14 resultados para bebida láctea

em Biblioteca Digital da Produção Intelectual da Universidade de São Paulo


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O objetivo deste trabalho consistiu em elaborar e avaliar a aceitação de bebida mista de extrato hidrossolúvel de soja (EHS) e suco de amora (SA). As bebidas, produzidas com diferentes proporções de EHS e SA (1:1; 1:1,5; 1:2 m/m), e diferentes concentrações de sólidos solúveis (10, 12 e 14 °Brix), foram analisadas sensorialmente e seus resultados foram submetidos à análise de variância e regressão. As diferentes proporções de EHS e SA nas bebidas produzidas interferiram no aroma e na aparência das bebidas; porém, não existiu uma relação direta entre essas proporções e a aceitabilidade desses atributos. O teor de sólidos solúveis, entretanto, influenciou o sabor e a impressão global. A preferência dos provadores, tanto no sabor como na impressão global, recaiu nas bebidas mais doces, havendo uma relação direta entre o teor de açúcar e a aceitação. Todas as bebidas formuladas foram aprovadas pela equipe de provadores.

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The scope of this paper is to analyze delays in locating health services for the diagnosis of tuberculosis in Ribeirao Preto in 2009. An epidemiological and cross-sectional study was conducted with 94 TB patients undergoing treatment. A structured questionnaire, based on the Primary Care Assessment Tool adapted for TB care was used. A median (15 days or more) was established to characterize delay in health attendance. Using the Prevalence Ratio, the variables associated with longer delay were identified. The first healthcare services sought were the Emergency Services (ES) (57.5%). The longest period between seeking assistance occurred among males, aged between 50 and 59, who earned less than five minimum wages, had pulmonary TB, were new cases, were not co-infected with TB/HIV, did not consume alcohol, had satisfactory knowledge about TB before diagnosis (with a statistically significant association with delay) and who did not seek healthcare close to home before developing TB. There is a perceived need for training healthcare professionals about the signs and symptoms of the disease, reducing barriers of access to timely diagnosis of TB and widely disseminating it to the community in general.

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This study evaluates social inequalities in health according to level of schooling in the male population. This was a cross-sectional, population-based study with a sample of 449 men ranging from 20 to 59 years of age and living in Campinas, Sao Paulo State, Brazil. The chi-square test was used to verify associations, and a Poisson regression model was used to estimate crude and adjusted prevalence ratios. Men with less schooling showed higher rates of alcohol consumption and dependence, smoking, sedentary lifestyle during leisure time, and less healthy eating habits, in addition to higher prevalence of bad or very bad self-rated health, at least one chronic disease, hypertension, and other health problems. No differences were detected between the two schooling strata in terms of use of health services, except for dental services. The findings point to social inequality in health-related behaviors and in some health status indicators. However, possible equity was observed in the use of nearly all types of health services.

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Objective: One of the factors associated with low rates of compliance in the treatment for alcoholism seems to be the intensity of craving for alcohol. This study aimed to evaluate the associations between alcohol craving and biopsychosocial addiction model-related variables and to verify whether these variables could predict treatment retention. Methods: The sample consisted of 257 male alcoholics who were enrolled in two different pharmacological trials conducted at the Universidade de Sao Paulo in Brazil. Based on four factors measured at baseline - biological (age, race, and family alcoholism), psychiatric (depression symptoms), social (financial and marital status), and addiction (craving intensity, severity of alcohol dependence, smoking status, drinking history, preferential beverage, daily intake of alcohol before treatment) - direct logistic regression was performed to analyze these factors' influence on treatment retention after controlling for medication groups and AA attendance. Results: Increasing age, participation in Alcoholics Anonymous groups, and beer preference among drinkers were independently associated with higher treatment retention. Conversely, higher scores for depression increased dropout rates. Conclusion: Health services should identify the treatment practices and therapists that improve retention. Information about patients' characteristics linked to dropouts should be studied to render treatment programs more responsive and attractive, combining pharmacological agents with more intensive and diversified psychosocial interventions.

