Sudden Cardiac Death in Brazil: Study Based on Physicians' Perceptions of the Public Health Care System

Background: There are no available statistical data about sudden cardiac death in Brazil. Therefore, this study has been conducted to evaluate the incidence of sudden cardiac death in our population and its implications. Methods: The research methodology was based on Thurstone's Law of Comparative Judgment, whose premise is that the more an A stimulus differs from a B stimulus, the greater will be the number of people who will perceive this difference. This technique allows an estimation of actual occurrences from subjective perceptions, when compared to official statistics. Data were collected through telephone interviews conducted with Primary and Secondary Care physicians of the Public Health Service in the Metropolitan Area of Sao Paulo (MASP). Results: In the period from October 19, 2009, to October 28, 2009, 196 interviews were conducted. The incidence of 21,270 cases of sudden cardiac death per year was estimated by linear regression analysis of the physicians responses and data from the Mortality Information System of the Brazilian Ministry of Health, with the following correlation and determination coefficients: r = 0.98 and r2= 0.95 (95% confidence interval 0.81.0, P < 0.05). The lack of waiting list for specialized care and socioadministrative problems were considered the main barriers to tertiary care access. Conclusions: The incidence of sudden cardiac death in the MASP is high, and it was estimated as being higher than all other causes of deaths; the extrapolation technique based on the physicians perceptions was validated; and the most important bureaucratic barriers to patient referral to tertiary care have been identified. (PACE 2012; 35:13261331)

Energy and system-size dependence of two- and four-particle nu(2) measurements in heavy-ion collisions at root S-NN=62.4 and 200 GeV and their implications on flow fluctuations and nonflow

We present STAR measurements of azimuthal anisotropy by means of the two- and four-particle cumulants nu(2) (nu(2){2} and nu(2){4}) for Au + Au and Cu + Cu collisions at center-of-mass energies root S-NN = 62.4 and 200 GeV. The difference between nu(2){2}(2) and nu(2){4}(2) is related to nu(2) fluctuations (sigma(nu 2)) and nonflow (delta(2)). We present an upper limit to sigma(nu 2)/nu 2. Following the assumption that eccentricity fluctuations sigma(epsilon) dominate nu(2) fluctuations nu(2)/sigma nu(2) approximate to epsilon/sigma epsilon we deduce the nonflow implied for several models of eccentricity fluctuations that would be required for consistency with nu(2){2} and nu(2){4}. We also present results on the ratio of nu(2) to eccentricity.

The Pst system of Streptococcus mutans is important for phosphate transport and adhesion to abiotic surfaces

The Pst system is a high-affinity inorganic phosphate transporter found in many bacterial species. Streptococcus mutans, the etiological agent of tooth decay, carries a single copy of the pst operon composed of six cistrons (pstS, pstC1, pstC, pstB, smu.1134 and phoU). Here, we show that deletion of pstS, encoding the phosphate-binding protein, reduces phosphate uptake and impairs cell growth, which can be restored upon enrichment of the medium with high concentrations of inorganic phosphate. The relevance of Pst for growth was also demonstrated in the wild-type strain treated with an anti-PstS antibody. Nevertheless, a reduced ability to bind to saliva-coated surfaces was observed, along with the reduction of extracellular polysaccharide production, although no difference on pH acidification was observed between mutant and wild-type strains. Taken together, the present data indicate that the S.similar to mutans Pst system participates in phosphate uptake, cell growth and expression of virulence-associated traits.

Successful Strategy for Targeting the Central Nervous System Using Magnetic Albumin Nanospheres

This study reports on the successful use of magnetic albumin nanosphere (MAN), consisting of maghemite nanoparticles hosted by albumin-based nanosphere, to target different sites within the central nervous system (CNS). Ultrastructural analysis by transmission electron microscopy (TEM) of the material collected from the mice was performed in the time window of 30 minutes up to 30 days after administration. Evidence found that the administered MAN was initially internalized and transported by erythrocytes across the blood-brain-barrier and transferred to glial cells and neuropils before internalization by neurons, mainly in the cerebellum. We hypothesize that the efficiency of MAN in crossing the BBB with no pathological alterations is due to the synergistic effect of its two main components, the iron-based nanosized particles and the hosting albumin-based nanospheres. We found that the MAN in targeting the CNS represents an important step towards the design of nanosized materials for clinical and diagnostic applications.

