z=7 to z=11.5. The SKA-Low phase 2, modeled in order to improve the sensitivity of the instrument by almost an order of magnitude, should be capable of providing images with good quality even when the signal is detected within a single frequency band. Considering also the serious effect that foregrounds could have on this detections, we discussed the limits of these results and also the possibility provided by these models of measuring an accurate lensing power spectrum.

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Die vorliegende Dissertation behandelt die Anwendung Übergangsmetall-katalysierter Anellierungsreaktionen zur Synthese neuartiger Chromophore. Dabei konnten sowohl benzoide als auch nicht-benzoide Strukturen insbesondere durch den Einsatz ausgewählter Pd(0)-Komplexe dargestellt werden. Die Arbeit gliedert sich in fünf Teile: Zunächst werden innovative Pentanellierungsreaktionen mit Acetylenen an bromierten Polycyclischen Aromatischen Kohlenwasserstoffen (PAK) beschrieben, wodurch bislang unbekannte Cyclopenta-PAKs zugänglich werden. Die untersuchten neuen Verbindungen umfassen dabei sowohl einfach als auch doppelt pentanellierte Pyrene, Anthracene und Perylene mit variablem Substitutionsmuster. Auf diese Weise werden bathochrome Wellenlängenverschiebungen bis zu max = 780 nm erreicht. Im zweiten Teil wurde die Pentanellierungstechnik auf Perylenmonoimid-(PMI)-Derivate angewandt. Die resultierenden Arylcyclopenta-PMIs weisen in ihren optischen Eigenschaften starke Ähnlichkeiten zu den verwandten Perylendiimiden (PDI) auf, bieten jedoch die Möglichkeit zusätzlicher Funktionalisierungen. Die Vergrößerung des aromatischen Systems des PDI durch Hexanellierung dagegen wurde im darauffolgenden Kapitel untersucht. Analog zur bekannten homologen Reihe der Rylene (Perylen, Terrylen, Quaterrylen) konnten im Rahmen dieser Arbeit die verwandten 1,12:6,7-Coronendiimid-(CDI)-Derivate um das im Kern unsubstituierte CDI selbst und das 3,4:9,10-Dinaphtho-CDI vervollständigt werden. UV/Vis-Absorptionsmessungen zeigen auch hier eine stete bathochrome Verschiebung der Absorptionswellenlängen. Das Wissen um die Coronendiimid-Synthesen sollte im vierten Teil weiterführend zur Darstellung eines Tetraketo-CDIs genutzt werden. Die finalen Oxidationsversuche zur Einführung der Keto-Gruppen waren nicht erfolgreich, bieten jedoch Einblicke in die Reaktivität unterschiedlicher CDI-Derivate. Der letzte Teil illustriert die Anwendung der bereits zuvor beschriebenen Hexanellierungsreaktion auf Tetrabrom-Terrylendiimid (TDI) zur Darstellung eines Tetranaphtho-TDI. Letzteres bildet dabei drei Isomere aus, wobei zwei optische Aktivität zeigen. UV/Vis und Circulardichroismus-Messungen zeigen hierfür auch bei erhöhten Temperaturen bemerkenswert hohe Racemisierungsbarrieren.

