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- 저자 : Presotto, Anna Gabriella Camacho (검색결과 2 건)
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Biomechanical behavior of CAD/CAM cobalt-chromium and zirconia full-arch fixed prostheses
Barbin, Thais,Silva, Leticia Del Rio,Veloso, Daniele Valente,Borges, Guilherme Almeida,Presotto, Anna Gabriella Camacho,Barao, Valentim Adelino Ricardo,Groppo, Francisco Carlos,Mesquita, Marcelo Ferra The Korean Academy of Prosthodonitics 2020 The Journal of Advanced Prosthodontics Vol.12 No.6
PURPOSE. To verify the influence of computer-aided design/computer-aided manufacturing (CAD/CAM) implant-supported prostheses manufactured with cobalt-chromium (Co-Cr) and zirconia (Zr), and whether ceramic application, spark erosion, and simulation of masticatory cycles modify biomechanical parameters (marginal fit, screw-loosening torque, and strain) on the implant-supported system. MATERIALS AND METHODS. Ten full-arch fixed frameworks were manufactured by a CAD/CAM milling system with Co-Cr and Zr (n=5/group). The marginal fit between the abutment and frameworks was measured as stated by single-screw test. Screw-loosening torque evaluated screw stability, and strain analysis was explored on the implant-supported system. All analyses were performed at 3 distinct times: after framework manufacturing; after ceramic application in both materials' frameworks; and after the spark erosion in Co-Cr frameworks. Afterward, stability analysis was re-evaluated after 106 mechanical cycles (2 Hz/150-N) for both materials. Statistical analyses were performed by Kruskal-Wallis and Dunn tests (α=.05). RESULTS. No difference between the two materials was found for marginal fit, screwloosening torque, and strain after framework manufacturing (P>.05). Ceramic application did not affect the variables (P>.05). Spark erosion optimized marginal fit and strain medians for Co-Cr frameworks (P<.05). Screw-loosening torque was significantly reduced by masticatory simulation (P<.05) regardless of the framework materials. CONCLUSION. Co-Cr and Zr frameworks presented similar biomechanical behavior. Ceramic application had no effect on the biomechanical behavior of either material. Spark erosion was an effective technique to improve Co-Cr biomechanical behavior on the implant-supported system. Screw-loosening torque was reduced for both materials after masticatory simulation.
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Girardi, M.,Mercurio, A.,Balestra, I.,Nonino, M.,Biviano, A.,Grillo, C.,Rosati, P.,Annunziatella, M.,Demarco, R.,Fritz, A.,Gobat, R.,Lemze, D.,Presotto, V.,Scodeggio, M.,Tozzi, P.,Bartosch Caminha, G. EDP Sciences 2015 Astronomy and astrophysics Vol.579 No.-
<P>Aims. In the effort to understand the link between the structure of galaxy clusters and their galaxy populations, we focus on MACSJ1206.2–0847at z ~ 0.44 and probe its substructure in the projected phase space through the spectrophotometric properties of a large number of galaxies from the CLASH–VLT survey. Methods. Our analysis is mainly based on an extensive spectroscopic dataset of 445 member galaxies, mostly acquired with VIMOS at VLT as part of our ESO Large Programme, sampling the cluster out to a radius ~2R<SUB>200</SUB> (4 h<SUB>70</SUB><SUP>−1</SUP>Mpc). We classify 412 galaxies as passive, with strong Hδ absorption (red and blue galaxies), and with emission lines from weak to very strong. A number of tests for substructure detection are applied to analyze the galaxy distribution in the velocity space, in 2D space, and in 3D projected phase-space. Results. Studied in its entirety, the cluster appears as a large-scale relaxed system with a few secondary, minor overdensities in 2D distribution. We detect no velocity gradients or evidence of deviations in local mean velocities. The main feature is the WNW-ESE elongation. The analysis of galaxy populations per spectral class highlights a more complex scenario. The passive galaxies and red strong Hδ galaxies trace the cluster center and the WNW–ESE elongated structure. The red strong Hδ galaxies also mark a secondary, dense peak ~2h<SUB>70</SUB><SUP>−1</SUP> Mpcat ESE. The emission line galaxies cluster in several loose structures, mostly outside R<SUB>200</SUB>. Two of these structures are also detected through our 3D analysis. The observational scenario agrees with MACS J1206.2–0847 having WNW–ESE as the direction of the main cluster accretion, traced by passive galaxies and red strong Hδ galaxies. The red strong Hδ galaxies, interpreted as poststarburst galaxies, date a likely important event 1–2 Gyr before the epoch of observation. The emission line galaxies trace a secondary, ongoing infall where groups are accreted along several directions.</P>
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