Transparent UV-absorbers thin films of zinc oxide: Ceria system synthesized via sol-gel process

Transparent nanostructure ZnO:CeO2 and ZnO thin films to use as solar protector were prepared by non-alkoxide sol-gel process and deposited on boronsilicate glass substrate by dip-coating technique and then heated at 300-500 degrees C. The films were characterized structurally, morphologically and optically by X-ray diffraction (XRD), atomic force microscopy (AFM), field emission gun-scanning electron microscopy (FEG-SEM), scanning electron microscopy (SEM) and UV-Vis transmittance spectroscopy. The coatings presented high transparency in the visible region and excellent absorption in the UV. The band gap of the deposited films was estimated between 3.10 and 3.18 eV. Absorption of the films in the UV was increased by presence of cerium. The results suggest that the materials are promising candidates to use as coating solar protective. (C) 2012 Elsevier B.V. All rights reserved.

Leptin as a link between the immune system and kidney-related diseases: leading actor or just a coadjuvant?

Food intake and nutritional status modify the physiological responses of the immune system to illness and infection and regulate the development of chronic inflammatory processes, such as kidney disease. Adipose tissue secretes immune-related proteins called adipokines that have pleiotropic effects on both the immune and neuroendocrine systems, linking metabolism and immune physiology. Leptin, an adipose tissue-derived adipokine, displays a variety of immune and physiological functions, and participates in several immune responses. Here, we review the current literature on the role of leptin in kidney diseases, linking adipose tissue and the immune system with kidney-related disorders. The modulation of this adipose hormone may have a major impact on the treatment of several immune- and metabolic-related kidney diseases.

Selection of compositions with high glass forming ability in the Ni-Nb-B alloy system

A combination of an extension of the topological instability "λ criterion" and the "average electronegativity" has been recently reported in the literature to predict compositions with high glass-forming ability (GFA). In the present work, both criteria have been applied to select the Ni61.0Nb36.0B3 alloy with a high glass-forming ability. Ingots were prepared by arc-melting and were used to produce ribbons processed by the melt-spinning technique further characterized by differential scanning calorimetry (DSC), X-ray diffraction (XRD) and scanning electron microscopy (SEM). The Ni61.0Nb36.0B3 alloy revealed a complete amorphization and supercooled liquid region ΔTx = 68 K. In addition, wedge-shaped samples were prepared using copper mold casting in order to determine the critical thickness for amorphous formation. Scanning electron microscopy (SEM) revealed that fully amorphous samples could be obtained, reaching up to ~800 µm in thickness.

Factor Xa activation of factor V is of paramount importance in initiating the coagulation system: lessons from a tick salivary protein

BACKGROUND: Generation of active procoagulant cofactor factor Va (FVa) and its subsequent association with the enzyme activated factor X (FXa) to form the prothrombinase complex is a pivotal initial event in blood coagulation and has been the subject of investigative effort, speculation, and controversy. The current paradigm assumes that FV activation is initiated by limited proteolysis by traces of (meizo) thrombin. METHODS AND RESULTS: Recombinant tick salivary protein TIX-5 was produced and anticoagulant properties were studied with the use of plasma, whole blood, and purified systems. Here, we report that TIX-5 specifically inhibits FXa-mediated FV activation involving the B domain of FV and show that FXa activation of FV is pivotal for plasma and blood clotting. Accordingly, tick feeding is impaired on TIX-5 immune rabbits, displaying the in vivo importance of TIX-5. CONCLUSIONS: Our data elucidate a unique molecular mechanism by which ticks inhibit the host's coagulation system. From our data, we propose a revised blood coagulation scheme in which direct FXa-mediated FV activation occurs in the initiation phase during which thrombin-mediated FV activation is restrained by fibrinogen and inhibitors.