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Pyrene derivatives as donors and acceptorsrnrnAlmost 200 years have passed since pyrene was first discovered, and to this day it garners unbroken interest by chemists around the world. One of the most fascinating areas of pyrene chemistry is its selective functionalization, since it is still currently a challenge to specifically functionalize different positions on the molecule.[1]rnIn this work, two new patterns of pyrene substitution have been developed. Under suitable conditions, a fourfold bromination of 4,5,9,10 tetramethoxypyrene is possible to yield eightfold functionalized pyrenes. Based on these molecules a novel series of 1,3,4,5,6,8,9,10-substituted pyrene derivatives was achieved. Synthetic approaches to a non-quinoidal, strong pyrene-4,5,9,10-tetraone based acceptor have been discussed. It emerged that the chosen synthetic approach is suitable for intermediate acceptors, yet it failed very electron deficient pyrene derivatives. Donors based on 4,5,9,10-tetramethoxypyrene (2,7- and 1,3,6,8-substitued) have been prepared and studied as CT complexes. In the SFB/TR 49 these complexes were analyzed in the solid state. For the first time charge transfer in a non-TTF CT-complex was studied by HAXPES and NEXAFS.rnBased on the works of ZÖPHEL et al.[2] it was possible to obtain an asymmetric 4,9,10 substituted pyrene derivative. This was used as a building block to prepare a non-planar acceptor molecule as well as electron-rich rylene-type molecules. rnFinally, two separate series of molecules intended as emitters for OLEDs were presented. Thermally activated delayed fluorescence (TADF) in OLEDs attracted significant academic interest as it is considered a promising approach to improve the efficiency of fluorescent OLEDs.[3] Our molecules were designed to have a deep blue emission spectrum and a minimal singlet triplet energy gap (∆ES1->T1) while retaining a high fluorescence quantum yield ϕPL. The initial OD series has a small ∆ES1->T1, yet had an insufficient ϕPL for the use in OLEDs. The Py series emitters, in contrast, combine both desired properties and were successfully implemented in efficient OLED devices.rn[1]. T. M. Figueira-Duarte and K. Müllen, Chem. Rev., 2011, 111, 7260-7314.rn[2]. L. Zöphel, V. Enkelmann and K. Müllen, Org. Lett., 2013, 15, 804-807.rn[3]. H. Uoyama, K. Goushi, K. Shizu, H. Nomura and C. Adachi, Nature, 2012, 492, 234-238.

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Il presente lavoro di tesi riguarda lo studio e l'impiego di architetture neurali profonde (nello specifico stacked denoising auto-encoder) per la definizione di un modello previsionale di serie temporali. Il modello implementato è stato applicato a dati industriali riguardanti un impianto fotovoltaico reale, per effettuare una predizione della produzione di energia elettrica sulla base della serie temporale che lo caratterizza. I risultati ottenuti hanno evidenziato come la struttura neurale profonda contribuisca a migliorare le prestazioni di previsione di strumenti statistici classici come la regressione lineare multipla.

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Autonomous system applications are typically limited by the power supply operational lifetime when battery replacement is difficult or costly. A trade-off between battery size and battery life is usually calculated to determine the device capability and lifespan. As a result, energy harvesting research has gained importance as society searches for alternative energy sources for power generation. For instance, energy harvesting has been a proven alternative for powering solar-based calculators and self-winding wristwatches. Thus, the use of energy harvesting technology can make it possible to assist or replace batteries for portable, wearable, or surgically-implantable autonomous systems. Applications such as cardiac pacemakers or electrical stimulation applications can benefit from this approach since the number of surgeries for battery replacement can be reduced or eliminated. Research on energy scavenging from body motion has been investigated to evaluate the feasibility of powering wearable or implantable systems. Energy from walking has been previously extracted using generators placed on shoes, backpacks, and knee braces while producing power levels ranging from milliwatts to watts. The research presented in this paper examines the available power from walking and running at several body locations. The ankle, knee, hip, chest, wrist, elbow, upper arm, side of the head, and back of the head were the chosen target localizations. Joints were preferred since they experience the most drastic acceleration changes. For this, a motor-driven treadmill test was performed on 11 healthy individuals at several walking (1-4 mph) and running (2-5 mph) speeds. The treadmill test provided the acceleration magnitudes from the listed body locations. Power can be estimated from the treadmill evaluation since it is proportional to the acceleration and frequency of occurrence. Available power output from walking was determined to be greater than 1mW/cm³ for most body locations while being over 10mW/cm³ at the foot and ankle locations. Available power from running was found to be almost 10 times higher than that from walking. Most energy harvester topologies use linear generator approaches that are well suited to fixed-frequency vibrations with sub-millimeter amplitude oscillations. In contrast, body motion is characterized with a wide frequency spectrum and larger amplitudes. A generator prototype based on self-winding wristwatches is deemed to be appropriate for harvesting body motion since it is not limited to operate at fixed-frequencies or restricted displacements. Electromagnetic generation is typically favored because of its slightly higher power output per unit volume. Then, a nonharmonic oscillating rotational energy scavenger prototype is proposed to harness body motion. The electromagnetic generator follows the approach from small wind turbine designs that overcome the lack of a gearbox by using a larger number of coil and magnets arrangements. The device presented here is composed of a rotor with multiple-pole permanent magnets having an eccentric weight and a stator composed of stacked planar coils. The rotor oscillations induce a voltage on the planar coil due to the eccentric mass unbalance produced by body motion. A meso-scale prototype device was then built and evaluated for energy generation. The meso-scale casing and rotor were constructed on PMMA with the help of a CNC mill machine. Commercially available discrete magnets were encased in a 25mm rotor. Commercial copper-coated polyimide film was employed to manufacture the planar coils using MEMS fabrication processes. Jewel bearings were used to finalize the arrangement. The prototypes were also tested at the listed body locations. A meso-scale generator with a 2-layer coil was capable to extract up to 234 µW of power at the ankle while walking at 3mph with a 2cm³ prototype for a power density of 117 µW/cm³. This dissertation presents the analysis of available power from walking and running at different speeds and the development of an unobtrusive miniature energy harvesting generator for body motion. Power generation indicates the possibility of powering devices by extracting energy from body motion.

