267 resultados para Monofilament Semmes-Weinstein
Comparação entre dois fios de sutura não absorvíveis na anastomose traqueal término-terminal em cães
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Doze cães sem raça definida, com idade variando entre 1 e 6 anos e peso de 6 a 20kg, foram submetidos a ressecção traqueal e anastomose término-terminal, na qual foram testados os fios poliéster trançado não capilar e náilon monofilamento. Seis animais, cada três com um mesmo tipo de fio de sutura, sofreram a excisão equivalente a três anéis traqueais. Com 15 dias foi executada uma nova intervenção onde se ressecou o equivalente a mais seis anéis, perfazendo um total de nove. Ao final de outros 15 dias foram sacrificados. Os outros seis animais, cada três com um mesmo tipo de fio, foram submetidos à excisão equivalente a três anéis traqueais e mantidos por 43 dias. As traquéias foram avaliadas por exames clínicos, radiográficos, macroscópicos e histopatológicos. O fio de náilon monofilamento apresentou menos reação tecidual do que o poliéster trançado não capilar, promoveu uma anastomose segura e com menor chance de formação de granuloma.
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Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
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18 rabbits, New Zealand, males, adults were used for clinical and histological evaluation of repair dorsal buccal branch of facial nerve after 15, 30 and 60 days postoperatively (PO). The animals were divided into two groups for transection and 10-0 nylon monofilament epineural suture of buccal branch. In animals in Group I, the nerve was coated with protection of jejunum allograft preserved in glycerin 98% and in group II was applied epineural suture. Both groups occurred the return of movement of the upper lip from the eighth week. There was infiltrated cellular and giant cells with fibrosis unsystematic and collagen fibers of the allograft jejunum joing to the connective tissue. At 15 and 30 days of PO, the distal nerve stumps of both groups were found with degeneration wallerian and in 60 days, regenerated fibers. The repair of the dorsal buccal branch of facial nerve with the allograft wasn't significantly different between the control rabbits as to the assessment of histological and functional recovery.
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Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
A ictiofauna no monitoramento da qualidade ambiental em um distrito industrial do estuário amazônico
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Vila do Conde está localizada no município de Barcarena, Pará, Brasil. Nesta região está concentrado um importante pólo industrial de mineração, constituindo um fator de risco para a qualidade da água. Diante do exposto, este trabalho teve o objetivo de avaliar a qualidade da água no ambiente estuarino localizado no entorno de Vila do Conde utilizando a ictiofauna como bioindicador e o fígado de duas espécies de peixes como biomarcador histopatológico. As coletas do material abiótico (água) e da ictiofauna ocorreram em três áreas considerando os diferentes níveis de impacto: Zona 1, localizado no entorno do terminal portuário e industrial de Vila do Conde, considerada como alto risco de contaminação; Zona 2, localizada na ilha do Capim, na divisa dos municípios de Barcarena e Abaetetuba, classificada com risco médio de impacto; Zona 3, localizada na ilha das Onças, município de Barcarena, classificada com risco minímo por está distante das fontes de contaminação. Para todas as áreas de estudo foram feitas amostragens tanto no ambiente de canal quanto no canal de maré ao longo de quatro coletas bimestrais -, transição chuvoso para o seco (Junho 2009), seco (Setembro 2009), transição seco para chuvoso (Janeiro 2010) e período chuvoso (Abril 2010), no período de um ano de coleta. Para a obtenção dos dados foram utilizados rede de emalhar e rede de tapagem. Como forma de abordar diferentes vertentes sobre a qualidade da água em Vila do Conde, este trabalho foi dividido em etapas. A primeira etapa consistiu do uso da ictiofauna como bioindicadora (capítulo 1). Na segunda etapa foram selecionadas duas espécies abundantes com hábitos alimentares distintos, Plagioscion squamosissimus e Lithodoras dorsalis, para avaliar a saúde do ambiente através da utilização do fígado como iomarcador histopatológico (capítulo 2). Por fim todas as famílias de descritores da comunidade estudadas nos capítulos 1 e 2 foram integralizadas através do uso de índices de integridade biológica (capítulo 3). A análise da ictiofauna como bioindicadora mostrou que, para os dois ambientes (canal e igarapé), considerando as várias famílias de descritores, foi evidente a composição diferenciada entre os locais. Das 77 espécies capturadas, apenas 23 foram encontradas na zona 1. Adicionalmente, também foi observada a diminuição de organismos de grande porte. Este decréscimo foi considerado como uma resposta ecológica inicial as alterações antrópicas. A análise dos biomarcadores, feito através do estudo histopatológico do fígado se mostrou eficiente e demonstrou que presença antrópica naquela região está afetando a saúde da P. squamosissimus e L. dorsalis. O MAV (Mean Assessment Values), HAI (Histological Alteration Index) e o MDS (multidimensional scaling) mostraram claramente as diferenças entre as áreas estudadas. Nas áreas em que existe o contato mais próximo com o porto e as indústrias, as alterações foram mais severas e algumas consideradas irreversíveis para as duas espécies. As principais lesões encontradas nas duas espécies foram: o aumento do centro melanomacrófagos, degeneração gordurosa, inflamação nos hepatócitos, hepatite, congestão nos vasos e necrose focal. As alterações hepáticas observadas neste estudo foram mais intensas em P. squamosissimus que é carnívora e se alimenta na área de estudo predominantemente de camarão. Através dos índices de integridade todas as informações sobre a comunidade descritas anteriormente foram agregadas e denominadas de métricas. Para os dois ambientes (canal e igarapé), a curva de biomassa/dominância ABC mostrou que as zonas 1 e 2 apresentaram alterações, sendo estas áreas classificadas como moderadamente impactadas. Os índices BHI (Estuarine biological health index), EFCI (Estuarine fish community índex), TFCI (Transitional fish classification índex) e EBI (Estuarine biotic integrity index) foram considerados excelentes indicadores de integridade nas áreas de estudos e foram eficientes em mostrar alterações graves da comunidade de peixes na zona 1. Quanto à zona 2, já foi possível observar algum tipo de alteração no ambiente, mostrando que a contaminação não está se restringindo apenas ao entorno de Vila do Conde. As metodologias aplicadas foram capazes de detectar as interferências antrópicas na área de estudo e podem para ser replicadas em outros ambientes estuarinos. Entretanto, estudos mais detalhados e por um maior período de tempo ainda são necessários em Vila do Conde, principalmente relacionadas à bioacumulação de metais pesados nas principais espécies consumidas.
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Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)
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PURPOSE:To investigate the effects of alloxan diabetes on the abdominal wall healing of rats undergoing laparotomy.METHODS:Ninety-six male Wistar rats weighing between 200 and 300 grams, divided into two groups: non-diabetic group (G1) and another with untreated diabetes (G2). Three months after diabetes induction, the animals underwent a 5cm-long- laparotomy and 5.0 nylon monofilament suture. After the surgery, 12 animals from each group were euthanized on days 4, 14, 21 and 30 corresponding to the moments M1, M2, M3 and M4. In each moment a fragment of the abdominal wall containing the scar was removed for tensile strength measurement, histological and morphometric study. Clinical and biochemical parameters were also analyzed.RESULTS:G2 animals showed parameters compatible with severe diabetes and decreased plasma levels of insulin. The tensile strength in G2 was significantly smaller in M2 and M4, with a tendency to fall in the other two. Through light microscope, diabetic animals showed more difficulty to increase collagen density and contraction. G2 animals showed high cellularity of fibroblasts in later healing moments, with collagen thinning in M2 and M4.CONCLUSION:The abdominal wound healing in untreated diabetic animals was altered and led to a higher incidence of dehiscence and infections.
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The goal of mentoplasty is to improve chin projection. Traditionally, this is accomplished by either mandibular osteotomy or alloplastic implants. However, these procedures are not free of complications. This report describes gliding mentoplasty, a novel, simple technique for chin projection.The 12 patients in this study underwent gliding mentoplasty. By means of a 2-cm intraoral incision, a subcutaneous dissection was made in the caudal direction. The dissection then proceeded in the subperiosteal plane, leaving a 1-cm cuff of muscle attached to the bone, and advanced toward the lower border of the chin. Subsequently, the dissection was extended laterally, and the whole mental area was dissected from the surrounding tissue. Three 2-0 monofilament nylon sutures were placed in the submandibular periosteum and connected through the remaining muscle cuff to the periosteum. These key sutures allowed the submandibular region to slide forward, project the subcutaneous tissue and mentalis muscle, define the labiomental fold, and improve the pogonion projection.Gliding mentoplasty resulted in a symmetric projection of the chin in all cases. In two patients, a submandibular dimple developed, which spontaneously resolved in 1 month. No revision surgery was performed, and no tissue relapse was noted. The mean follow-up period was 24.7 +/- A 5.17 months (range 19-33 months). All the patients were satisfied with the result.Gliding mentoplasty is a simple, easy-to-perform, rapid surgical technique of chin projection that produces low pain, rapid recovery, and excellent cosmetic results.This journal requires that authors assign a level of evidence to each article. For a full description of these Evidence-Based Medicine ratings, please refer to the Table of Contents or the online Instructions to Authors www.springer.com/00266.