Effect of culture system and diet in early larval stages over skeletal deformities development in gilthead sea bream

[ES] Main deformities such as lordosis, opercular deformities and upper/lower jaws shortening are considered as quality descriptors in commercial marine fish fry production and seem to be related with larval culture conditions in early larval stages. The aim of this work was to obtain information about the contribution of the diet and rearing system to the apparition of these abnormalities in gilthead sea bream (Sparus aurata) larvae in semi-industrial scale facilities. For that purpose, two different larval rearing systems semi-intensive and intensive were compared; besides, two different rotifer enrichments, DHA Protein Selco, (Inve Aquaculture, Dendermonde, Belgium) (R1) and Red Pepper Paste, (Bernaqua bvba, Turnhout, Belgium) were tested in the intensive system. Biochemical composition of larvae, preys and commercial products was analysed. At 50 days post hatching six hundred fish per treatment were individually studied under stereoscope and deformity frequency recorded. Besides at 95 days post hatching fry were soft X ray monitored. Both rotifer enrichment and rearing system affected survival, growth and deformity frequency. Rearing system did not affect total larvae fatty acid content except at 20 dah, where DHA were significantly higher and EPA significantly lower in Semi-intensive system. A significantly lower percentage of deformity rates together with better survival and growth were obtained in the semi-intensive system. In dietary treatment, rotifer enrichment significantly affected larval survival. R1 rotifers enrichment significantly (P<0.05) improved survival when compared to fed R2 larvae. The content of DPA was significantly (P<0.05) higher in R2 fed larvae reflecting the R2 rotifers content of this fatty acid. The level of this FA tended to decrease in concordance with the rotifers replacement by artemia in the diet. The effects n-3-HUFA and DPA (22:5n-6) over larval survival and skeletal deformities development is discussed.

Sincronizzazione e condivisione di file system tra sistemi operativi

La necessità di sincronizzare i propri dati si presenta in una moltitudine di situazioni, infatti il numero di dispositivi informatici a nostra disposizione è in continua crescita e, all' aumentare del loro numero, cresce l' esigenza di mantenere aggiornate le multiple copie dei dati in essi memorizzati. Vi sono diversi fattori che complicano tale situazione, tra questi la varietà sempre maggiore dei sistemi operativi utilizzati nei diversi dispositivi, si parla di Microsoft Windows, delle tante distribuzioni Linux, di Mac OS X, di Solaris o di altri sistemi operativi UNIX, senza contare i sistemi operativi più orientati al settore mobile come Android. Ogni sistema operativo ha inoltre un modo particolare di gestire i dati, si pensi alla differente gestione dei permessi dei file o alla sensibilità alle maiuscole. Bisogna anche considerare che se gli aggiornamenti dei dati avvenissero soltanto su di uno di questi dispositivi sarebbe richiesta una semplice copia dei dati aggiornati sugli altri dispositivi, ma che non è sempre possibile utilizzare tale approccio. Infatti i dati vengono spesso aggiornati in maniera indipendente in più di un dispositivo, magari nello stesso momento, è pertanto necessario che le applicazioni che si occupano di sincronizzare tali dati riconoscano le situazioni di conflitto, nelle quali gli stessi dati sono stati aggiornati in più di una copia ed in maniera differente, e permettano di risolverle, uniformando lo stato delle repliche. Considerando l' importanza e il valore che possono avere i dati, sia a livello lavorativo che personale, è necessario che tali applicazioni possano garantirne la sicurezza, evitando in ogni caso un loro danneggiamento, perchè sempre più spesso il valore di un dispositivo dipende più dai dati in esso contenuti che dal costo dello hardware. In questa tesi verranno illustrate alcune idee alternative su come possa aver luogo la condivisione e la sincronizzazione di dati tra sistemi operativi diversi, sia nel caso in cui siano installati nello stesso dispositivo che tra dispositivi differenti. La prima parte della tesi descriverà nel dettaglio l' applicativo Unison. Tale applicazione, consente di mantenere sincronizzate tra di loro repliche dei dati, memorizzate in diversi dispositivi che possono anche eseguire sistemi operativi differenti. Unison funziona a livello utente, analizzando separatamente lo stato delle repliche al momento dell' esecuzione, senza cioè mantenere traccia delle operazioni che sono state effettuate sui dati per modificarli dal loro stato precedente a quello attuale. Unison permette la sincronizzazione anche quando i dati siano stati modificati in maniera indipendente su più di un dispositivo, occupandosi di risolvere gli eventuali conflitti che possono verificarsi rispettando la volontà dell' utente. Verranno messe in evidenza le strategie utilizzate dai suoi ideatori per garantire la sicurezza dei dati ad esso affidati e come queste abbiano effetto nelle più diverse condizioni. Verrà poi fornita un' analisi dettagiata di come possa essere utilizzata l' applicazione, fornendo una descrizione accurata delle funzionalità e vari esempi per renderne più chiaro il funzionamento. Nella seconda parte della tesi si descriverà invece come condividere file system tra sistemi operativi diversi all' interno della stessa macchina, si tratta di un approccio diametralmente opposto al precedente, in cui al posto di avere una singola copia dei dati, si manteneva una replica per ogni dispositivo coinvolto. Concentrando l' attenzione sui sistemi operativi Linux e Microsoft Windows verranno descritti approfonditamente gli strumenti utilizzati e illustrate le caratteristiche tecniche sottostanti.