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Cochlear implants have been of great benefit in restoring auditory function to individuals with profound bilateral sensorineural deafness. The implants are used to directly stimulate auditory nerves and send a signal to the brain that is then interpreted as sound. This project focuses on the development of a surgical positioning tool to accurately and effectively place an array of stimulating electrodes deep within the cochlea. This will lead to improved efficiency and performance of the stimulating electrodes, reduced surgical trauma to the cochlea, and as a result, improved overall performance to the implant recipient. The positioning tool reported here consists of multiple fluidic chambers providing localized curvature control along the length of the attached silicon electrode array. The chambers consist of 200μm inner diameter PET (polyethylene therephthalate) tubes with 4μm wall thickness. The chambers are molded in a tapered helical configuration to correspond to the cochlear shape upon relaxation of the actuators. This ensures that the optimal electrode placement within the cochlea is retained after the positioning tool becomes dormant (for chronic implants). Actuation is achieved by injecting fluid into the PET chambers and regulating the fluidic pressure. The chambers are arranged in a stacked, overlapping design to provide fluid connectivity with the non-implantable pressure controller and allow for local curvature control of the device. The stacked tube configuration allows for localized curvature control of various areas along the length of the electrode and additional stiffening and actuating power towards the base. Curvature is affected along the entire length of a chamber and the result is cumulative in sections of multiple chambers. The actuating chambers are bonded to the back of a silicon electrode array.

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Supercritical carbon dioxide is used to exfoliate graphite, producing a small, several-layer graphitic flake. The supercritical conditions of 2000, 2500, and 3000 psi and temperatures of 40°, 50°, and 60°C, have been used to study the effect of critical density on the sizes and zeta potentials of the treated flakes. Photon Correlation Spectroscopy (PCS), Brunauer-Emmett-Teller (BET) surface area measurement, field emission scanning electron microscopy (FE-SEM), and atomic force microscopy (AFM) are used to observe the features of the flakes. N-methyl-2-pyrrolidinone (NMP), dimethylformamide (DMF), and isopropanol are used as co-solvents to enhance the supercritical carbon dioxide treatment. As a result, the PCS results show that the flakes obtained from high critical density treatment (low temperature and high pressure) are more stable due to more negative charges of zeta potential, but have smaller sizes than those from low critical density (high temperature and low pressure). However, when an additional 1-hour sonication is applied, the size of the flakes from low critical density treatment becomes smaller than those from high critical density treatment. This is probably due to more CO2 molecules stacked between the layers of the graphitic flakes. The zeta potentials of the sonicated samples were slightly more negative than nonsonicated samples. NMP and DMF co-solvents maintain stability and prevented reaggregation of the flakes better than isopropanol. The flakes tend to be larger and more stable as the treatment time increases since larger flat area of graphite is exfoliated. In these experiments, the temperature has more impact on the flakes than pressure. The BET surface area resultsshow that CO2 penetrates the graphite layers more than N2. Moreover, the negative surface area of the treated graphite indicates that the CO2 molecules may be adsorbed between the graphite layers during supercritical treatment. The FE-SEM and AFM images show that the flakes have various shapes and sizes. The effects of surfactants can be observed on the FE-SEM images of the samples in one percent by weight solution of SDBS in water since the sodium dodecylbenzene sulfonate (SDBS) residue covers all of the remaining flakes. The AFM images show that the vertical thickness of the graphitic flakes can ranges from several nanometers (less than ten layers thick), to more than a hundred nanometers. In conclusion, supercritical carbon dioxide treatment is a promising step compared to mechanical and chemical exfoliation techniques in the large scale production of thin graphitic flake, breaking down the graphite flakes into flakes only a fewer graphene layers thick.