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Objective: To evaluate the effect of different chewing gum brands on the salivary pH of children with primary dentition. Method: Forty children were selected and assigned to four groups: control (no chewing gum); sugarless chewing gum; chewing gum with casein phosphopeptide-amorphous calcium phosphate; and chewing gum with xylitol. The first saliva collection was made after supervised tooth brushing for stabilization of the oral pH. Next, all children were instructed to drink slowly 100 mL of a cola-based soft drink (Coca-Cola®) and a new saliva collection was made 10 min later. Then, each group chewed on the chewing gum for 5 min and discarded it after this time. Saliva was collected again at 5, 10 and 15 min intervals after start using the chewing gum. Measurement of salivary pH was made with colorimetric test papers and a digital pH-meter. Data were analyzed statistically by analysis of variance and Tukey’s test at a 5% significance level. Results: The use of chewing gums accelerated the increase of salivary pH to considerably alkaline levels after consumption of an acidic beverage, especially within the first minutes. The highest levels were obtained in the groups of children that used chewing gums containing xylitol and casein phosphopeptide-amorphous calcium phosphate. Conclusion: Children that used the chewing gums after ingestion of an acidic soft drink presented an increase in salivary pH, with the best results in the groups that used chewing gums containing casein phosphopeptide-amorphous calcium phosphate and xylitol.

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OBJETIVO: investigar se a abreviação do jejum pré-operatório com uma bebida contendo glutamina e dextrinomaltose melhora a resposta orgânica ao trauma cirúrgico. MÉTODOS: trinta e seis pacientes adultas, (18-62 anos) candidatas à colecistectomia videolaparoscópica eletiva foram aleatoriamente divididas em três grupos: grupo jejum convencional (grupo Jejum), ou em dois grupos para receber duas dietas diferentes, oito horas (400ml) e duas horas antes da indução anestésica (200ml): grupo carboidrato (12,5% de dextrinomaltose) e glutamina (12,5% de dextrinomaltose e, respectivamente, 40 e 10g de glutamina). As amostras de sangue foram coletadas no período pré e pós-operatório. RESULTADOS: vinte e oito pacientes completaram o estudo. Nenhuma complicação pulmonar ocorreu durante o estudo. O volume residual gástrico foi similar entre os grupos (p=0,95). No pós-operatório, todas as pacientes do grupo jejum apresentaram glicemia anormal (>110mg/dl), sendo essa anormalidade 50% para o grupo CHO (p=0,14) e, apenas, 22,2% para o grupo GLN (p=0,01). No pós-operatório, todas as pacientes que abreviaram o jejum (grupo CHO + GLN) apresentaram insulinemia normal, contrastando com 66,7% no grupo jejum (p=0,02). A sensibilidade anormal à insulina subiu no pós-operatório de 32,1% para 46,4% dos casos (p=0,24). A sensibilidade anormal à insulina, no pós-operatório, ocorreu em apenas 11,1% das pacientes do grupo GLN comparado com 55,5% do grupo jejum (p=0,02). CONCLUSÃO: a abreviação do jejum pré-operatório para duas horas com glutamina e dextrinomaltose melhora a sensibilidade à insulina de pacientes submetidas à colecistectomia videolaparoscópica eletiva.

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Foi analisado o atraso na busca por serviço de saúde para o diagnóstico da Tuberculose (TB) em Ribeirão Preto, 2009, em um estudo epidemiológico, transversal, realizado com 94 doentes. Utilizou-se questionário baseado no Primary Care Assessment Tool, adaptado para avaliar a atenção à TB. Estabeleceu-se a mediana (15 dias ou mais) para caracterizar atraso na busca pelo primeiro atendimento. Através da Razão de Prevalência, identificaram-se as variáveis relacionadas ao maior atraso. O primeiro serviço de saúde procurado foi o de pronto atendimento (57,4%). Verificou-se um maior tempo na procura pelos serviços de saúde entre os doentes: do sexo masculino; com idade entre 50 a 59 anos; com renda familiar inferior a cinco salários mínimos; forma pulmonar; casos novos; não coinfecção TB/HIV; não consumiam bebida alcoólica, conhecimento satisfatório sobre TB (apresentou significância estatística na associação com o atraso) e que não procuravam o serviço de saúde próximo do domicílio antes de ter TB. Verificou-se a necessidade de capacitação para os profissionais de saúde quanto aos sinais e sintomas da doença, reduzindo as barreiras de acesso ao diagnóstico oportuno da TB e divulgação ampla para a comunidade em geral.