X-Ray studies of the physics of matter around super-massive black-holes in nearby Seyfert galaxies

Seyfert galaxies are the closest active galactic nuclei. As such, we can use them to test the physical properties of the entire class of objects. To investigate their general properties, I took advantage of different methods of data analysis. In particular I used three different samples of objects, that, despite frequent overlaps, have been chosen to best tackle different topics: the heterogeneous BeppoS AX sample was thought to be optimized to test the average hard X-ray (E above 10 keV) properties of nearby Seyfert galaxies; the X-CfA was thought the be optimized to compare the properties of low-luminosity sources to the ones of higher luminosity and, thus, it was also used to test the emission mechanism models; finally, the XMM–Newton sample was extracted from the X-CfA sample so as to ensure a truly unbiased and well defined sample of objects to define the average properties of Seyfert galaxies. Taking advantage of the broad-band coverage of the BeppoS AX MECS and PDS instruments (between ~2-100 keV), I infer the average X-ray spectral propertiesof nearby Seyfert galaxies and in particular the photon index (~1.8), the high-energy cut-off (~290 keV), and the relative amount of cold reflection (~1.0). Moreover the unified scheme for active galactic nuclei was positively tested. The distribution of isotropic indicators used here (photon index, relative amount of reflection, high-energy cut-off and narrow FeK energy centroid) are similar in type I and type II objects while the absorbing column and the iron line equivalent width significantly differ between the two classes of sources with type II objects displaying larger absorbing columns. Taking advantage of the XMM–Newton and X–CfA samples I also deduced from measurements that 30 to 50% of type II Seyfert galaxies are Compton thick. Confirming previous results, the narrow FeK line is consistent, in Seyfert 2 galaxies, with being produced in the same matter responsible for the observed obscuration. These results support the basic picture of the unified model. Moreover, the presence of a X-ray Baldwin effect in type I sources has been measured using for the first time the 20-100 keV luminosity (EW proportional to L(20-100)^(−0.22±0.05)). This finding suggests that the torus covering factor may be a function of source luminosity, thereby suggesting a refinement of the baseline version of the unifed model itself. Using the BeppoSAX sample, it has been also recorded a possible correlation between the photon index and the amount of cold reflection in both type I and II sources. At a first glance this confirms the thermal Comptonization as the most likely origin of the high energy emission for the active galactic nuclei. This relation, in fact, naturally emerges supposing that the accretion disk penetrates, depending to the accretion rate, the central corona at different depths (Merloni et al. 2006): the higher accreting systems hosting disks down to the last stable orbit while the lower accreting systems hosting truncated disks. On the contrary, the study of the well defined X–C f A sample of Seyfert galaxies has proved that the intrinsic X-ray luminosity of nearby Seyfert galaxies can span values between 10^(38−43) erg s^−1, i.e. covering a huge range of accretion rates. The less efficient systems have been supposed to host ADAF systems without accretion disk. However, the study of the X–CfA sample has also proved the existence of correlations between optical emission lines and X-ray luminosity in the entire range of L_(X) covered by the sample. These relations are similar to the ones obtained if high-L objects are considered. Thus the emission mechanism must be similar in luminous and weak systems. A possible scenario to reconcile these somehow opposite indications is assuming that the ADAF and the two phase mechanism co-exist with different relative importance moving from low-to-high accretion systems (as suggested by the Gamma vs. R relation). The present data require that no abrupt transition between the two regimes is present. As mentioned above, the possible presence of an accretion disk has been tested using samples of nearby Seyfert galaxies. Here, to deeply investigate the flow patterns close to super-massive black-holes, three case study objects for which enough counts statistics is available have been analysed using deep X-ray observations taken with XMM–Newton. The obtained results have shown that the accretion flow can significantly differ between the objects when it is analyzed with the appropriate detail. For instance the accretion disk is well established down to the last stable orbit in a Kerr system for IRAS 13197-1627 where strong light bending effect have been measured. The accretion disk seems to be formed spiraling in the inner ~10-30 gravitational radii in NGC 3783 where time dependent and recursive modulation have been measured both in the continuum emission and in the broad emission line component. Finally, the accretion disk seems to be only weakly detectable in rk 509, with its weak broad emission line component. Finally, blueshifted resonant absorption lines have been detected in all three objects. This seems to demonstrate that, around super-massive black-holes, there is matter which is not confined in the accretion disk and moves along the line of sight with velocities as large as v~0.01-0.4c (whre c is the speed of light). Wether this matter forms winds or blobs is still matter of debate together with the assessment of the real statistical significance of the measured absorption lines. Nonetheless, if confirmed, these phenomena are of outstanding interest because they offer new potential probes for the dynamics of the innermost regions of accretion flows, to tackle the formation of ejecta/jets and to place constraints on the rate of kinetic energy injected by AGNs into the ISM and IGM. Future high energy missions (such as the planned Simbol-X and IXO) will likely allow an exciting step forward in our understanding of the flow dynamics around black holes and the formation of the highest velocity outflows.