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One of the original ocean-bottom time-lapse seismic studies was performed at the Teal South oil field in the Gulf of Mexico during the late 1990’s. This work reexamines some aspects of previous work using modern analysis techniques to provide improved quantitative interpretations. Using three-dimensional volume visualization of legacy data and the two phases of post-production time-lapse data, I provide additional insight into the fluid migration pathways and the pressure communication between different reservoirs, separated by faults. This work supports a conclusion from previous studies that production from one reservoir caused regional pressure decline that in turn resulted in liberation of gas from multiple surrounding unproduced reservoirs. I also provide an explanation for unusual time-lapse changes in amplitude-versus-offset (AVO) data related to the compaction of the producing reservoir which, in turn, changed an isotropic medium to an anisotropic medium. In the first part of this work, I examine regional changes in seismic response due to the production of oil and gas from one reservoir. The previous studies primarily used two post-production ocean-bottom surveys (Phase I and Phase II), and not the legacy streamer data, due to the unavailability of legacy prestack data and very different acquisition parameters. In order to incorporate the legacy data in the present study, all three poststack data sets were cross-equalized and examined using instantaneous amplitude and energy volumes. This approach appears quite effective and helps to suppress changes unrelated to production while emphasizing those large-amplitude changes that are related to production in this noisy (by current standards) suite of data. I examine the multiple data sets first by using the instantaneous amplitude and energy attributes, and then also examine specific apparent time-lapse changes through direct comparisons of seismic traces. In so doing, I identify time-delays that, when corrected for, indicate water encroachment at the base of the producing reservoir. I also identify specific sites of leakage from various unproduced reservoirs, the result of regional pressure blowdown as explained in previous studies; those earlier studies, however, were unable to identify direct evidence of fluid movement. Of particular interest is the identification of one site where oil apparently leaked from one reservoir into a “new” reservoir that did not originally contain oil, but was ideally suited as a trap for fluids leaking from the neighboring spill-point. With continued pressure drop, oil in the new reservoir increased as more oil entered into the reservoir and expanded, liberating gas from solution. Because of the limited volume available for oil and gas in that temporary trap, oil and gas also escaped from it into the surrounding formation. I also note that some of the reservoirs demonstrate time-lapse changes only in the “gas cap” and not in the oil zone, even though gas must be coming out of solution everywhere in the reservoir. This is explained by interplay between pore-fluid modulus reduction by gas saturation decrease and dry-frame modulus increase by frame stiffening. In the second part of this work, I examine various rock-physics models in an attempt to quantitatively account for frame-stiffening that results from reduced pore-fluid pressure in the producing reservoir, searching for a model that would predict the unusual AVO features observed in the time-lapse prestack and stacked data at Teal South. While several rock-physics models are successful at predicting the time-lapse response for initial production, most fail to match the observations for continued production between Phase I and Phase II. Because the reservoir was initially overpressured and unconsolidated, reservoir compaction was likely significant, and is probably accomplished largely by uniaxial strain in the vertical direction; this implies that an anisotropic model may be required. Using Walton’s model for anisotropic unconsolidated sand, I successfully model the time-lapse changes for all phases of production. This observation may be of interest for application to other unconsolidated overpressured reservoirs under production.