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Analisar práticas alimentares de crianças desnutridas menores de dois anos. Estudo exploratório e descritivo, com análise qualitativa dos dados, realizado a partir de observação participante e entrevistas. Participaram 42 sujeitos. Os dados foram submetidos à análise temática. Ao explorar as práticas alimentares dessas crianças, os temas que emergiram foram: quem prepara a alimentação e o que é preparado; como são preparados os alimentos; a rotina alimentar das crianças; onde e como as crianças são servidas. A alimentação era pouco variada; láctea, no café da manhã e lanches, e no almoço com alimentos como arroz, batata, feijão e, às vezes, carnes. Frutas e hortaliças eram escassas, e alimentos industrializados estavam presentes em todos os domicílios. Foi possível apreender o cotidiano das práticas alimentares, suas inadequações, insuficiência de alimentos, higiene precária dos alimentos complementares, influência das avós, ambiente inadequado às refeições e situação de vida das famílias.

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A fenilcetonúria (PKU) ocorre na incapacidade para transformar fenilalanina em tirosina, trazendo efeitos tóxicos para o sistema nervoso central. Tradicionalmente, no tratamento da PKU, o aleitamento materno é substituído por fórmula láctea. Este estudo verificou os efeitos do aleitamento materno como fonte de fenilalanina no desenvolvimento de crianças com PKU. Participaram dez lactentes com PKU, que iniciaram o tratamento com a introdução de fórmula láctea antes dos 30 dias e que mantiveram o aleitamento materno por no mínimo 30 dias de vida após o início dos procedimentos. Os procedimentos basearam-se em estimar a ingestão de leite materno, com margem segura da concentração da fenilalanina, calculando o volume gástrico e oferecendo inicialmente fórmula láctea, seguida do aleitamento materno em demanda livre, em todas as mamadas. O tempo de amamentação variou de um mês e cinco dias a 14 meses. Os controles sanguíneos foram semanais. Se o nível sérico da fenilalanina estivesse >2 mg/dL e <6 mg/dL mantinha-se a prescrição; se estivesse <2 mg/dL, diminuía-se a fórmula láctea em 25%, aumentando indiretamente o aleitamento materno; se estivesse >6 mg/dL, aumentava-se a fórmula em 50%. Avaliou-se os níveis de fenilalanina, aplicou-se a Early Language Milestone Scale e Passos Básicos do Desenvolvimento. Foram considerados adequados aqueles lactentes que apresentaram índices normativos em todas as avaliações. Dos lactentes, 80% conseguiram manter limites seguros da fenilalanina e desenvolvimento nos índices normativos. Há viabilidade da continuidade do aleitamento materno no tratamento de crianças com PKU desde que os níveis de fenilalanina sejam rigorosamente controlados e que os efeitos do aleitamento materno para o desenvolvimento infantil sejam verificados.

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Deep Galileo (Telescopio Nazionale Galileo) B, V and I images of Segue 3, reaching V ∼ 25, reveal that it is the youngest globular cluster known so far in the Galaxy. A young age of 3.2 Gyr is found, differently from a previous estimate of 12 Gyr. It also appears to be moderately metal rich with [Fe/H] ∼ −0.8, rather than [Fe/H] ∼ −1.7, as previously suggested by Fadely et al. A main difference in the age derivation relative to Fadely et al. comes from the consideration of subgiant branch stars in the isochrone fitting. A deduced distance of d⊙ = 29.1 kpc is compatible with the outer halo location of other low luminosity globular clusters.