Background minimization issues for next generation hard X-ray focusing telescopes

The hard X-ray band (10 - 100 keV) has been only observed so far by collimated and coded aperture mask instruments, with a sensitivity and an angular resolution lower than two orders of magnitude as respects the current X-ray focusing telescopes operating below 10 - 15 keV. The technological advance in X-ray mirrors and detection systems is now able to extend the X-ray focusing technique to the hard X-ray domain, filling the gap in terms of observational performances and providing a totally new deep view on some of the most energetic phenomena of the Universe. In order to reach a sensitivity of 1 muCrab in the 10 - 40 keV energy range, a great care in the background minimization is required, a common issue for all the hard X-ray focusing telescopes. In the present PhD thesis, a comprehensive analysis of the space radiation environment, the payload design and the resulting prompt X-ray background level is presented, with the aim of driving the feasibility study of the shielding system and assessing the scientific requirements of the future hard X-ray missions. A Geant4 based multi-mission background simulator, BoGEMMS, is developed to be applied to any high energy mission for which the shielding and instruments performances are required. It allows to interactively create a virtual model of the telescope and expose it to the space radiation environment, tracking the particles along their path and filtering the simulated background counts as a real observation in space. Its flexibility is exploited to evaluate the background spectra of the Simbol-X and NHXM mission, as well as the soft proton scattering by the X-ray optics and the selection of the best shielding configuration. Altough the Simbol-X and NHXM missions are the case studies of the background analysis, the obtained results can be generalized to any future hard X-ray telescope. For this reason, a simplified, ideal payload model is also used to select the major sources of background in LEO. All the results are original contributions to the assessment studies of the cited missions, as part of the background groups activities.