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Reflection seismic data from the F3 block in the Dutch North Sea exhibits many large-amplitude reflections at shallow horizons, typically categorized as “brightspots ” (Schroot and Schuttenhelm, 2003), mainly because of their bright appearance. In most cases, these bright reflections show a significant “flatness” contrasting with local structural trends. While flatspots are often easily identified in thick reservoirs, we have often occasionally observed apparent flatspot tuning effects at fluid contacts near reservoir edges and in thin reservoir beds, while only poorly understanding them. We conclude that many of the shallow large-amplitude reflections in block F3 are dominated by flatspots, and we investigate the thin-bed tuning effects that such flatspots cause as they interact with the reflection from the reservoir’s upper boundary. There are two possible effects to be considered: (1) the “wedge-model” tuning effects of the flatspot and overlying brightspots, dimspots, or polarity-reversals; and (2) the stacking effects that result from possible inclusion of post-critical flatspot reflections in these shallow sands. We modeled the effects of these two phenomena for the particular stratigraphic sequence in block F3. Our results suggest that stacking of post-critical flatspot reflections can cause similar large-amplitude but flat reflections, in some cases even causing an interface expected to produce a ‘dimspot’ to appear as a ‘brightspot’. Analysis of NMO stretch and muting shows the likely exclusion of critical offset data in stacked output. If post-critical reflections are included in stacking, unusual results will be observed. In the North Sea case, we conclude the tuning effect was the primary reason causing for the brightness and flatness of these reflections. However, it is still important to note that care should be taken while applying muting on reflections with wide range of incidence angles and the inclusion of critical offset data may cause some spurious features in the stacked section.

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We used the Green's functions from auto-correlations and cross-correlations of seismic ambient noise to monitor temporal velocity changes in the subsurface at Villarrica volcano in the Southern Andes of Chile. Campaigns were conducted from March to October 2010 and February to April 2011 with 8 broadband and 6 short-period stations, respectively. We prepared the data by removing the instrument response, normalizing with a root-mean-square method, whitening the spectra, and filtering from 1 to 10 Hz. This frequency band was chosen based on the relatively high background noise level in that range. Hour-long auto- and cross-correlations were computed and the Green's functions stacked by day and total time. To track the temporal velocity changes we stretched a 24 hour moving window of correlation functions from 90% to 110% of the original and cross correlated them with the total stack. All of the stations' auto-correlations detected what is interpreted as an increase in velocity in 2010, with an average increase of 0.13%. Cross-correlations from station V01, near the summit, to the other stations show comparable changes that are also interpreted as increases in velocity. We attribute this change to the closing of cracks in the subsurface due either to seasonal snow loading or regional tectonics. In addition to the common increase in velocity across the stations, there are excursions in velocity on the same order lasting several days. Amplitude decreases as the station's distance from the vent increases suggesting these excursions may be attributed to changes within the volcanic edifice. In at least two occurrences the amplitudes at stations V06 and V07, the stations farthest from the vent, are smaller. Similar short temporal excursions were seen in the auto-correlations from 2011, however, there was little to no increase in the overall velocity.

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The Bloom protein (BLM) and Topoisomerase IIIalpha are found in association with proteins of the Fanconi anemia (FA) pathway, a disorder manifesting increased cellular sensitivity to DNA crosslinking agents. In order to determine if the association reflects a functional interaction for the maintenance of genome stability, we have analyzed the effects of siRNA-mediated depletion of the proteins in human cells. Depletion of Topoisomerase IIIalpha or BLM leads to increased radial formation, as is seen in FA. BLM and Topoisomerase IIIalpha are epistatic to the FA pathway for suppression of radial formation in response to DNA interstrand crosslinks since depletion of either of them in FA cells does not increase radial formation. Depletion of Topoisomerase IIIalpha or BLM also causes an increase in sister chromatid exchanges, as is seen in Bloom syndrome cells. Human Fanconi anemia cells, however, do not demonstrate increased sister chromatid exchanges, separating this response from radial formation. Primary cell lines from mice defective in both Blm and Fancd2 have the same interstrand crosslink-induced genome instability as cells from mice deficient in the Fancd2 protein alone. These observations demonstrate that the association of BLM and Topoisomerase IIIalpha with Fanconi proteins is a functional one, delineating a BLM-Topoisomerase IIIalpha-Fanconi pathway that is critical for suppression of chromosome radial formation.