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The present star formation rate (SFR) in the inner Galaxy is puzzling for the chemical evolution models (CEM). No static CEM is able to reproduce the peak of the SFR in the 4 kpc ring. The main reason is probably a shortage of gas, which could be due to the dynamical effects produced by the galactic bar, not considered by these models. We developed a CEM that includes radial gas flows in order to mimic the effects of the galactic bar in the first 5 kpc of the galactic disk. In this model, the star formation (SF) is a two-step process: first, the diffuse gas forms molecular clouds. Then, stars form from cloud-cloud collisions or by the interaction between massive stars and the molecular gas. The former is called spontaneous and the latter induced SF. The mass in the different phases of each region changes by the processes associated with the stellar formation and death by: the SF due to spontaneous fragmentation of gas in the halo; formation of gas clouds in the disk from the diffuse gas; induced SF in the disk due to the interaction between massive stars and gas clouds; and finally, the restitution of the diffuse gas associated to these process of cloud and star formation. In the halo, the star formation rate for the diffuse gas follows a Schmidt law with a power n = 1.5. In the disk, the stars form in two steps: first, molecular clouds are formed from the diffuse gas also following a Schmidt law with n=1.5 and a proportionality factor. Including a specific pattern of radial gas flows, the CEM is able to reproduce with success the peak in the SFR at 4 kpc (fig. 1).

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We use the star count model of Ortiz & Lépine to perform an unprecedented exploration of the most important Galactic parameters comparing the predicted counts with the Two Micron All Sky Survey observed star counts in the J, H, and KS bands for a grid of positions covering the whole sky. The comparison is made using a grid of lines of sight given by the HEALPix pixelization scheme. The resulting best-fit values for the parameters are: 2120 ± 200 pc for the radial scale length and 205 ± 40 pc for the scale height of the thin disk, with a central hole of 2070$_{-800}^{+2000}$ pc for the same disk, 3050 ± 500 pc for the radial scale length and 640 ± 70 pc for the scale height of the thick disk, 400 ± 100 pc for the central dimension of the spheroid, 0.0082 ± 0.0030 for the spheroid to disk density ratio, and 0.57 ± 0.05 for the oblate spheroid parameter.

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The orbits of the stars in the disk of the Galaxy, and their passages through the Galactic spiral arms, are a rarely mentioned factor of biosphere stability which might be important for long-term planetary climate evolution, with a possible bearing on mass extinctions. The Sun lies very near the co-rotation radius, where stars revolve around the Galaxy in the same period as the density wave perturbations of the spiral arms. conventional wisdom generally considers that this status makes for few passages through the spiral arms. Controversy still surrounds whether time spent inside or around spiral arms is dangerous to biospheres and conductive to mass extinctions. Possible threats include giant molecular clouds disturbing the Oort comet cloud and provoking heavy bombardment: a higher exposure to cosmic rays near star forming regions triggering increased cloudiness in Earth atmosphere and ice ages; and the desctruction of Earth's ozone layer posed by supernova explosiosn. We present detailed calculations of the history of spiral arm passages for all 212 solar-type stars nearer than 20 parsecs, including the total time spent inside armsin the last 500 Myr, when the spiral arm position can be traced with good accuracy. We found that there is a large diversity of stellar orbits in the solar neighborhood, and the time fraction spent inside spiral arms can vary from a few percent to nearly half the time. The Sun, despite its proximity to the galactic co-rotation radius, has exceptionally low eccentricity and a low vertical velocity component, and therefore spends 30% of its lifetime crossing the spiral arms, more than most nearby stars. We discuss the possible implications of this fact to the long-term habitability of the Earth, and possible correlations of the Sun's passage through the spiral arms with the five great mass extinctions of the Earth's biosphere from the Late Ordovician to the Cretaceous-Tertiary.

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We use the star count model of Ortiz & L´epine to perform an unprecedented exploration of the most important Galactic parameters comparing the predicted counts with the Two Micron All Sky Survey observed star counts in the J, H, and KS bands for a grid of positions covering the whole sky. The comparison is made using a grid of lines of sight given by the HEALPix pixelization scheme. The resulting best-fit values for the parameters are: 2120 ± 200 pc for the radial scale length and 205 ± 40 pc for the scale height of the thin disk, with a central hole of 2070+2000 −800 pc for the same disk, 3050 ± 500 pc for the radial scale length and 640 ± 70 pc for the scale height of the thick disk, 400 ± 100 pc for the central dimension of the spheroid, 0.0082 ± 0.0030 for the spheroid to disk density ratio, and 0.57 ± 0.05 for the oblate spheroid parameter.