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We report results from a search for gravitational waves produced by perturbed intermediate mass black holes ( IMBH) in data collected by LIGO and Virgo between 2005 and 2010. The search was sensitive to astrophysical sources that produced damped sinusoid gravitational wave signals, also known as ringdowns, with frequency 50 <= f(0)/Hz <= 2000 and decay timescale 0.0001 less than or similar to tau/s less than or similar to 0.1 characteristic of those produced in mergers of IMBH pairs. No significant gravitational wave candidate was detected. We report upper limits on the astrophysical coalescence rates of IMBHs with total binary mass 50 <= M/ M circle dot <= 450 and component mass ratios of either 1: 1 or 4: 1. For systems with total mass 100 <= M/M circle dot <= 150, we report a 90% confidence upper limit on the rate of binary IMBH mergers with nonspinning and equal mass components of 6.9 x 10(-8) Mpc(-3) yr(-1). We also report a rate upper limit for ringdown waveforms from perturbed IMBHs, radiating 1% of their mass as gravitational waves in the fundamental, l = m = 2, oscillation mode, that is nearly three orders of magnitude more stringent than previous results.
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In this paper we report on a search for short-duration gravitational wave bursts in the frequency range 64 Hz-1792 Hz associated with gamma-ray bursts (GRBs), using data from GEO 600 and one of the LIGO or Virgo detectors. We introduce the method of a linear search grid to analyze GRB events with large sky localization uncertainties, for example the localizations provided by the Fermi Gamma-ray Burst Monitor (GBM). Coherent searches for gravitational waves (GWs) can be computationally intensive when the GRB sky position is not well localized, due to the corrections required for the difference in arrival time between detectors. Using a linear search grid we are able to reduce the computational cost of the analysis by a factor of O(10) for GBM events. Furthermore, we demonstrate that our analysis pipeline can improve upon the sky localization of GRBs detected by the GBM, if a high-frequency GW signal is observed in coincidence. We use the method of the linear grid in a search for GWs associated with 129 GRBs observed satellite-based gamma-ray experiments between 2006 and 2011. The GRBs in our sample had not been previously analyzed for GW counterparts. A fraction of our GRB events are analyzed using data from GEO 600 while the detector was using squeezed-light states to improve its sensitivity; this is the first search for GWs using data from a squeezed-light interferometric observatory. We find no evidence for GW signals, either with any individual GRB in this sample or with the population as a whole. For each GRB we place lower bounds on the distance to the progenitor, under an assumption of a fixed GW emission energy of 10(-2)M circle dot c(2), with a median exclusion distance of 0.8 Mpc for emission at 500 Hz and 0.3 Mpc at 1 kHz. The reduced computational cost associated with a linear search grid will enable rapid searches for GWs associated with Fermi GBM events once the advanced LIGO and Virgo detectors begin operation.
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We present the results of a search for gravitational waves associated with 223 gamma-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second, and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality gravitational wave data are available, we place lower bounds on the distance to the source in accordance with an optimistic assumption of gravitational wave emission energy of 10(-2)M(circle dot)c(2) at 150 Hz, and find a median of 13 Mpc. For the 27 short-hard GRBs we place 90% confidence exclusion distances to two source models: a binary neutron star coalescence, with a median distance of 12 Mpc, or the coalescence of a neutron star and black hole, with a median distance of 22 Mpc. Finally, we combine this search with previously published results to provide a population statement for GRB searches in first-generation LIGO and Virgo gravitational wave detectors and a resulting examination of prospects for the advanced gravitational wave detectors.
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The Numerical INJection Analysis (NINJA) project is a collaborative effort between members of the numerical relativity and gravitational-wave (GW) astrophysics communities. The purpose of NINJA is to study the ability to detect GWs emitted from merging binary black holes (BBH) and recover their parameters with next-generation GW observatories. We report here on the results of the second NINJA project, NINJA-2, which employs 60 complete BBH hybrid waveforms consisting of a numerical portion modelling the late inspiral, merger, and ringdown stitched to a post-Newtonian portion modelling the early inspiral. In a 'blind injection challenge' similar to that conducted in recent Laser Interferometer Gravitational Wave Observatory (LIGO) and Virgo science runs, we added seven hybrid waveforms to two months of data recoloured to predictions of Advanced LIGO (aLIGO) and Advanced Virgo (AdV) sensitivity curves during their first observing runs. The resulting data was analysed by GW detection algorithms and 6 of the waveforms were recovered with false alarm rates smaller than 1 in a thousand years. Parameter-estimation algorithms were run on each of these waveforms to explore the ability to constrain the masses, component angular momenta and sky position of these waveforms. We find that the strong degeneracy between the mass ratio and the BHs' angular momenta will make it difficult to precisely estimate these parameters with aLIGO and AdV. We also perform a large-scale Monte Carlo study to assess the ability to recover each of the 60 hybrid waveforms with early aLIGO and AdV sensitivity curves. Our results predict that early aLIGO and AdV will have a volume-weighted average sensitive distance of 300 Mpc (1 Gpc) for 10M circle dot + 10M circle dot (50M circle dot + 50M circle dot) BBH coalescences. We demonstrate that neglecting the component angular momenta in the waveform models used in matched-filtering will result in a reduction in sensitivity for systems with large component angular momenta. This reduction is estimated to be up to similar to 15% for 50M circle dot + 50M circle dot BBH coalescences with almost maximal angular momenta aligned with the orbit when using early aLIGO and AdV sensitivity curves.