Grazing incidence pumped Zr x-ray laser for spectroscopy on Li-like ions

X-ray laser fluorescence spectroscopy of the 2s-2p transition in Li-like ions is promising to become a widely applicable tool to provide information on the nuclear charge radii of stable and radioactive isotopes. For performing such experiments at the Experimental Storage Ring ESR, and the future NESR within the FAIR Project, a grazing incidence pumped (GRIP) x-ray laser (XRL) was set up at GSI Darmstadt using PHELIX (Petawatt High Energy Laser for heavy Ions eXperiments). The experiments demonstrated that lasing using the GRIP geometry could be achieved with relatively low pump energy, a prerequisite for higher repetition rate. In the first chapter the need of a plasma XRL is motivated and a short history of the plasma XRL is presented. The distinctive characteristic of the GRIP method is the controlled deposition of the pump laser energy into the desired plasma density region. While up to now the analysis performed were mostly concerned with the plasma density at the turning point of the main pump pulse, in this thesis it is demonstrated that also the energy deposition is significantly modified for the GRIP method, being sensitive in different ways to a large number of parameters. In the second chapter, the theoretical description of the plasma evolution, active medium and XRL emission properties are reviewed. In addition an innovative analysis of the laser absorption in plasma which includes an inverse Bremsstrahlung (IB) correction factor is presented. The third chapter gives an overview of the experimental set-up and diagnostics, providing an analytical formula for the average and instantaneous traveling wave speed generated with a tilted, on-axis spherical mirror, the only focusing system used up to now in GRIP XRL. The fourth chapter describes the experimental optimization and results. The emphasis is on the effect of the incidence angle of the main pump pulse on the absorption in plasma and on output and gain in different lasing lines. This is compared to the theoretical results for two different incidence angles. Significant corrections for the temperature evolution during the main pump pulse due to the incidence angle are demonstrated in comparison to a simple analytical model which does not take into account the pumping geometry. A much better agreement is reached by the model developed in this thesis. An interesting result is also the appearance of a central dip in the spatially resolved keV emission which was observed in the XRL experiments for the first time and correlates well with previous near field imaging and plasma density profile measurements. In the conclusion also an outlook to the generation of shorter wavelength XRL’s is given.

Oxidierte Kohlenwasserstoffe in der oberen Troposphäre: Kinetische Untersuchungen zum Abbau und Einfluss auf HO x und Ozon-Chemie

Der erste Teil dieser Arbeit befasst sich mit der Kinetik der Reaktion des OH-Radikals mit Glykolaldehyd (HOCH2CHO). Die Geschwindigkeitskonstante k1 wurde für diese Reaktion temperaturabhängig bestimmt. Durch gepulste Photolyse wurden OH-Radikale erzeugt. Anschließend wurde die laserinduzierte Fluoreszenz der OH-Radikale bei 309 nm detektiert. Die ermittelte Geschwindigkeitskonstante k1 für die Reaktion von OH mit HOCH2CHO von (8,0 ± 0,8) x 10-12 cm3 Teilchen-1 s-1 erweist sich für den Temperaturbereich von 240 K < T < 362 K als temperaturunabhängig. Zwischen 60 und 250 Torr kann zudem keine Druckabhängigkeit für k1 beobachtet werden. Die unerwartet niedrigere Geschwindigkeitskonstante für die betrachtete Reaktion im Vergleich zur Reaktion von OH mit CH3CHO konnte anhand von Überlegungen zur Korrelation zwischen der C-H-Bindungsstärke und dem H-Abstraktionskanal erklärt werden. Im zweiten Teil dieser Arbeit wurde die Photochemie von Aceton (CH3C(O)CH3), Methylethylketon (C2H5C(O)CH3, MEK) und Acetylbromid (CH3C(O)Br) betrachtet. Für die Photolyse von Aceton (bei 248 nm und 266 nm), MEK (bei 248 nm) und Acetylbromid (bei 248 nm) wurden bei 298 ± 3 K druckabhängig zwischen 5 und 1600 Torr N2 Quantenausbeuten für die Methylbildung (Phi(CH3)) bestimmt. Nach gepulster Photolyse der betrachteten Moleküle wurden die transienten Absorptionssignale der Methylradikale bei 216,4 nm verfolgt. Die Quantenausbeuten wurden relativ zur Photolyse von Methyliodid (CH3I) unter gleichen Reaktionsbedingungen ermittelt. Die erhaltenen Quantenausbeuten für CH3-Radikale nehmen für die beiden Systeme Aceton / 248 nm (Phi(CH3, Aceton) = 1,42 – 0,99) und MEK / 248 nm (Phi(CH3, MEK) = 0,45 – 0,19) druckabhängig zu hohen Drücken ab. Die Druckabhängigkeit von Phi(CH3) wird auf die Konkurrenz zwischen Stoßrelaxation und Dissoziation der schwingungsangeregten Acetylradikale (CH3CO#) zurückgeführt. Für das System Aceton / 266 nm wird keine Druckabhängigkeit von Phi(CH3) = 0,93 ± 0,1 beobachtet. Dies wird damit erklärt, dass CH3CO# nicht genügend Energie besitzt, um die Barriere zur Dissoziation zu überschreiten. Bei der Photolyse von Acetylbromid bei 248 nm wird druckunabhängig Phi(CH3) = 0,92 ± 0,10 bestimmt. In diesem System dissoziieren die schwingungsangeregten Acetylradikale bei allen Drücken vollständig. Bei 266 nm wurde die Gesamtquantenausbeute für die Photodissoziation von Aceton (Phi(diss, 266nm)) bestimmt. Die nach Photolyse erhaltenen Methyl - und Acetylradikale wurden nach Titration mit Br2 durch die Resonanzfluoreszenz der Bromatome detektiert. Phi(diss, 266nm) wurde mit 0,92 ± 0,07 bestimmt.

Synthetische Glycopeptide mit Sulfatyl-Lewis X-Struktur als potenzielle Inhibitoren der Zelladhäsion

Zelladhäsionsprozesse sind von großer Bedeutung für zahlreiche biologische Prozesse, wie etwa die Immunantwort, die Wundheilung und die Embryogenese. Außerdem spielen sie eine entscheidende Rolle im Verlauf inflammatorischer Prozesse. An der Zelladhäsion sind verschiedene Klassen von Adhäsionsmolekülen beteiligt. Die erste leichte „rollende“ Adhäsion von Leukozyten am Ort einer Entzündung wird durch die Selektine vermittelt. Diese binden über die Kohlenhydrat-Strukturen Sialyl-Lewisx und Sialyl-Lewisa über eine calciumabhängige Kohlenhydrat-Protein-Bindung an ihre spezifischen Liganden und vermitteln so den ersten Zellkontakt, bevor andere Adhäsionsmoleküle (Cadherine, Integrine) die feste Adhäsion und den Durchtritt durch das Endothel bewirken. Bei einer pathogenen Überexpression der Selektine kommt es jedoch zu zahlreichen chronischen Erkrankungen wie z. B. rheumatoider Arthritis, Erkrankungen der Herzkranzgefäße oder dem Reperfusions-syndrom. Außerdem wird eine Beteiligung der durch die Selektine vermittelten Zellkontakte bei der Metastasierung von Karzinomzellen angenommen. Ein Ansatzpunkt für die Behandlung der oben genannten Erkrankungen ist die Gabe löslicher kompetitiver Inhibitoren für die Selektine. Ziel der Arbeit war die Modifikation des Sialyl-Lewisx-Leitmotivs zur Steigerung der metabolischen Stabilität und dessen Einbau in die Peptidsequenz aus der für die Bindung verantwortlichen Domäne des endogenen Selektin-Liganden PSGL-1. Dazu wurden mit einer modifizierten Lewisx-Struktur glycosylierte Aminosäurebausteine dargestellt (Abb.1). Die Verwendung von Arabinose und des Sulfatrestes anstelle von Fusose und Sialinsäure sollte außerdem zu einer gesteigerten metabolischen Stabilität des synthetischen Liganden beitragen. Die so erhaltenen Glycosylaminosäuren sollten nun in die Festphasenpeptidsynthese eingesetzt werden. Aufgrund der großen säurelabilität konnte hier nicht auf das Standartverfahren (Wang-Harz, Abspaltung mit TFA) zurückgegriffen werden. Deshalb kam ein neuartiges UV-labiles Ankersystem zum Einsatz. Dazu wurde ein Protokoll für die Synthese und Abspaltung von Peptiden an diesem neuen System entwickelt. Daran gelang die Synthese des nichtglycosylierten Peptidrückgrats sowie eines mit der dem sulfatierten Lewisx-Motiv versehenen Glycopeptids. Ein vierfach sulfatiertes Glycopeptid, welches durch den Einsatz von im Vorfeld chemisch sulfatierer Tyrosin-Bausteinen dargestellt werden sollte, konnte massenspektrometrisch nachgewiesen werden.